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the projection of
|. Further, following the proof of Lemma 3.17, we find that Ai * n+i —^ 6j(£jii)++l. The formula for A2 is derived similarly. ■ For algebras of types C Q ' and D n the realization of Che generalized KdV in the form of a system (7.1) is found in exactly the same way. In the case of the algebras B^ 1 ', Ajjjlj, L and D n ) the arguments are somewhat more involved, since det A ■ 0. In the next subsection we treat the case D£ ' which is the most complicated, since Che zero eigenvalue of the matrix A is multiple (multiplicity 2 ) . 7.3.
We denote by G the scandard realization of the algebra of type Dn
corresponding
to a vertex Cm, 1 < m < n — 1 (see Appendix 2 ) . We note chat if ( a 5)eO. a€Mat(2/» — 2m, C(X, V'j). 6eMat(2m. C | * . V ] ) .
then „ ( X ) - a ( - X ) , o(X)-6(-X), P(X)
P ( - * ) . Y(M
Y<-*) •
He
a
henceforth write matrices of order 2n in the form [ £j , where Che orders of a and 6 are equal, respectively, to 2n — 2m and 2m. The operator S, corresponding to che pair (G, c m ) has the form 2 — ~7T^"('o matrices a{(x)
«.) + ^'
wher
e
A— 2 * '
(the
£orm
"t e£ is indicated in Appendix 2 ) , the
are upper triangular, and <Ji6'(2rt — 2m), 0,6'(2m)-
We shall formulate some properties of the matrix A that we need below. LEMMA 7.4.
1) The eigenvalues of A are rooCs of degree 2n — 2 in X
and zero (having
multiplicity two). 2) BftX-'))5" — Kef A © l m A . 3) The matrix P — X - W " ' is the projector onto ImA. P does not depend on X, and the first and (2n — 2m ♦ 1)-th columns of P have the form ^, — (1,0
0)' and 9, — ( 0
0, 1, 0, ..., 0)', respectively.
4) The centralizer of A in G is
lM-7m
generated as a vector space over C by the elements A"*1
and XV'F, l£Z.
Here A* for k < 0 is
defined by the formula A*-X-»'A* +,fa " n ^ r » 0 ; *t, F — -j- («.-«.!■-• + <»-«+! ,li-«+l + ( — Vp*U-m.m-m + l—\y,eu-m+i.~-m+,)—e^m.1.-m,t+l—\)m"eu-m,^m+,—
+
— J (««-«+!.!«-» + (—l)*«2»-«+l.»-«). 5) For k < 0, A** does not contain p o s i t i v e powers of X; the f i r s t and (2n — 2m + 1 ) - t h columns of A^ contain only s t r i c t l y negative powers of X. ■ We denotebyWj the s e t of columns of the form ( u l f . . . . u j n ) ' such that l , . . . , 2 n , u£(X) - u i ( - X ) for i < 2n - 2m, uj.(X) - - u i ( - X ) for i > 2n It i s c l e a r that B((X"1))*-W,(BWt, 8(W,)cJT„ X<W,)<=W, for a l l X € 0 .
K,6£((V'))
2m. We s e t
According to P r o p o s i t i o n 6 . 2 , there e x i s t s a s e r i e s T such that the operator has the form
for i 01 Wt—XW,. &<, — TSiT~'
*.--£■+A f gM-^^+gi*-*"*^. where
/ „ gjiB. LEMMA 7.5.
We shall need the following properties of T. 1) T(Wi) - Wi.
2) T(*i) - *i is a series in strictly negative power* of X.
2019
70
Proof.
Since T - e u , where UeQ, it follows that T(Wj) - W£.
Since U&J-,
it follows
that T does not contain positive powers of X while the free tern of T has the form I Q _ j . where <*j are upper triangular matrices with ones on the main diagonal. assertion 2 ) . ■
From this we obtain
We set IV,' — T - ' O ^ n l m A ) , If',"-7-"1 (W, n KerA). Since B(Qr')f — K e r A © I m A — W,BW, and A0F,)<=XP, , it follows that IT, — (W, f| Ker A)®(K, f) 'm A) , and hence IT, — W/9W,". It is clear that 2(W,')cW/, 8 (ir,*)clp," . Moreover, it is not hard to show that the operator C is invertible on wj. On w[ we introduce by means of the operator 2 the structure of a BCtD"*1))module in the same way as this was done in part 3.4. LEMMA 7.6. Any element of W^ can be represented uniquely in the form A-ij, where A 6 B((D - 1 )), and ij»j is the projection of \fi^ onto \>[. Proof.
It suffices to verify that any element of Wt{]lTn\
can be represented uniquely
*
in the form
2
ffit'PT^,,
ffcB.
where P is the projector onto Im A such that Ker P - Ker A.
This can easily be seen directly. It is only necessary to note that PTi^ ■ i^j + Ri, where Ri is a series in strictly negative powers of X (this follows from assertion 2) of Lemma 7.5 and assertion 3) of Lemma 7.4). ■ According to Lemma 7.6, there exist pseudodifferential symbols Li and L2 such that Li* ' X*2, L2 - *2 - X*l. LBiMA 7.7. Lj and L2 have the forms Rn- m and Rgp respectively (see part 7.t).
il
Proof. In analogy to the way this was done in the proof of Lemma 7.2, it can be shown that I* - —Li, and Lj - A(Pi), where /to t I.0 1. V t'*ilx>'
I
0 0 0
••• \ ?
0
V\\. • * 3
'0*3/
It remains to find the order and leading coefficient of Li and also prove that (Li>_ has the form /£)"'/i /6B. Let, say. i - 1. We recall that Pi has dimension 2n — 2m. It is convenient to go over from the matrix Pi to the matrix Px-*SPxS~l, 2eH-m+itn-m+i-\-en-m-„-m+i-r-^e„-m+i^-m
where S — £ " — «■£.._»,,,._„,—
and then in Pi permute the columns with indices n — m and
n — m + J_. We denote the matrix obtained as a result of this by Pj. It is clear that A(Pi) ■ A(Pi). Pi has the form T', -= ?{j:)-r(f-«.-«.*-«- ^-«+i,,-«+i + ««-«,..„+, + *..a+It((.m)Z) + ^
el+l./— «i,_w+i.i,_m , where the matrix q(x) is upper triangular.
deduce that (Li)+ has the form D7*'2*"1 -f £u,(x)Dl, Let £,.*.[ 4 " jl"),
From this it is not hard to
2n—2m
'—'
and (Li)- has the following structure.
where Aij are blocks of order n - m.
and A(A 2 2 ) in the form ^ D'b,-
-1
Then (Li)- *—<2oD bo.
We write A ( A l t ) in the form
^a,D'
It remains to note that A22 ■ d i a g O ,
1. - 1 . 1. - 1 (- 1)""" Xi4l,diag(I, - 1 , 1, - 1 (-1)"""",whence *(A27)) -(-1)-*-'(A <*.,))• and hence * 0 — (— l)"""* 1 ^- Thus, ( £ 1 ) - — < — I ) " - * ^ - 1 ^ ■ n m We set fi ■ i ~ rto, where aa is the same as in the proof of the lemma. The analogue of fi constructed on the basis of the matrix P2 we denote by f2* It is easy to see that Li and fi do not change under gauge transformations of €. Thus, we have constructed a mapping from the set of classes of gauge equivalence of operators (Lj, L2, fi, f2>, where f(6fl and Lj are skew-symmetric pseudodifferential symbols with leading coefficient 1 such that 2020
71
(Z,i)-"/»^-tf(. ord/., — 2rt—2m—1, ordLi=2m—I. Later (see Proposition 8.5) it will be shown that We note that the mapping from the set of classes of gauge equiv chis mapping is bijective. alence of operators 8 into the set of pairs (Li, L2) is not bijective, since, knowing Li, it is possible to recover f^ only up to sign. In part 7.1 an assertion was formulated that the generalized KdV corresponding to a classical Kats—Moody algebra distinct from A^ 1 ' reduces to the system (7.1), where Ai and A2 are expressed in terms of fractional powers of L1L2 and L2L1. In the case D ^ 1 ' this asser tion needs refinement: the generalized KdV in question must correspond to an element «63. having the form u —2*'A 3 '*', * ^
(we
n
°te that in all cases except D n
any element of
3
t
has this form; see Appendix 2 ) . Proposition 7.3. Suppose the operator fi satisfies Eq. (6.5), where it — y b ^ i v * 1 , /-o Then L x and L2 satisfy the system (7.1), where 4 , — (Mt).,
Mx~* — ^ftj^i,)*^ 5 .
bfC.
x
^ 2 — — 2*/
The proof is entirely analogous to the proof of Proposition 7.3. However, because the ]>i are not entirely explicitly defined the proof of the formula Pt'^i " Aj/i^i is nontrivial. It is based on the following lemmas.
LEMMA 7 . 9 . DrWtfcW/t Proof. [i.e.,
DfWfczWf.
We denote by V t the operator on W acting according to the formula V t (w) - D t *w Since [V,. fi|—0 , it follows that \TvtT~l, fio]— 0.
V | — j f — 9 ( a ) * ]•
From this it is
easily deduced that [TV t T~ , A] " 0 , and hence the kernel and image of A are invariant under TV t T~ l . Using assertion 1) of Lemma 7.5, we find that T^,T-[ (Wt)czXPt whence the lemma fol lows. ■ LEMMA 7.10. Proof.
(M-ii) + - M+'i^ for any
(M^t)^—
M+^t
Afg5((£>"')).
— (^♦(—Af*-ifri)» —(Af.-^( —Af + -^j) + , where
$,—ty— $ , . It remains to
verify that (fi'9()„ — 0 for > < 0 , ( £ / ^ - 0 for j a O . It suffices to prove that ( f i o T ^ — 0 for y < 0 , ( Q o ^ r ^ M 0 for j > 0. We have 7*9,— PT$t, Tyt-- (E — P) T$t, where P is the same as in Lemma 7.4. Therefore from assertion 2) of Lemma 7.5 and assertion 3) of Lemna 7.4. it fol lows that (7*9,),— 0, (7*9,).,—♦,. Since T^eKerA, the equality (T*i)* - 0 implies that (flo'T"*]),.— 0 for j > 0. The equality (So^if,),,, — 0 , where j < 0, follows from assertion 5) of Lemma 7.4. ■ The formula D ^ * ^ ■ Aj/^£ is induced from these lemmas as follows. It( follows from Lemma 7.9 that Dt»ijii ■ ^ ( D t / ^ i ) . where *{:Wi -»■ W^ is the projector with kernel W^. By definition, 0„ Df-9,_—j*^
9/——(J*9()^ where J* — 2
*/"'A2/*'7".
Since
J # ( W V ) — 0 , it follows that J*^ —
•s*^,. Since ■&$,— — Af*9, (see the proof of Proposition 7.3), we have plying now Lemma 7.t0, we find that Dt*£i • *i(A£*iJii) ■ A i * ^ . If u has the form ^
btA7i*1
Dt$t
—ft*((Aft • 9*)J*
Ap-
, then, as before, the corresponding generalized KdV reduces
/ to the system (7.1), but unfortunately in this case we do not know an explicit formula for Ai and A2> In the simplest nontrivial case Ai - f 2 n _ 1 f i , A2 " fiD~ l f2. 7.4. In part 7.1 a rule was formulated for determining the types of the operators Lx and L 3 corresponding to a given pair (G, c m ) , where G is a classical Kats—Moody algebra and C Q is a vertex of its Dynkin scheme. However, in the case of algebras G of low rank and also in the case where c m is an extreme vertex this rule cannot be understood literally. We there fore present a table (Table 4) in which for each pair (G, Cm) the types of the corresponding tftf
4t(
tef
operators Li and L2 are indicated. In t h i s t a b l e i t i s understood that P0—•£>, Qo—«1. /?©—D"1. The v e r t i c e s of the Dynkin scheme of G are numbered as in Table 2 . It was noted in part 7.1 that i f Li and L2 s a t i s f y the system ( 7 . 1 ) , then the operator L—LfLi s a t i s f i e s the equation dL/dt - [ A l t L ] .
It i s clear that i f one of the operators
2021
72
TABLE 4
<£
•n»f
*K-t " » t «?
»»I
> —n>1 »
CS'
eff *
»>i —■
»Si »><
c«
kt
0«m«n 2«m«n
'«-«» «n-m
m-V
On ^n-m
><m<* m-V
0<m
<•!
tm »m •o *m
%
«. •m
•n »0
«. •« *w
«n-m B »-m
«m
Pn-m
Li belongs to type Po, Qo, or Ro (this condition is almost equivalent to C Q being an extreme vertex) the system (7.1) is equivalent to this equation. In conclusion we consider conservation laws for generalized KdV. In analogy to Proposi tion 3.20, it can be proved that in the case of classical Kats-Moody algebras distinct from D^ ' the densities of the conservation laws Hi considered in Proposition 6.6 up to constant multiples and addition of total derivatives are equal to res ( L i L j ) ' ^ , where k - ord(LiL2). In the case of D n '> the situation is as follows. We write the element W € C ~ ( R , 8")- considered A/A-'"+1l + 2sA _l, ' + "/ : '.
in Proposition 6.6, in the form H—2 '~°
"here
A„ gfiB
(see Lemma 7.4).
—
ti+i
Then up to a constant multiple and addition of total derivatives hj is equal to res (£,£,) * . Unfortunately, we do not know a general formula expressing gi in terms of L j , L j , fi, fz (the f£ are the same as in part 7.3). We note only that up to a multiple and total derivatives go is equal to fif2. 8.
HAMILTONIAN MANIFOLDS
M(9)
In part 6.5 for any semisimple Lie algebra 9 we defined a manifold A (9) equipped with two Hamiltonian structures. Moreover, jf(|I(A)) is by definition the manifold denoted in part 3.6 by
Jt.
We denote by
M(|t(*)) the set of operators of the form D'+\u.,D',
u£B*
In
part 3.3 we constructed a bijection F:JC(H(k))*M(tl(k)). and in part 3.7 it was ahown that the first and second Hamiltonian structures on JT(|I(*)) go over under the mapping F into the cor responding Gel'fand-Dikii structures on A1(|I(*)). In the present section for each classical simple Lie algebra 9 we define a manifold M(9) consisting of scalar differential [and in the case € ) — »(2/i) pseudodifferential) operators of special form' and a bijective mapping F:JC{9)-*M(9). Moreover, the Hamiltonian structures on M(9) corresponding to the first and second Hamiltonian structures on A (6) will be found. We recall (see part 6.5) that the definition of the manifold Jf(«) and the Hamiltonian structures on it involves the Weyl generators of 9 , an invariant scalar product on 9 , and an element e of the center of the algebra a. For all classical algebras 9 we use the Weyl generators presented in Appendix I and the scalar product (X, Y) - tr (XY). We shall indicate the element e each time. 8.1.
We begin with the simplest case
«-•<(*).
It is easy to see that Jf(«l(*))cJf(•'(*)).
We set M("(*))-{i)' +Vu,£)'|U,eBo • It i« clear that the bijection Uf(|l(*)) — M(«<(*)) consi-o I tructed In part 3.3 map* Jt (•'(*)) onto M(•!(*)). We denote by {•, -)i and (•, - h the Poisson brackets on M(»>(*)). corresponding to the first and second Hamiltonian structures on •*(»'(*)) (as the element e in the definition of the first Hamiltonian structure we take the matrix e ^ k as in Sec. 3 ) . We shall find the explicit form of these brackets. For this it suffices for any integral symbols JT, Y£B, ((O"')) to find {/*. /K}i and {lx, lr)%, where /jr:M(»l(*))-»C is defined by the formula Ixjf-) — Tr (XL). It is not hard to see that if a and * are functionals on jT(|l(*)) and m and * are their restrictions to •#(•!(*)), then fi, ^}, and fi, ^ } 2 are equal to the restrictions to Jt(»!(*)) of Mikhallov [65] pointed out the connection between the types of scalar differential operators and the types of the classical simple Lie algebras. 2022
73
the functionals {9. 9}i and {9, if),. It therefore follows from Theorem 3.22 that {lx. M i and (/*. M J « e defined by formulas (2.16), (2.17). 8.2. Now let «—e(2n+l) —(i46«l(2n+l)|o(^)=i4} , where a is the automorphism of il(2rt + l). given by the formula o(A) — — dlag(l, — 1 l)-i4r-diig(l, — 1 1). The Borel subalgebra in 6 will be denoted by lg, while t denotes the set of all upper triangular matrices (we recall that »g — >n®)- The meaning of the notation Hq, and • is similar. Since l^ci, '$cr», while the elements I for the algebras 8 and jl(2rt+l) coincide (namely, /-= V «,+1,,) , there is the i—i
natural mapping ?:Jl(9)-*Jl(il(2/i + 1)). Since o(») —», o(«) —», o(/) —/,it follows that o in duces a mapping .if (al(2/l+I))-*-*(l<(2/.+I)), which we also denote by a. LEMMA 8.1. f maps .* (8) in one-to-one fashion onto the set of elements of jf(gt (2/t + 1)). invariant under o. Proof. We denote by I, the set of matrices (aag) such that a0g » 0 for S — a * i. For any i > 0 we choose a vector subspace V,
«/./+. I- We set
V —©V,. It is clear that »a = [/, »8]SK», where V°— {A&/\o(A)~A)
. Ac
cording to Proposition 6.1, it is possible to replace JT(9'(2rt+1)) by C~(B/Z, V) and Jf(8) by C*(R/Z, V a ) after which the assertion of the lemma becomes obvious. ■ We henceforth identify Jt(>(2n + \)) with its image in Jt(il(2n +1))- We recall that the bljective mapping constructed In Sec. 3 F: JT(|I(2n+ 1)) —Af(«I(2n +1)) assigns to a class of gauge equivalence of the operator d/dx + I + q the operator L ■ —(A(P))*, where P ■ I ♦ q ♦ diag (D, 0,... ,D) (see part 3.3). If q is replaced by o(q), then P is replaced by—diagO, —1 1)-PT-diag (1, —1 1), and hence (see Lemma 3.13) L is replaced by -L*. Thus, the mapping icoF-':/W(l<(2rt + l))->-Af(l<(2)t +1)) takes L into -L*. From Lemma 8.1 we therefore obtain the following result. dtr
Proposition 8 . 2 . {£6Af(«'(2tt + l)) | £ • - - ! } Remark 1. It is verse to it are given
F maps Jl(>(2«-)-l))
in one-to-one fashion onto the s e t M(• (2r»+1)) =-
. clear that the mapping F:JC(»(7n-\-\))-*MlfC2n-\-\)) by differential polynomials.
and the mapping in
Remark 2. Let 4 be the Cartan subalgebra of «(2*i-f 1). Composition of the Miura trans formation u:C~(R/Z. !))—■£(o(2«+l)) and the mapping F:Jt(>C2n + l))->-M(°(2n + \)) takes the matrix dlag(/, /„, 0. — / . —/,) into the operator I — (D + /,) • • • (D + f„)D(D—/„)... (D- fO. We denote by {•, *}i and {•, »}2 the Poisson brackets on Af(»(2fi-f-1)), corresponding to the f i r s t and second Hamiltonian structures on J[{*{2n+1)) [for e we take (e x 2 n * e 2 2n+i)/ 2 ) . We shall find the e x p l i c i t form of these brackets. For t h i s i t s u f f i c e s for any i n t e gral symbols X, K6flo((D"')) to find Ifx, Mi and (/», I,), , where lX-M(»(2n+1)) — C i s defined by the formula lx(L) = 7t (XL). Moreover, i t may be assumed with no l o s s of g e n e r a l i t y that X* - X, Y* - Y [indeed, the formula Tr Z* - -Tr Z v a l i d for any ZtBMD'% implies that i f L* - - L , then T r ( X £ ) - T r ( - ^ ^ - - Z . ) J . Proposition 8 . 3 .
Let £ C M(»(2»+1)). X, Y^B^D-% ordA'<0, ordK<0. X'-X,
Y'-Y
. Then
l'x. lrh(l)-T'C-(YDX-XDY)), Vx. lrh{i-)-Ti((LYUX-XHYL)J. We note that since L* - -L, X* - X, Y* - Y, it follows that lt(L-(YDX (LYDX), Tr lif.Y)JJC - XL (YL) J - 2 Tr ((LY).LX).
(8.t) (8.2) — XDY)) — 2Tr
x
Proof. From formula (3.17) it follows that if the functionals I,, l,:Jl(«'(2n+l)-*C are invariant under a and Z\ and Z2 are their restrictions Co Jf(*(2n-(-1)), then {'1, £2)2 is equal to the restriction of Hi, £2)2 to JT(• (9n +1)) [to see this it suffices to note that if o(q) q, then for a suicabl* normalization of Che gradienc o(grady,) — grsd,/, , whence gttdfl,gC"(R/Z, O(2B+J1)) and hence grad,/,—grtd,/, ]. Therefore, if 9, and 9, are functionals on yW(|!(2n + 1)) such that ?,(£) —9,( — £•) and 9, and 9] are their restrictions to Af (• (2»+1)), then 2023
74
{9i. ^jk i s e qu«l to the restriction of {9i, »,}, to jW(»(2n + l)). Setting now *,(£)— Jt(XL), 9,(i) —Tr(Ki) , we obtain (8.2). Since the element e for the algebras >(2n-fl) and (1(21 + 1) do not coincide, equality (8.1) cannot be proved in a similar way. It is not hard, however, to deduce (8.1) from (8.2) by arguing in the same way as at the end of the proof of Theorem 3.22. Here we use the following simple assertion: if to the operator d/dx ♦ 1 ♦ q(x), where q(x) is an upper triangular matrix in »(2« + l), there corresponds LGM(»(2n+\)), then to the operator d/dx ♦ I ♦ q(x) — e there corresponds L ♦ D. ■ 8.3. We consider the case 6—»Pf2l)—Me»l(2«)|o(.A) —.A)i where o is the automorphism of |I(ai), given by the formula a(A) — — ateg(l. — 1 1, — l)-i*r-dlag(l, — 1 1, — 1 ) . Lemma 8.1 also holds in this case. In particular, JT(sv(2n)) can be considered a subset of Uf(|l(2l))> The following assertion is proved in the same way as Proposition 8.2, 8.3 [and even somewhat more simply since the elements e in the definition of the first Hamiltonian structure for the al gebras ff(2n) and i<(2n) coincide]. Proposition 8.4.
1) The mapping F:UT(«l(2ri)-»A1(|I(2n)) maps Jf(»>(2n)) in one-to-one fash-
ion onto the set At(•»(2*) — (i6M(l'(2n)) | £• — £). The mapping F: Jl (•»(2rt))-<-.M(»»(2n)) and the mapping inverse to it are given by differential polynomials. 2) Let $ be the Cartan subalgebra of <>(2R). Composition of the Miura transformation u:C~(R/Z, !})-*■ JH*i(2n)) and the mapping F:JHn(2n)) — AHt (2n)) takes the matrixdlag(/ /«• _/ - / , ) into the operator !-(£> + / , ) . . . ( D + /„)(£>-/.)••• (£>-/.)• 3) We denote by {*, *}j and {*, *)2 the Poisson brackets on M*>(2n)), corresponding to the first and second Hamiltonian structures on uT(*9(2n)) (for e we take eiv2n)> For any integral symbol X6B0(D-i)) we define 1, : M(«»(2n))->-C by the formula /,(L) -ir(XL). Then for any Z.€M(*p(2n)) and any skew-symmetric integral symbols X, Y^B0(D~1)) the following equali ties hold: {'x. /r},(£)-Tr(£.IK,
X])-2-Tr(LVX).
Vx.lrhM-TH(t-r)A*-XL(n).)-2TT((Lr).LX). Remark. The analogue found in [27, 44] of the interpretation of the first Gel'fand— Dikii bracket as the Kirillov bracket also holds for the first Hamiltonian structures on Af(*»(2n)) and M(o(2n+1)). In the case »(2n) it is necessary to consider the Kirillov bracket for the Lie algebra of skew-symmetric integral symbols. In the case e(2n+l) it is necessary to consider the Lie algebra of symmetric integral symbols with the unusual commu tator [X, Y]-XDY-YDX. 8.4. We consider, finally, the most difficult case C«»(2n). We denote by M(o(2n)) the set of pairs (L, f ) , where ftBi, IeBc((£)-i)), !•- — L, L.-fD-'f, ordI-2rt— 1. and the leading coefficient of L is equal to 1. In part 7.3 (see the proof of Lemma 7.7) we essentially con structed a mapping F : jT(o(2n))->M(»(2n)). Proposition 8.5. polynomials.
1) F is bijective.
The mappings F and F - 1 are given by differential
2) Let t) be the Cartan subalgebra of *(2n). Composition of the Miura transformation u:C"(R/Z, $)-jr(o(2n)) and the mapping F:J*(o(2ri|)-*Af (»(2n)) takes the matrix dlag(/, /•• -/. -ft) into the pair (L, f), where I_(D + / , ) . . . (D + /„) D-'{D-f.)... (D-/,). / (-1)-W>(1), where P = (D + / , ) • • • (D + /»). 3) We denote by {•, • )i and {•, • >2 the Poisson brackets on M(»(2n)), corresponding to the first and second Hamiltonian structures on UT(°(2n)) [for e we take ( e 1 ( 2 n - 1 + e 2 , 2 n ) / 2 ] . For any integral symbol X£Bt((£>-')). such that X* - X we define lx:M{>(2n))->C by the formula U(£. /)-Tr(A'I). Moreover, for any s6B0
we
set X,(£, / ) — \ S{x)/(x)dx.
Then
(lx.lr)i(L.f)>-,n<(LYDX). Vx,K)>-0,
{K. U — j - $ s(x)t"(x)dx;
{'x. lrh(L, / ) - 2Tr ({LY),LX), {).., /,},(£, f)-Tt(LXfD-'s),
^..M 8 (i./)-T T '(" D " J )2024
75
We shall only outline the proof. Assertion 2 ) , of course, is proved by direct computa tion. The difficulty in the proof of the remaining assertions as compared with the analogous assertions for o(2n+I) (see part 8.2) is connected with the fact that the matrices I for o(2n) and gl(2n) do not coincide, and hence there is no natural mapping Jf(o(2n))-*-Jf(gt(2n)). In order to overcome this difficulty, we define a new manifold Jf', in which Jf(e(2n)) is imbedded in a natural way. For this we consider operators ft of the form
*-£
+ r+i. ?ec-(R/z,e),
(8.3)
where I is the sum of the Weyl generators Xi of the algebra o(2re) (see Appendix 1) and 9 is a set of matrices (aag) of order 2n such that Sag - 0 for a > B and (a, 8) * (n ♦ 1, n ) . We denote by 91 the set of matrices (a a g) of order 2n such that a 0 g ■ 0 for o > 8 and, more over, aa [,*! - 0. It is easy to verify that if 2 has the form (8.3) and 56C"(R/Z, S ) , then esie~s also has the form (8.3). Such transformations we call gauge transformations. The sec of classes of gauge equivalence of operators 2 of the form (8.3) we denote by JL' . We recall that • (2n) =» {A&S (2/t)| a (A) =- A \ , where o is the automorphism of «<(2n), given by the for mula o(/4)--diag(1. - 1 (-1)"-'. (-!)"-'.(-')" 0 <*r.di«g(l, - 1 (-If1. <-ir'. (-1)* !)• Since o(/)=«/. o(8)«=$, o_[3i)»=9l, it follows that c induces a mapping Jt'-*-JC', which we also denote by a. In analogy to Lemma 8.1 it can be shown that the natural mapping from Jt(°ipi)) into the set of elements M', fixed under a is bijective. We denote by M' the set of qua druples of the form (L, f, g, h) , where /. g, A(=fl0. and L is a pseudodif ferential symbol of order 2n — 1 with leading coefficient 1 such that L_ ■ f(D + h) - 1 g. We define the mapping F':Jt'-*M', assigning to the class of the operator d/dx ♦ I ♦ q(x) the following quadruple (i./.g.*): «) i - A ( P ) , where P= dla?(D, D
D) + q + f,
b) *=--£-(?„. . + ?„+i. .+ i)-?.+l. . -
-r-tjit. n+i, where qi,j are the elements of the matrix q; c) let Aij be the same as in the proof of Lemma 7.7; we write i ( * n ) in the form 2 a , ( & + *)'• •i«t
d*r
and
M A 2 2 ) in the form 2 ( ^ + *)'*j • i
'
then /S-X^OQ, g — ( — I f i * ^ . It is not hard to verify that F' is well defined and is bijective, whereby the elements of the matrix q corresponding to the quadruple (L, f, g, h) can be chosen in the form of differential polynomials in f, g, h and the coefficients of L; the mapping F'-o-(F')~':M' -► M' acts by the formula (L, f, g, h) ■» (-L*, g, f, - h ) . From this we obtain assertion 1) of Proposition 8.5. On Jt' we consider the Poisson bracket given by formula (3.17) and carry it over to M' by means of the mapping F'. For any integral symbol X^BQ((D':)) we define lx:M'-*C by the formula lx(L, f, g. A) — Tr (XL). Moreover, for any s£B0 we define functiooals
,(•) _ s , and hence •, induces a mapping 5,:Jf (•)-► JT(I). It can be shown that if « is a simple algebra, then a, preserves the scalar product, and hence the mapping S T is Hamiltonian relative to the second Hamiltonian structure (relative to the first structure it is almost Hamiltonian). Among the Dynkin schemes of the classical Lie algebras An and D Q have nontrivial automorphisms (see Table 1). It is not hard to verify that to the nontrivial automorphism of An there corre sponds the mapping Af(»l(ii+l))-*/to(»l(B+l)), acting by the formula L-*(— l)**'!*. while to the automorphism of the scheme of Dn changing the places of en and cn-1 there corresponds a map ping M{»
* are invariant, but they are only well defined for WZNW solu tions in that neighbourhood of the identity where the Gauss-decomposition (2.9) is valid. Of course one could cover G with a finite number of patches and introduce locally regular Toda fields on them. These local fields would be related by some group transformations on the intersections of these patches and together they would define a global Toda field. Fortunately there is a simpler and more direct way to find globally well defined quantities which reduce to the local Toda fields in the neighbourhood of the iden tity. Consider some (d-dimensional) representation of G and choose a basis such that the Cartan subalgebra is represented by diagonal matrices, and the Lie algebras of N and N are represented by upper and lower triangular matrices, respectively. Then, because a. and /? in (2.21) are upper and lower triangular matrices, respectively, with l's in their diagonals, it follows that the lower-right sub-determinants + i ^ v j ) exp(Xy*oJ, l+ -QU + nQA) + DA + QDQ -(4>+n£2) U + Q ). Note that the in variance of J* under the residual gauge transformations can be explicitly checked thanks to Ad(Al,Ql)Ad(A2,Q2)=Ad(Al -(i.-x.)-'(i,-i.)- , C. / .(*), n + 1 describe the multicritical behavior of ZH symmetric statistical systems. In particular, the anomalous dimensions (1.3) (///') with the anomalous dimensions (1.3) all values of parameters wk{l/i) corresponding to thesefieldscan be obtained from Eqs. (5.6), (4.9), and (3.7). Note, that identification (5.8) breaks the conservation of two "Z„ charges" (5.3). However, one Z„ charge always survives. This Z„ charge for the models [Z„(p)] can be described in the following way. Let p = k (mod n); then the operator algebra of models [ZM Jexpf/kS W2 J fl ) + i J ^ I (,tC modulo the BRST operator. This completes the proof of the lemma. On the other hand, the total energy-momentum tensor is expressed as 7™"(z) = TFF(z) - {QBRSTMz)db(z)} *+l TFF(z) = - $(d (z), j2k a0 = +■ 4 2 Cv is decomposed into subspaces with definite 1/(1) charges with respect to — idcp, r.s + can be written as a unique linear combination E' = !«,«,-, where the ni are non-negative integers. We call ht a = E,7J, the height of a. Obviously, simple roots have height 1 and all other 0 since d^N e C^ + / = 0. Therefore ^ = d£N and hence a rf-coboundary. Suppose that this is the case for all positive orders > n. Then if ty has order n, again dQtyn = 0 and by the lemma i/f„ = d0gn for some £n e C*. But then i// — d£n is a d-cocycle of order n + 1, which by the induction hypothesis is a d-coboundary. Hence by induction we find that all J-cocycles of positive order are rf-coboundaries. Exactly the same argument shows that for h ¥= 0 allrf-cocyclesare d-coboundaries since d0 has no cohomology here. This proves the first of the two isomorphisms of the theorem. Suppose now that h = 0. In this case deg is bounded above by zero. If ^ is a d-cocycle of order zero then if/ = t/r0 and dQil> = 0. By the lemma it is d0-cohomologous to some multiple of the vacuum, that is, t/r = aflQ + d0€0 for some £0 e CQ. But djt;0 G C° = 0 so that i/> is actually d-cohomologous to some multiple of the vacuum. Suppose now that this is the case for all d-cocycles of order >p (p < 0). Then if i/f has order p, so that if = *l>p ® • • • ® a(z) = E m € Z ^ ( m ) z " m " ' 1 C ( 2 : ) = E m e z V ' a ( m ) 2 _ m , a £ A+, and their derivatives. The differ ential d acts on Ck(g) and preserves the structure of Lie algebra. Therefore the cohomol ogy (B]Hlloc is a Lie algebra. It was proved in [2], that Hkloc it is spanned by Fourier coefficients of local fields from Hk. The Lie bracket in Wk(g)ioc = Hkloc is defined by the singular part of the O P E in Wk(g). Note that for any positive-energy module M over g we may consider the complex M ® A with respect to the differential d. The cohomology (&Hk{M) of this complex is a module over Wit(<7)ioc- This defines a functor from the category of positive-energy representations of g to a category of Wk(g)\oc—modules, which is studied in detail in [6]. Note that H3k = H3k{Vk). In the conclusion of this Section I want to explain a finite-dimensional counterpart of the definition of W-algebra. Let o be a Lie algebra, and 6 - its Lie subalgebra. Let X : b —► C be a character of b, which defines its one-dimensional representation C x . We can ask the following question: what is the (maximal) algebra, which acts on the space ( M ® C x ) k for any g—module M? Here (M ® Cx)h denotes the space of invariants of the 6—module (M ® C x ) , which is the subspace of all vectors in M, such that any element x £ b acts on them by multiplication by — x{x)- This algebra is called the Hecke algebra, associated to the triple (a,b,\)Note that the algebra 7iq, which is usually called the Hecke algebra, appears in a similar context: when a is replaced by a finite group of Lie type over the finite field of q elements, 6 - by its Borel subgroup. One possibility to find this algebra is the following. Recall that the space of 6—invari ants of a module N coincides with the 0th cohomology of 6 with coefficients in N. This cohomology is defined as the cohomology of the complex N ® A(6) with respect to the standard (BRST) differential dat. More precisely: let {e,-, i £ / } be a basis in 6. Introduce the Clifford algebra Cl, generated by fa, rp', i € / with the standard anti-commutation relations: [fa,ipj] = Sij. Denote by A(6) its representation, generated by the vacuum vector, annihilated by all fa: this is the exterior algebra of the dual space to 6. We have dat = J2ei1l>' — l ^ E ^ j W ? ^ ; * ! where c£- are the structure constants of 6. If N = M ® C X , then this complex is isomorphic to the complex M® A(6) with respect to the differential d = d,t + £ x(ei)i>i- The algebra of all endomorphisms of the complex is U(g) ® Cl. The Hecke algebra consists of such endomorphisms of this complex, which commute with the differential d. The operator D = [d, •] - the supercommutator with d, defines a differential in U(g) ® Cl. All elements of U(g) g) Cl, which commute with d, act naturally on the cohomologies of M ® A(6) for any a—module M, and those of them, which are of the form [d, x] for some x, act by 0. Therefore the cohomologies of this complex with respect to D, i.e. the quotient of the kernel of D modulo the image of D, act on the cohomologies of M ® A(6). The cohomologies of U{g) ® Cl form an algebra. The 0th cohomology is the Hecke algebra we were looking for. Here is an example. Let a be a simple Lie algebra g, b - its upper-nilpotent subalgebra H = ®H°(£,nd'+1), which sends (P,() £ T'Ma{£) to ( A j ( £ ) , . . . , A r (£)), where A< is a primitive generator of the algebra of G—invariant polynomials on the dual space g* tog; A,- is of degree dj + 1 , and it sends £ to H°(£,Cld,+l). The miraculous fact is that the dimension of H is equal to the dimension of the moduli space, that is to one half of the dimension of T"MG(£)Indeed, the dimension of MG{£) is equal to (g — 1) dim G, where g is the genus of the curve £, and the dimension of 7i is equal to (g - 1) £(2 /PiP. u {0} which is 0 outside Nk- and q>': Nk- ->IP,,' is \W\ to 1. Here ~ °/and characterize the set N + of " + "-nondegenerate weights. (N ± 4= 0 only if p' ^ h, the Coxeter number.) The map module F±(M) in terms of residues of affine characters (Pro position 3.2.3 and Theorem 3.2). The key fact here is Proposition 3.2.2 which asserts that functors F± map positive energy g-modules to positive energy W * (g)modules. In Sect. 3.3 we prove some properties of the W-algebras using representa tion theory. Using this and the fundamental irreducibility Conjecture 3.4 ± , we derive in Sect. 3.4 the character formula for F±(L(A)), where AeNk±, and show that these W* (g)-modules are parameterized by the set 7P>P-. In Sect. 3.5 we state conjectures on resolutions, which, in particular, imply the irreducibility conjecture. Finally, in Sect. 4 we use results of Sects. 1 and 3 to derive fusion rules for the W-algebra in the case of simply laced g. It turns out, in particular, that if | W+ \ is relatively prime to p or to p' (which holds for all k in all cases except for g of type An, where n is not a power of a prime number) then the fusion algebra for Wf (g) is isomorphic to s/p~h(g) s/(~h or to $t\~k / p u be the map defined as follows: q>-(A) = q>f{A)ifAePk9, + := q>~ "/corresponding to the quantization of the second Drinfeld-Sokolov reduction. Consider the set N\ :=f-l(Ni) = {A e Prk\ )mo IPiU is \ W\ to 1. (b) The same statement holds for (p +: N\ -> /„_„. Proof. Let A = y.(k-(u(1.5.2) we have: p'-= tp+uVy 6 W by the condition yf(RM) <= A X". This gives us a map 0, a(z):) ■ We have to show that [r(z),d + ] = 0 . a(z): is an energymomentum field with central charge cx= (z)d the (bi)grade (0,0) piece of T is given by T<°'O) = i ( 9 ^ 0 ) + a o ^ , where a0 = 2 v of a freefieldcf>. , G++ = 2ii JG~ = ( J - J ° ) + (J°J-) + 2{k + 3)dJ~ - 2d(f>J- , T 0, [c] = (m, -m + 1) fore e 77mf, m > 0 and [t] = (0,0). Through this A acquires a double grading: 2 = Qo(Qi'P). It is equally triv ial to verify that d\ = 0. The o^-cohomology gives the next term in the sequence, and so on, until the sequence stabilizes (i.e. the derivation operator van ishes). Applying this to H'(A\Q), using eq. (12), one finds that £1 is represented by*3 £ | - A /7ke, ))(z) = ! « ? • , 2 ) . 0 has the consequence that for y > 1 the generators V£ do not have definite conformal spin. This is because, as can be seen from eq. (2.1), the commutator of Lm with K„; will then give not only the leading order g%Km, n)Vj,+n term appropriate to a generator of conformal spin (;' + 2), but also lower-order terms of the form g%iim,n)V,>,-+2nr. As a general rule, any terminating saalschiitzian 4F3(l) series can be recast into the form of a Wigner 6-j symbol, at least formally. The general correspondence is given in eq. (A. 14); after some manipulation one finds for the case of present interest
is the set of all operators of Bo[Dl of the form
£ > ' + « Z ) » + £>»« + ( ^ - 2 B » J D
S
+ D»(-£ —
2u") ♦ vD + Dv. 9.
EXAMPLES OF GENERALIZED KdV and mKdV EQUATIONS
In this section we present some examples of generalized KdV and mKdV corresponding to classical Kats-Moody algebras distinct from »!(*, C[X,X"']. The generalized KdV are hereby considered as equation for «**° (see part 6.2). The form of e°™ is chosen so that the sim plest equation of the corresponding series has minimal possible order. Table 5 is devoted to generalized mKdV for which the type of the algebra G and the Hamil tonian H is shown that leads to the simplest equation of the series [the generalized mKdV corresponding to the Hamiltonian H(ui
uk) has the form -37^~"s—1—,i«], .■.,* ]•
We further indicate the Hamiltonian for mKdV corresponding to D ^ 1 ' and having the form ■ 3 P ~ I ' ( T . £]. where F is the same as in Appendix 2. H in this case is equal to —4(u,'tf4'-fU.'tt>tt4— Ut'U,U,
— I^UJUJK,).
Examples of generalized KdV are presented in Tables 6 and 7. Table 6 is devoted to equations corresponding to pairs (G, c m ) such that after removal of the vertex c m of the Dynkin scheme G decomposes into unconnected points. In this case the algebra 9 (see part 6.1) is isomorphic to the direct product of several copies of sl(2) . Therefore, for suitable choice of the "coordinate system" ui,...,u K the generalized KdV corresponding to the Hamil tonian H and the second Hamiltonian structure has the form
- £ - _ A,(D«+2(«1D + 0«1))-Si7. '-1
*•
<9-'>
where X|£C. We mention that the operator D 3 + 2 ( U J D + Du^) corresponds to the second Hamil tonian structure on M(*l(2)), and the occurrence of the factors Xi is connected with the fact that the isomorphism 6^.»1(2)X •• • X**(2) does not preserve scalar products. The simplest example of an equation admitting the form (9.1) is the KdV equations for which k - 1, X\ - 1, H ■ uf/2. In Table 6 for each pair (G, c m ) of this type the factors Xi and Hamiltonian H are presented that correspond to the simplest equation of the series. The simplest generalized KdV corresponding to algebras of types A?*, A™, B"* are pre sented in Table 7. We recall that each generalized KdV possesses the Lax representation ^ L — jj^c-ii^ gcM], w here £ C M — JJ- + A-fg CM
(see part 6.2).
For each equation Table 7 shows the
can
form of the matrix q . The matrix A is equal to the sum of all canonical generators e j . The explicit form of the ej is indicated in Appendix 2. Remark 1. The equations of Table 7 corresponding to the pairs (Af ) , c0) (A-?\ ct), ( A f , after linear changes of unknowns and scale transformations can be written in the Hamiltonian form (9.1) (see Table 6 ) . The remaining two equations, which are of a rather simple form, have a very complicated Hamiltonian form. Remark 2. Tables 6 and 7 contain all the simplest generalized KdV corresponding to al gebras G of ranks 1 and 2 except the equations corresponding to (A;2', Co) and ( A j 2 \ C i ) . In
2026
77
TABLE 6 Cm »i Cf * , • <
» JJ Cf a,.f j j C| JJ C| •W^i Vl.lt-*
TABLE 5
1*-
»f*»I-tu,«, tluf ♦ « ! -f?UiUt uf.u{-«}-»li,U t .«U,Uj«fcl ; U| !
1
'I
-T7JT
M
JfuJJi -MnJ J«j)« -Uj
sftsfcy*"'
1.-/ li«2t-l
u, »u;-(u,u,
•? 'C|I *,.!,< li"»
•r
feeaiaaafestay^
»7
UfU]-U,U|-U2U|*Uj *|f-1t t U]«-U,Uj*Us1l«-U]U«J»
'2
TABLE 7 6 A.
i
,*■
Simplest generalized KdV
•'
SX*tOfL*Ux
l
i
txxxx
T
*$U*U?
-«<«..« ♦ « I . J H "
"1.5"' ""U^"''^*"?"
S^c.
IT:. these two cases ic is possible to choose 2 C U so that the simplest equations of the series have third order. However, due to the complexity of the formulas, we note here only that both these equations have the form
v, - a.o,,, -f a,u,u„+GVI'U,+a« {uv,—vti,), where the coefficients a£ appropriate to each equation belong to Q[>ol. 10. TWO-DIMENSIONALIZED TODA LATTICES 10.1. In this subsection we recall the definition of the two-dimensionalized Toda lat tice corresponding to a Kats-Moody algebra, and for it we present the Zakharov—Shabat repre sentation found in [61]. In the next subsection, following [65, 72, 12], we consider local conservation laws and the connection of the Toda lattices with generalized mKdV. Let C be a Kats—Moody algebra with canonical generators e£, f£, h{, 0 < i < r. On G we fix a nondegenerate, invariant, symmetric, bilinear form coordinated with the canonical gradation G — 90'
(see Proposition 5.20).
We set ft — 0 ° .
We recall that the elements hj
generate 6 as a vector space, and there is exactly one linear relation (5.12) between then. For any i, 0 < i < r we denote by aj the linear functional on t>, such that [h, ej] ai(h)ei for all Ag$ (the a; are called simple roots of the algebra G). It is clear that [h, fj] - -ai(h)f j. We note that aj(b.£) - Aij , where (Aij) is the Cartan matrix. We call the two-dimensionalized Toda lattice corresponding to G the equation
£_2«"' W , -A..
+(*,T)e*.
(10.1)
This name is also sometimes applied to the system of equations J^R-exp2'V/'
0
n,(jc, x)eC.
(10.2)
We shall discuss the connection between (10.1) and (10.2). There is a mapping from the set of solutions of (1U.2) into the set of solutions of (10.1) given by the formula
2027
78
$ — 2 u'*i* ^ u e
to
r*!*1^00 (5.12) this napping is not bijective.
However, for any solution
i> or Eq. (10.1) it is not hard to find all solutions ( u 0 , . . . , u r ) of the system (10.2) such r
that y a,A,—if .
Namely, for u 0 it is possible to take any solution of the equation
,!??* —
£«•<*>, and after U Q has been chosen the remaining ui are found uniquely from the relation r 2 * * ( A i ~ ♦ !*■*• *■* n o t n a r < * t o s e * that the ui found in this manner satisfy (10.2)]. Thus, Eq. (10.1) is almost equivalent to (10.2). We further present the Lagrangian form of Eq. (10.1):
1-0 The equivalence of (10.1) and (10.3) follows from the following well-known lemma. LEMMA 10.1.
For any
y6$, g,(y)— ^ ' * ' ) .
Proof. (y, hi) - (y, [ei, fi]) - (ty, ejj, f£) - o,i(y)(ei, f i ) . Setting y - hi and using the equality ai(hi) - Aii ■ 2, we obtain (h£, h^) « 2(ei, fi)» whence the lemma fol lows . ■
Remark.
The equation J?!|-_grad U (+),
r U (+)—2 C|«*'W £ o r any
tf
/€C reduces to (10.3)
by means of a transformation of the form ^—^-f^, T —ax, where W&< a^C* Finally, we present the Zakharov—Shabat form of Eq. (10.1): l£.S]-0, 2 - r ^ . ^ . ^ + A - ^ + f + A . £-£ where A — 2'it A — 2 / i t i-o
and
(10.4)
+ €-■ Ae»,
t strictly speaking, e~*Ae* must be understood to be
e'^^Oi).
i-o
The equivalence of (10.1) and (10.A) follows immediately from the relations [ei, fjJ ■ ^ijnjt [h, fj] - - a i ( h ) f i . Remark 1. Equation (10.4) admits the more symmetric form f e ~ * n j - 1 * " + e*"Ae-*", t*n »
£ e-w+e-+*Ae**]
-0.
Remark 2. If we interpret A, A, and iKx, T ) as elements of a "genuine" Kats—Moody al gebra G (see Remark 2 following Proposition 5.8), then relation (10.4) is equivalent to the system (10.2). To conclude this subsection we clarify the origin of the term "two-dimensionalized Toda lattice." — 2 «*'""*"'
The Toda lattice is properly the system of equations ifo ■ ■ (*c
was
investigated in [33, 52, 53]).
. i£Z , where U -
From this infinite system there are two
t
ways to obtain finite systems: a) require that +i<.n " *i for some n (the periodic Toda lat tice); b) require that *o - i^+i ■ 0 for some n (the corresponding system of equations for ^l * n is called the nonclosed Toda lattice). The two-dimensionalization consists in 2 2 replacing 3 /3t by the operator 3 2 / 3 X 3 T . The two-dimensionalized periodic Toda lattice is essentially equivalent to Eq. (10.1) for an algebra G of type A^ 1 ', while the two-dimensional ized nonclosed Toda lattice is equivalent to the system (10.2) for the case where (Aij) is the Cartan matrix of an algebra of type AiiJ. The history of two-dimensionalization of the periodic Toda lattice and passage from A O ) to arbitrary Kats—Moody algebras can be traced in t30, 36, 45, 61, 64, 46, 5 5 ] . Concerning the nonclosed Toda lattice and its generaliza tions see [28, 29, 37, 44, 6 1 ] .
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79
10.2. The relation between two-dimensionalized Toda lattices and generalized mKdv cor responding to the same Kats-Moody algebra G is based on the fact that on operator 8 of the form (6.7) after the substitution fl-9* is converted into an operator 8 of the form (10.A). Proposition 10.2. Let Hi be the densities of conservation laws for generalized mKdV considered in Proposition 6.6. Then Hi, considered as differential polynomials in tj», are densities of conservation laws for (10.1). The proof is essentially the same as that of Proposition 1.5. We recall (see Sec. 6) that Hi has degree of homogeneity i ♦ 1 if it is assumed that degj-^ — J.
Moreover, Hi * 0 if and only if the remainder on division of i by the Coxeter
number of G is an exponent. Definition.
It is said that the equation £ " / ( * . *r.*T. *>„.««. S-TT...0
HO.5)
is a symmetry for the equation
^W. 9,. 9*. 9,,. ♦,*, ¥„.- • -)-0.
(10.6)
if the derivative with respect Co c of the left side of (10.6) computed by Eq. (10.5) vanishes on substituting for
qXJI...).
This equation for
4» by abuse of language we call, as before, a generalized mKdV. Proposition 10.3. for Eq. (10.1).
The generalized mKdV corresponding to the algebra G are symmetries
This proposition can be derived from Proposition 10.2 by means of a Hamiltonian formalism (see [72]). We present a direcC proof. Proof. where
i*63**
We recall (see part 6.4) that a generalized mKdV has the form It must be shown that if (fi, £J=0, then the derivative
generalized mKdV is equal to zero.
|i —[tp(u)*, g|,
;#[fi.fi).computed by the
For this it suffices to verify that
^ ™ = [9(u)*"( fi].
LEMMA 10.4. [fi, 9 («)]=-0. Proof. that
Let U and fio be the same as in Proposition 6 . 2 .
fi~**dy(fi0),
»(«)«■ e—'u(u).
Since [fi,fij —0 , i c follows that
easy Co deduce chat fi has che form fi— j ^ + c ( x ,
T), V (X, x)fc3 •
We s e t
£— e-Mt/(S)-
ISo.fi]—0.
We r e c a l l
From t h i s i t
is
Therefore, [fi. «] —0 » and hence
12. ?(«)!-0. ■ From the lemma i t follows Chac [9(a)*, fi)— — [9(a)", fi]. The degree of the l e f t s i d e (in the sense of the canonical gradation) i s not l e s s than —1, while che degree of che righC s i d e i s noc more than - 1 . Therefore, [9(u)*> fi|6C~ (R1. G-1). a n d i f 9(«) —]R Ai * w h e r e A* 6C-(R 2 , Gl), then
[©(a)*, fil —l-^ot. *~*A**I>
On the other hand, ^ . » _ l l *
«-»A**l.
In the course of the
proof of P r o p o s i t i o n 6.8 i t was shown that g e n e r a l i z e d mKdV as an equation for q has the form dq/dt - —3Ao/3x. Therefore, as an equation for 9 i t haa the form d$/3t - —Ao • Thus, rfj* — ^ —[9(a)*,fi], as was required to prove. ■ The conservation laws considered in Proposition 10.2 are only half of the known local conservation laws for Eq. (10.1). In order to obtain the second half it is necessary, roughly speaking, to interchange x and T . The same pertains to the symmetries considered in Proposi tion 10.3. 2029
80
APPENDIX 1 CLASSICAL SIMPLE LIE ALGEBRAS In this appendix for each classical simple Lie algebra 9 we list the system of Weyl generators Xi, Y^, H j t 1 < i < n (the numbering of the generators corresponds to the number ing of the vertices in Table 1 ) . In all cases the realization and the system of Ueyl genera tors are chosen that the Borel (Cartan) subalgebra of 9 is equal, respectively, to the inter section of 6 with the set of all upper triangular (diagonal) matrices. We recall that X T denotes the matrix obtained from X by transposition relative to the secondary diagonal. Type Aj,, n > 1 6 —»l(n + l) —{^eMat(n-(-l, C)|tr A— 0} . System of Weyl generators: X, — e,+,.i,
K,— «,,,+,, H,—
Type B„, n > 1 -
0*1
-*f
e - » ( & J - l ) - H A € M a t ( 2 r i + l , C ) | i * — — - S i T S - ' , S—dlag(l. - 1 - 1 . 1). System of Weyl gener a t o r s : XJ^-^J+I.J -\-e2n+?-i,if>-\-i, ' Ki — tfj.j+i + tfaTH-/.«*+*-/. # i ™ —«I.I -r-tf.+i.i+i—«2a+i-i.iM-i-.+ tfta+s-i.to+i-d * —1.2 « —1; Xa"=«*+,.n-t-«*+2.rt+i. J'.— 2(tf«,(,+i + e„+\,H+?), //„—2(«?.+».«+t—««.»)• Type C n , n > 1 « — »»<2/t) — {>4eMal(2rt, C ) [ * — — S ^ ^ - ' , 5 — dlig(l, — 1 1. — 1) . System of Weyl gen e r a t o r s : X,—et+i.t -f«2«+]-/.a«-i. ^j^*i.i+i -¥^u-t.u+i—t* W I ™ - * ( , I + 3 ©-•(2n)-{AeMat(2fl, C ) | J 4 - - 5 A r 5 - ' , S-diag(l, - 1 <-l)"-\ (-If 1 , (-1)* !)• System of Weyl generators: A", — «i+i.i +tfta+i-j.*i-i»K(«*i?,,.-4-i + £3«-..ai+i-i. //j — — *i,j-f*.+u+i — eU-l.7*-l + €u+\-t,7*+1-t-
' —1
1 — 1 ; Xft^-g-fe.+i.a-i + C«+2.a),
K* — 2(e«-l.«-H + '*.■+»).
^«
—
-e,_i,,-i-f M -fe l+ i,, + i + «,+!,,+a. For n - 2 all formulas remain in force, but the Dynkin scheme is not connected, so that the algebra 0(4) is semisimple rather than simple. Since the Dyn kin scheme of e(4) consists of two vertices not connected by edges it follows that «(4)=*t(2)X .1(2). APPENDIX 2 CLASSICAL KATS-M00DY ALGEBRAS In this appendix for each classical Kats—Moody algebra we present 1) a realization of G in the form L(£, C) , where C is the Coxeter automorphism; 2) a basis of the vector space 3d**—{*6G| [A, x] — 0 } and the eigenvalues of the matrix A in the realization; 3) the standard realization of G. We shall consider part 3) in more detail. Generally speaking, for each vertex c m of the Dynkin scheme of G we ought to present the corresponding standard automorphism oM:C-*-V . In constructing the standard realization corresponding to c m we actually replace M by an algebra %m of the form Rm%Rm\ where R Q is a permutation matrix, so that o m is an automorphism of %m rather than M. R Q is chosen so that the elements of the semisimple algebra 6 — { J C 6 *« I<*m(■*)—x} have block-diagonal form. Further, we do not consider all vertices of the Dyn kin scheme (for our purposes it suffices that each vertex be carried by some automorphism of the Dynkin scheme into one of the vertices considered). For all vertices c m considered we indicate %mt om, C , and also the canonical generators e£f.(Mm, oM)> Due to the special choice of the matrices R^ the algebras t) and I (see part 6.1) in all cases are equal, respectively, to G f l D U g and 6fi1. where t is the set of upper triangular matrices. In this appendix ©(*) and *t(2n) are the same as in Appendix 1. The number of the canonical generators of the Kats—Moody algebras corresponds to the number of the vertices of the Dynkin schemes in Table 2.
2030
81
Type A n l } ,
n > I
Mr
«-,l(n+l),
C(X)-5XS-',
*i
•<•), where « - « T ,
S-diag(l, a
A-»+1.
System of canonical generators: fg —Ci.a+iCt/a—'a+i.iC'1! A, — < n — «•+■.«+■: «, —«I+I.IC, / , — e,.1+iC"', *,— «/+!.n-i —«/./. i — I «. Eigenvalues of A equal to Cm1, i - 0, 1 n. Basis in 3 i s formed by A', where <€Z, i i s not d i v i s i b l e by n + 1. Standard r e a l i z a t i o n corresponding to « i , n * i A . *i " e i * l , i . f o r i " 1 , - . . , n .
c 0 :Vo—S, at(X) —X.
In t h i s r e a l i z a t i o n £o ■
Type A2(n' , n > 1 «-,c(2*+l), C(J0--5X r 5-'. S-dlag(l. -a, sf
-«*-', u»), u - « T , A-4n + 2.
System of canonical generators: e„—e,.j,+1C, / 0 —•JJ.+LIC*', *i-«i.i-«i.+i,i+i: «r(«iti.i + «t>+2-l. Ia+1-lKi / , — (
Eigenvalues of A equal to C w 2 1 , i ■ 0, t 21+1 is not divisible by 2n + 1. to c0:%
Standard realization corresponding -1
— 1 , t).
et—ci+i,t
2n.
Basis in
— %, o„(X) — —QXTQ-',
Order of Oo equal to two, « —»(2n-fl).
-\-ci*+7—t. %M-I—!• '■—I
formed by A 2 1 + 1 , where
3
where Q - d i a g O ,
In this realization i,—e,.
1.+1X ;
«.
Standard r e a l i z a t i o n corresponding to cm, m — \ a: «„ —«, o . (A^ — —QXTQ~', where -(jlo). a-dtag-(/, - i -MeiI(2«-2)n+l),B-dlag(l.-l 1,-1) e,t(2/n). Order of om equal to four, 6 —J|Q j l , O6C(2B —2»t+I), *€»»(2«)) .* *!,_■+»-/. J « - « + i - ; + * i i - « + 2 + / . J « - « + I + / . « / + l . / + '*■-»«+ ^ ->• s «- s "+ 1 -'■
In t h i s r e a l i z a t i o n
y -" 1
■'"" ,
/n — I;
«o"-«s«-«+>. J»-«+I - . «y —
« . — («i. i«+i - f e»,-2«+}. i«-2»+i) ^
<«♦/-
n—m.
Type A(2n>_1( n > 2 «-.l(2s),C(X)
«*■-« , - a * - ' ) . u-*" 5 ". A - 4 * - 2 .
SJC\S-'. 5 - d l a g ( l . - « . »»
System of canonical generators: e 0 —^(e,. J»_I + «J. u)(, / O " * 2 ( « J _ I . 1 + **.. i)C"', Aj—eLi + ^ j — tfb-l.2t-l—*ta.
to!
/ i " " ( ' i . ( + 1 + ' l t - 1 , Li-fl-.)*."1.
' l ™ ' ('/+!.( + «lt+I-(. l i - i ) C ,
The eigenvalues of A are equal to by A"" — ~nU(\"-')E,
i&.
" J ™ — £ ( . ( - r * l + l , (+1 —
* — 1 ; <« — «.+!.»C, / « — «/■.,+ii'1. A,— —e».« +««+I.»+I-
w4*~4C. A basis in the space 3
0, C, o^C
where for i < 0 A*" — C-"A"*'**\ A » 0
i s formed
(we note that t r A ^ V O
only
if 21 + 1 i s d i v i s i b l e by 2n — 1 ) . The standard r e a l i z a t i o n corresponding to —1
1, —1).
The
order of «o i s
e
( i. 2M-I -)-£?. it)X; et~€t+\,
e0:Mim^%t a0(X) w^—QXTQ"1, where Q ■ d i a g ( 1 ,
equal to two,
t + 'a«+i-(. 2«-(. /—1
0_t,(2n).
In t h i s r e a l i z a t i o n
e0—-7
ft — I; £»"**a+i. it-
Standard r e a l i z a t i o n corresponding to c„:K, — *, a„(JT) —»—Q^rQ-1, where Q«di*g(l, ( —1)«*>, (— l)"'1, (—1>"'1
—1. 1).
The order of a n i s equal to two,
i z a t i o n «j — ■ J ( « « + I . ^ I + «»+J.«)'I
l)eil(2w»). The
order
' —1
cm, m — 2, 3
is equal
6 — o(2n).
—1
In t h i s r e a l
n— 1; «, —
- ' . 06iI(2*-2/n), B-dlag(l. of o n
x
-1
<„ — %,
oa(X) — — QX'Q''.
(-1)-". (-I)-'.
to four, « - ! ( o ° ) . a€»»(2n—2m), »€.(2fit)}.
In
*The fact that •*>o(2>i — im+l)x«p(2m) follows from the general theory of Kats-Moody algebras (we recall that the Dynkin scheme of A is obtained from the Dynkin scheme of G by removing the vertex c m and the edges continuous to it). 2031
82
this
realization
•
m—1; « „ — ( « i . s » + « j . - i i i + i , ii_j«)X: *«,„/ — «/+i. / + « > » - i « + i - / . J » - J « I - ; .
c
£0— -K (tf&,-«,+l. U-m-l + ein-m+l. im-m)'* C) —■ Clit-m+l-J. 2it-M-J + £l«-*+l+7.24i-«-W. / * "
./ — 1
»—at—1:
*« —
n-m+i,n-m' Type B n 1 } , n > 2 4.1
*■'
«-=o(2n-j-l). C (JO-SATS"1. S = d i a g ( l . o, u*
o*- 1 , 1), a-*" 1 ", h-2n.
System of canonical generators: eo—-j (tfi. 2J> + « : . 2J+I)C./o—=2(tfi,, i + tf^+i. 2)C"1, Ao«—
rt—
1; C = (««+l.« + e«+2. « + l) C
/ « — 2(*«, iwl + «»+l. «+2> »"'.
*» —
2(e.+j, »+2—e...)-
The eigenvalues of A are equ al to 0, i, at
w5"-1;. A basis in 3 is formed by A"*', i€Z,
where for 1<0 A^'-C^A""*", * > 0 . Standard r e a l i z a t i o n corresponding t o £(,:«<> —M, ization
o0{X) — X,
<0 — f (
« —1
8 — o (2n + 1). In t h i s r e a l «•
n: « „ — {Xei<(2n+l)|X — — RX1 Rr%
Standard r e a l i z a t i o n corresponding t o c.,, m = 2
where / ? _ ( ° ° ) , a - d l a g ( l , - l - 1 , l)e«l(2n-2m + 1), p_diag(-l,l (-1)". (-1)". (—1)"*' —l)«l(2m); om(X) — QXQ-', where Q — dlag( — 1, —1 — 1 . 1,1 I). The order of 2
o m i s equal to two, 8 —((„ ?), a€»(2fi — 2/n-f 1), &e»(2m)l.
In t h i s r e a l i z a t i o n
«2i-«+S.2»-»+l); « ; — <2i-.»+2+;,2»-«+l + / + <2»-«+2-/.2»-«+l-y, CU-2m+2.U-lM+l)k\ em.i-*ej+1./-TCU-2m+2-J.7i-7m+l-j>
j-=\,...,m—
7 - = U •••■
1;
« 0 —■j(«2«-»+2.x < -»+ e » — (<1.2*+l +
fl—m.
Type C < J ) , n > I d.-f
^
B-«»(2n), C(X) = SXS', 5 - d i a g ( l , u, »-' (a5""1). <■> — « T , A —2n. System of canonical generators: «0 — «i.j,t, / 0 — ej»,iC"', A„ — e,,, — «2«,2«; «2t+l-/.2n-/)C,
*i — («I+I.< +
/ ( — (£*.l-t-l +«2Jf-i.2*+1-j)C"1, A , ~ — * l . l + £t + l,/+!—tfld-(.2«-( + *2jt+l-J.2n+l-it f «« 1
ft— \',
1
««—««+i.ni, /.■"<».«+iC" . A, ——e„..+ e„+,,»+i. The eigenvalues of A are equal to Cw1, i ■ 0 , 1 , . . . , 2 n — 1. A b a s i s in 3 i s formed by A**1. i&. Standard r e a l i z a t i o n corresponding to c0:%<^^it oQ(X)~X, «o"=*i.2«'-'i «. — «i+i.i+e««+i-i.2«-i,
i—I
6 —*»(2rt) .
In t h i s
realization
n —1; «. — «,+, „. del
Standard realization corresponding to cm. m — 1 n—1: Km->{X£t>(2n)\X——RXR~'}, where /?-*(£*). o-diag(l, - 1 1, - l)68l(2B-2m), p-diag(l, - 1 , .. .rr. — l)£|I(2m); o„(*)QXQ"1, where Q —dlag(—1, — 1
—1.1, 1
1). The order of a m is equal to two, « — ((<>>)•
Vi-2m
a€»>(2/i —2m), »e»»(2m)). In t h i s r e a l i z a t i o n ■i-1 m —1; e „ — («!.!. +«2.-2«+i.2«-2m)>-;
e „ - e2»-«+i.2»_i»; *, — «2— «+i+;.ai-«+/ + «!.-m+i-;.2,-«-;, e».; "= 'in.i +
C* ~ £
Type D ^ 1 ) , n > 3 d.i « - ° ( 2 n ) , C(X) = 5 ^ 5 " , S — d l a g ( l , u
w«-', w»-', u"
SI w2"-3, 1), a—e* , A - 2 n — 2 .
System of canonical generators: «0— -^(«i.2»-i + <2.2«){. / o — 2(e»,_i,i + ej,.j)t"1, «2n-i;j«-l — *2«.2V»
*J ■"('(+!./ - i - <2»+l-l.2«-l)C,
e i . - i . 3 a - i - f eiM-i-i.to+i-',
2032
' —1
/(""('l.i+1 +
ftfl-l.aw+l-JC"1,
n — 1 ; «. —-jfe.+i.n-i + e.+2.«)C,
A„—e,,,-|-<j,—
A , ^ — * ( . ( + *(+!./+! —
^"« —= 2<«„_,.„_n -1- „.„_,.->e;-", A.—
83
The eigenvalues of A are equal Co 0 (of multiplicity two), C, taC. 3
is formed by A21*', i£Zt
where for i < 0, A3**' — C"**AJI*l*w, A » 0
Standard realization corresponding to CQ-,%^ -= K, o0(X)=*X,
Standard realization corre sponding to c„, m-=2,3
GI*'*"^ . A basis in
and ;*-i**/?, igl.
6 —o(2/i).
In this realization
« - 2 : * „ - LYe»l(2/t)| A ' - — /?Aftf-'},
where /? — (f j). a — d1ag(l, — 1 , (—1)«-«-', ( —1)«—> l)6ll(&t — 2m), B — diag( — 1 , 1 (-I)".)-!)" -l)€«l(2m); am[X)-QXQ-}, where Q-dltg(-l, - 1 - 1 , 1, 1 1). order of o m is equal to two, 6 — I" X a€°(2» — 2m), *6«(2/n)| .
The x
In this realization e 0 — y
(«!«->i+i.ii->.-i + «n-«+j.!n-«i) i ef — eii-»,+i+/.2»-«,+/ + ei,-»!+i-/.i,_„_;, «;»-2*+i.2«-i«)A;
Here
y » I , . . . . m—1;
«„ -=(ei.i,+
em.) — e;-+i,/ + ej«-2«+i-/.2«-j«-;)' . / « - ! , . . . , / i — m — 1; *» —-5 («,_„+,.„-*-[ + «„_«+j.»-«). Type D ^ J , n > 2
l
*-{-*'e« (2«+2)|A' e,+J.»+i,
C(^0 —5^5"',
dii
T
RX R->),
fl-dlag(t,
S — dlag(u, a1
System of canonical generators: eau-i.ii+j);
-1
(-I)'",
0, 0, (-1)"* 1
o>», — 1, 1, w**,
l) + ( - l ) » « . + , . » + 2 <■> — e T _
A —2« + 2. ,
e0 —(«I..+J + «.+MI+2)C, / 0 — 2(«„+^l^-«!,+^.„+:)C" , A„ —2(«,.,—
/ I ~ ( « I . I + > + «J«+S-I.3«+J—iK"'i
w2"*'),
*i = —«i. 1 + « I + I . 1+1 —
«— I; «„-=(e»+i.«+«»+3.«+i)5, /» = 2(«»,.+,+ e, + ,.„ +J ){-', A„—2
(—«..«+*«+).«+J)-
The eigenvalues of A are equal to Cw 1 , i * 0,...,2n ♦ 1. A basis in 3 is formed by
A2"', ieZ. Standard realization corresponding to c„, m—0,1 where /?-(Jol- <» —dlag(l. — 1 where Q — dlag(— 1,— 1
2m+l). *e»(2m+l)}.
n: %m — [XT:tt(2n + 2)\X— —RXTR~'} ,
l)€H(2«-2m+ 1), B-dlag(-l, 1
—I, 1, 1
-l)e«l(2nt+l); o«(J0-QA-Q-'.
1) . The order of om i s equal t o two, ®""{(o »)• fl€'(2n —
In t h i s r e a l i z a t i o n «^ = «!,_„+!_/.j»_„ + ,_ ; +eu-m+*+i.n-m+i+j, j — 0. 1
C«=(£l.2*+J + *'4t-2«i+?.2»-2«i+l)*;
m— 1;
**+y "== * > + ! . ; + *li-2«+2-/.l«-2m+l-/. y — 1 , . . . . It— "1. LITERATURE CITED
1. 2. 3. 4. 5. 6. 7. 8. 9. ■0.
V. I. Arnol'd, Mathematical Methods of C l a s s i c a l Mechanics [ i n Russian], Nauka, Moscow (1979). N. Bourbaki, Lie Groups and Algebras [Russian t r a n s l a t i o n ] , Mir, Moscow (1976). N. Bourbaki, Lie Groups and Algebras. Lie Algebras. Free Lie Algebras [Russian trans l a t i o n ] , Mir, Moscow ( 1 9 / 2 ) . N. Bourbaki, Lie Groups and Algebras. Cartan Subalgebras, Regular Elements, Decomposable Semisimple Lie Algebras [Russian t r a n s l a t i o n ] , Mir, Moscow (1973). I. M. Gel'fand and L. A. D i k i i , "Fractional powers of operators and Hamiltonian systems," Funkts. Anal. P r i l o z h e n . , 10, No. 4 , 13-29 (1976). I. M. Gel'fand and L. A. Dlk~ii, "The resolvent and Hamiltonian systems," Funkts. Anal. P r i l o z h e n . , _H_. No. 2 , 11-27 (1977). I . M. Gel'fand and L. A. D i k i i , "A family of Hamiltonian structures connected with i n t e grable nonlinear d i f f e r e n t i a l equations," Preprint Mo. 136, IPM AN SSSR, Moscow (1978). I . M. Gel'fand, L. A. D i k i i , and I . Ya. Dorfman, "Hamiltonian operators and algebraic structures connected with them," Funkts. Anal. P r i l o z h e n . , J3_, No. 4 , 13—30 (1979). I. M. Gel'fand and L. A. D i k i i , "The Schoutten bracket and Hamiltonian operators," Funkts Anal. P r i l o z h e n . , J^, No. 3 , 71-74 (1980). I . M. Gel'fand and L. A. D i k i i , "Hamiltonian operators and i n f i n i t e - d i m e n s i o n a l Lie a l gebras," Funkts. Anal. P r i l o z h e n . , 15, No. 3 , 23-40 (1981).
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11. 12. 13. 16. 15. 16. 17.
18. 19.
20.
21. 22. 23. 24. 25. 26. 27.
28. 29.
30. 31. 32. 33. 34. 35. 36. 37.
38.
I. M. Gel'fand and L. A. Dikii, Hamiltonian operators and the classical Yang—Baxter equation," Funkts. Anal. Prilozhen., J£, No. 4, 1-9 (1982). V. G. Drinfel'd and V. V. Sokolov, "Equations of Korteweg—de Vries type and simple Lie algebras," Dokl. Akad. Nauk SSSR, 258, No. 1, 11-16 (1981). A. V. Zhiber and A. B. Shabat, "Klein-Gordon equations with a nontrivial group," Dokl. Akad. Nauk SSSR, 247, No. 5, 1103-1107 (1979). V. E. Zakharov, "On the problem of stochastization of one-dimensional chains of non linear oscillators," Zh. Eksp. Teor. Fiz., 65_, No. 1, 219-225 (1973). V. E. Zakharov and S. V. Manakov, "On the theory of resonance interaction of wave packets in nonlinear media," Zh. Eksp. Teor. Fiz., 69_, No. 5, 1654-1673 (1975). V. E. Zakharov, S. V. Manakov, S. P. Novikov, and L. P. Fitaevskii, Theory of Solitons: the Method of the Inverse Problem [in Russian], Nauka, Moscow (1980). V. E. Zakharov and A. V. Mikhailov, "Relativistically invariant two-dimensional models of a field theory integrable by the method of the inverse problem," Zh. Eksp. Teor. Fir., 74., No. 6, 1953-1973 (1978). V. E. Zakharov and L. A. Takhtadzhyan, "Equivalence of the nonlinear SchrCJdinger equa tion and Heisenberg's ferromagnetic equation," Teor. Mat. Fiz., 3_8, No. 1, 26-35 (1979). V. E. Zakharov and A. B. Shabat, "A scheme of integrating nonlinear equations of mathe matical physics by the method of the inverse scattering problem. I," Funkts. Anal. Prilozhen., 8_, No. 3, 54-56 (1974). V. E. Zakharov and A. B. Shabat, "Integration of nonlinear equations of mathematical physics by the method of the inverse scattering problem. II," Funkts. Anal. Prilozhen., J 2 . No. 3, 13-22 (1979). V. G. Kats, "Simple irreducible graded Lie algebras of finite growth," Izv. Akad. Nauk SSSR, Ser. Mat.. 22., No. 6, 1323-1367 (1968). V. G. Kats, "Infinite Lie algebras and the Dedekind n-function," Funkts. Anal. Prilozhen., 8, No. 2, 77-78 (1974). V. G. Kats, "Automorphisms of finite order of semisimple Lie algebras," Funkts. Anal. Prilozhen., 2 . No. 3, 94-96 (1969). E. A. Coddington and N. Levinson, Theory of Ordinary Differential Equations, McGraw-Hill (1955). V. G. Konopel'chenko, "The Hamiltonian structure of integrable equations under reduction," Preprint Inst. Yad. Fiz. Sib. Otd. Akad. Nauk SSSR No. 80-223, Novosibirsk (1981). I. M. Krichever, "Integration of nonlinear equations by methods of algebraic geometry," Funkts. Anal. Prilozhen., U_, No. 1, 15-31 (1977). D. R. Lebedev and Yu. I. Manin, "The Hamiltonian operator of Gel'fand—Dikii and the coadjoint representation of the Volterra group," Funkts. Anal. Prilozhen., 13, No. 4, 4046 (1979). A. N. Leznov, "On complete integrability of a nonlinear system of partial differential equations in two-dimensional space," Teor. Mat. Fiz., 42^, No. 3, 343-349 (1980). A. N. Leznov and M. V. Savel'ev, "Exact cylindrically symmetric solutions of the clas sical equations of gauge theories for arbitrary compact Lie groups," Fiz. El. Chastits At. Yad., J2> No. 1, 40-91 (1980). A. N. Leznov, M. V. Savel'ev, and V. G. Smirnov, "Theory of group representations and integration of nonlinear dynamical systems," Teor. Mat. Fiz., 48, No. 1, 3-12 (1981). I. G. Macdonald, "Affine root systems and the Dedekind n-function," Matematika, 16, No. 4, 3-49 (1972). S. V. Manakov, "An example of a completely integrable nonlinear wave field with nontrivial dynamics (the Lie model)," Teor. Mat. Fiz., 28_, No. 2, 172-179 (1976). S. V. Manakov, "On complete integrability and stochastization in discrete dynamical systems," Zh. Eksp. Teor. Fiz., 67_, 543-555 (1974). Yu. I. Manin, "Algebraic aspects of nonlinear differential equations," in: Sov. Probl. Mat. Tom 11 (Itogi Nauki i Tekhniki VINITI AN SSSR), Moscow (1978), pp. 5-112. Yu. I. Manin, "Matrix solitons and bundles over curves with singularities," Funkts. Anal. Prilozhen., U_, No. 4, 53-67 (1978). A. V. Mikhailov, "On the integrability of a two-dimensional generalization of the Toda lattice," Pis'ma Zh. Eksp. Teor. Fiz., 3_0, No. 7, 443-448 (1979). A. G. Reiman, "Integrable Hamiltonian systems connected with graded Lie algebras," in: Differents. Geometriya, Gruppy Li i Mekhanika. Ill, Zap. Nauchn. Sem., LOMI, Vol. 95, Nauka, Leningrad (1980), pp. 3-54. A. G. Reiman and M. A. Semenov-Tyan-Shanskii, "Algebras of flows and nonlinear partial differential equations," Dokl. Akad. Nauk SSSR, 251, No. 6, 1310-1314 (1980).
85 39.
A. G. Reiman and M. A. Semenov-Tyan-Shanskii, "A family of Hamiltonian s t r u c t u r e s , a hierarchy of Hamiltonians, and reduction for matrix d i f f e r e n t i a l operators of f i r s t order," Funkts. Anal. P r i l o z h e n . , Ut_, No. 2, 77-78 (1980). 40. J . - P . Serre, Lie Algebras and Lie Groups, W. A. Benjamin (1965). 41. V. V. Sokolov, "Quasisoliton s o l u t i o n s of Lax equations," D i s s e r t a t i o n , Sverdlovsk (1981). 42. V. V. Sokolov and A. B. Shabat, "(L—A) pairs and s u b s t i t u t i o n of R i c a t t i type," Funkts. Anal. P r i l o z h e n . , J £ , No. 2 , 79-80 (1980). 43. I. V. Cherednik, "Differential equations for Baker—Akhiezer functions of algebraic curves," Funkts. Anal. P r i l o z h e n . , _U, No. 3, 45-54 (1978). 44. M. Adler, "On a trace functional for formal pseudodifferential operators and the symp l e c t i c structure of Korteweg-de Vries type equations," Inventiones Math., 5£, 219-248 (1979). 45. 0. I. Bogojavlensky, "On perturbations of the periodic Toda l a t t i c e , " Comaun. Math. Phys., 5J_, 201-209 (1976). 46. S. A. Bulgadaev, "Two-dimensional integrable f i e l d theories connected with simple Lie algebras," Phys. L e t t . , 96B, 151-153 (1980). 47. E. Date, M. Jimbo, M. Kashivara, and T. Miwa, "Transformation groups for s o l i t o n equa t i o n s , " Preprint RIMS-394, Kyoto Univ. (1982). 48. E. Date, M. Kashivara, and T. Miwa, "Vertex operators and T-functions. Transformation groups for s o l i t o n equations. I I , " Proc. Jpn. Acad., A57, No. 8 , 387-392 (1981). 49. R. K. Dodd and J. D. Gibbons, "The prolongation structure of higher-order Korteweg-de Vries equation," Proc. R. Soc. London, 358, Ser. A, 287-296 (1977). 50. B. L. Feigin and A. V. Zelevinsky, "Representations of contragradient Lie algebras and the Kac-Macdonald i d e n t i t i e s , " Proc. of the Summer School of Bolyai Math. Soc. Akademiai Kiado, Budapest (to appear). 51. H. Flashcka, "Construction of conservation laws for Lax equations. Comments on a paper of G. Wilson," Q. J. Math., Oxford (to appear). 52. H. Flaschka, "Toda l a t t i c e I , " Phys. Rev., B9. 1924-1925 (1974). 53. H. Flaschka, "Toda l a t t i c e I I , " Progr. Theor. Phys., 5\_, 703-716 (1974). 54. A. P. Fordy and J. D. Gibbons, "Factorization of operators. I . Miura transformations," J. Math. P h y s . , 2±, 2508-2510 (1980). 55. A. P. Fordy and J. D. Gibbons, "Integrable nonlinear Klein-Gordon equations and Toda l a t t i c e , " Coramun. Math. Phys., JT_. 21-30 (1980). 56. I. B. Frenkel and V. G. Kac, "Basic representation of affine Lie algebras and dual r e s o nance models," Invent. Math., 62_, 23-66 (1980). 57. V. G. Kac, "Infinite-dimensional algebras, Dedekind's n-functions, c l a s s i c a l MSbius function and the very strange formula," Adv. Math., 2p_» *>• 2> 85-136 (1978). 58. B. Konstant, "The p r i n c i p l e three-dimensional subgroup and the Bettin numbers of a complex simple Lie group," Am. J. Math., _131_, 973-1032 (1959). 59. B. A. Kupershmidt and G. Wilson, "Conservation laws and symmetries of generalized s i n e Gordon e q u a t i o n s , " Commun. Math. Phys., 8 1 , No. 2 , 189-202 (1981). 60. B. A. Kupershmidt and G. Wilson, "Modifying Lax equations and the second Hamiltonian s t r u c t u r e , " Invent. Math., 6 2 , 403-436 (1981). 61. A. N. Leznov and M. V. SaveTTev, "Representation of zero curvature for the system of nonlinear p a r t i a l d i f f e r e n t i a l equations XQ* Z Z * exp (KX)a and i t s i n t e g r a b i l i t y , " L e t t . Math. P h y s . , 2 . *>• * . 489-494 (1979). 62. I. G. Macdonald, G. Segal, and G. Wilson, Kac-Moody Lie Algebras, Oxford Univ. Press (to appear). 63. F. Magri, "A simple model of the integrable Hamiltonian equation," J. Math. Phys., 19, No. 5, 1156-1162 (1978). 64. A. V. Mikhailov, "The reduction problem and the inverse s c a t t e r i n g method," i n : Proceed ings of Soviet—American Symposium on S o l i t o n Theory (Kiev, September 1979), Physics, 2> Nos. 1-2, 73-117 (1981). 65. A. V. Mikhailov, M. A. Olshanetsky, and A. M. Perelomov, "Two-dimensional generalized Toda l a t t i c e , " Commun. Math. P h y s . , .79, 473-488 (1981). 66. R. V. Moody, "Macdonald i d e n t i t i e s and Euclidean Lie a l g e b r a s , " Proc. Am. Math. S o c , 4 8 , No. 1, 43-52 (1975). 67. D. Muaford, "An algebrogeometric construction of commuting operators and of s o l u t i o n of the Toda l a t t i c e equation," Korteweg-de Vries Equation and Related Equations. Proceed ings of the International Symposium on Algebraic Geometry, Kyoto (1977), pp. 115-153. 68. J . L. Verdier, "Les representations des algebres de Lie a f f i n e s : applicationa a quelques problemes de physique," Scainaire N. Bourbaki, Vol. 1981-1982, j u i n , expose No. 596 (1982).
203J
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69. 70. 71. 72.
J. L. Verdier, "Equations differentielles algebriques," Sem. Bourbaki 1977-1978, expose 512, Lect. Notes Math., No. 710, Springer-Verlag, Berlin (1979), pp. 101-122. G. Wilson, "Commuting flows and conservation laws for Lax equations," Math. Proc. Cambr. Philos. S o c , 86_, No. 1, 1 3 1 - H 3 (1979). G. Wilson, "On two constructions of conservation laws for Lax equations," Q. J. Math. Oxford, 32_, No. 128, 491-512 (1981). G. Wilson, "The modified Lax and two-dimensional Toda lattice equations associated with simple Lie algebras," Ergodic Theory and Dynamical Systems, ^, 361-380 (1981).
HIGHER REGULATORS AND VALUES OF L-FUNCTIONS A. A. Beilinson
UDC 512.7
In the work conjectures are formulated regarding the value of L-functions of mo tives and some computations are presented corroborating them.
INTRODUCTION Let X be a complex algebraic manifold, and let Kfi,X), HJQ(X,Q) be its algebraic K-groups and singulary cohomology, respectively. We consider the Chern character ch: Kj(X)®Q-*-® J Hj0~ (X,Q). It is easy to see that there are the Hodge conditions on the image of ch: we have ch (Kt(X))cz Q^tfjf'iX, Q)) f) (PZ/jf"' (X, C)), where W., F* are the filtration giving the mixed Hodge structure on H'$(X). For example, if X is compact, then ch (Kj(X)) - 0 for j > 0. It turns out that the Hodge conditions can be used, and, untangling them, it is pos sible to obtain finer analytic invariants of the elements of K.(X) than the usual cohomology classes. For the case of Chow groups they are well known: they are the Abel—Jacobi-Criffiths periods of an algebraic cycle. Apparently, these invariants are closely related to the values of L-functions; we formulate conjectures and some computations corroborating them. In Sec. 1 our main tool appears: the groups Hg>(x,Z{i)) of "topological cycles lying in the i-th term of the Hodge filtration." These groups are written in a long exact sequence
~"+**iil(X. C)-.//^(X, Z(i))
* H'm{X. Z)
On H'g) we construct a U -product such that *,# becomes a ring morphism, and we show that fig, form a cohomology theory satisfying Poincare duality. Therefore, it is possible to apply the machinery of characteristic classes to Hg> [22] and obtain a morphism chg>:Kj{X)Q Q -*®//J>~y(X, Q(i)). The corresponding constructions are recalled in Sec. 2. Let H*£l{Xt Q (t))dX'y(.Y)8Q be the eigenspace of weight i relative to the Adams operator [2]; then ch^ defines a regulator - a morphism r^://^(X, Q(*))-► #£>(*. Q(0). lit is thought that for any schemes there exists a universal cohomology theory Ji'^^X, Z(i))t satisfying Poincare duality and related to Quillen's K-theory in the 6ame way as in topology the singular cohomology is related to K-theory; H'^ must be closely connected with the Milnor ring.] In the appendix we study the connection between deformations of ch^, and Lie algebra cohomologies; as a consequence we see that if X is a point, then our regulators coincide with Borel regulators. There we present a formulation of a remarkable theory of Tsygan-feigin regarding stable co homologies of algebras of flows. Finally, Sec. 3 contains formulations of the basic conjec tures connecting regulators with the values of L-functions at integral points distinct from the middle of the critical strip; the arithmetic intersection index defined in part 2.5 is responsible for the behavior in the middle of the critical strip. From these conjectures (more precisely, from the part of them that can be applied to any complex manifold) there follow rather unexpected assertions regarding the connection of Hodge structures with alge braic cycles. The remainder of the work contains computations corroborating the conjectures in Sec. 3. Thus, in Sec. 7 we prove these conjectures for the case of Dirichlet series; Translated from Itogi Nauki i Tekhniki, Seriya Sovremennye Problemy Matematiki Dostizheniya), Vol. 24, pp. 181-238, 1984.
2036
0090-4104/85/3002-2036$09.30
C 1985 Plenum Publishing Corporation
(Noveishie
89
Reprinted with permission from Physics Letters B Vol. 206, No. 3, pp. 412-420,26 May 1988 © 1988 Hsevier Science Publishers B.V. (North-Holland Physics Publishing Division)
SYSTEMATIC APPROACH TO CONFORMAL SYSTEMS WITH EXTENDED VIRASORO SYMMETRIES Adel BILAL and Jean-Loup GERVAIS Laboratoire de Physique Thtorique de VEcole Normale Suptrieure \ 24 rue Lhomond, F- 75231 Paris Cedex 05. France Received 29 February 1988
The Toda field theories, which exist for every simple Lie group, are shown to give realizations of extended Virasoro algebras that involve generators of spins higher than or equal to two. They are uniquely determined from the canonical lagrangian formal ism. The quantization of the Toda field theories gives a systematic treatment of generalized conformal bosonic models. The wellknown pattern of conformal field theories with non-extended Virasoro algebra, appears to be repeated for any simple group, leading to a "periodic table", parallel to the mathematical classification of simple Lie groups.
1. Introduction It is important to organize the growing number of discrete series of conformal models, and to devise methods that allow to derive all such models systematically. The basic point in this connection is to extend the Virasoro algebra in all possible ways. In the present paper, we develop a general approach to this problem that, for any givenflnite-dimensionalLie group, leads to an extended Virasoro algebra, together with the associated families of conformal field theories. Details will be left for future publications and we shall, for the time being, only consider bosonic theories. Consider, as a warming up, the conformal models with unextended Virasoro symmetry. They are completely consistent only if the central charge C takes the values C=l-6/r(r+l),
rinteger>2,
C=7,13, 19, C=l+6(r+l)7/-,
(1.1) (1.2)
rinteger>0.
(1.3)
The first set is the celebrated series of Friedan, Qiu, and Shenker (FQS) [ 1 ]. The other two are not so wellknown at the present time. They were obtained by Gervais and Neveu (GN) [2,3], from their study of the Liouville field theory. These three sets lie in the ranges C< 1, 1 < C< 25, C> 25, respectively. The corresponding models are closely related since their spectrum of highest weights are given by the general formula [4] *' t(m,n) = ^ ( l - C ) [ m + n + ( m - f i ) V ( C - 2 5 ) / ( C - l ) ] 2 + 5 ! , ( C - l ) ,
(1.4)
where m and n are integers which vary over an appropriate range that depends on C. Although it looks superfi cially different, this last formula does give back the correct highest weights of the FQS series [ 1 ] upon substi tuting eq. (1.1) since the square root becomes rational. In general, this square root makes it clear why there are three different regions for C separated by the special values C0=l,
and C , = 2 5 .
(1.5)
' Laboratoire Propre du Centre National de la Recherche Scientifique associe 41'Ecole Normale Superieure et I l'Universit6 Paris-Sud. *' See ref. [ 5 ] for a review.
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Remarkably the series (1.1) and (1.3) are both particular cases of the general formula of Belavin, Polyakov and Zamolodchikov [6]. C=l+6(r+s)2/rs,
r,s integers.
The FQS series corresponds to r+s=(1.6) is that it leads to (C-25)/(C-\)
(1.6) 1, while the GN series (1.3) is given by 5=1, r>0. The point of eq.
= [(r-s)/(r+s)]2,
(1.7)
and formula (1.4) gives rational and real values for all m and n. The region 1
(1.8)
The FQS series (1.1) may be obtained by the Goddard-Kent-Olive construction [12] which is based on the SU(2) Kac-Moody algebra. On the other hand, theGN series (1.2), (1.3) which both lie in the region C> 1, have been obtained by quantizing the Liouville field theory, that is a field theory involving one bosonic field with an exponential potential. Such a theory is a particular case of an infinite family of generalized Liouville dynamics, called Toda field theories [13], each of them being associated with a given standard Lie group. The number of fields is equal to the rank of the group, and the standard Liouville theory corresponds to SU(2) in this general picture. One thus sees that the family of theories (1.1)-(1.3) is related to the group SU(2). Our aim, in the present article, is to extend the scheme we have just outlined to groups of higher rank. This will lead to a systematic formulation of models with extended Virasoro algebras, of the type introduced by Zamolodchi kov [14]. The basic tool will be the Toda field theories [13] that generalize the Liouville field theory for arbi trary groups. This will be the subject of section 3, but it is useful to draw the general picture before plunging into the details. This is done in the next section.
2. The general picture of bosonic conformal Held theories In this section we give, without proof, the generalization of the above formulae to an arbitrary simply-laced group g. Some of these formulae have already been written down, but no systematic treatment exists to our knowledge. This will be given in section 3. We shall denote by / the rank of g and by hc its Coxeter number. The discrete series (1.1) becomes '2 See ref. 18 ] for a review.
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C=l[l-hc(K
PHYSICS LETTERS B
+ l)/r(r+l)],
26 May 1988
rinteger>h c .
(2.1)
The corresponding highest weights are given by «. J .= [ l / 2 r ( r + l ) J { [ ( r + l ) m , - r n ' ] » u [ ( r + l ) m ' - r / i ' ] - T L A c ( d i m g ) } ,
(2.2)
where m and n are sets of/ integers. Throughout this paper, j is an index. When we need the square root of minus one, we shall write it explicitly in order to avoid confusions. %, is the inverse of the Cartan matrix of the group g. The series (2.1) is obviously such that C<1. It was first derived by Fateev and Zamolodchikov [15], for SU(3). Both eqs. (2.1) and (2.2) appear, but without complete proof, in an article by Bais, Bouwknegt, Surridge and Schoutens [ 16 ], who carry out the GKO [12] construction for general groups. A recent paper " of Fateev and Lykyanov treats the case of SU (N) [17]. The generalization of eq. (2.2) to other values of C may be written down by extending relation (2.1) to noninteger values of r. One may then determine r as a function of C, obtaining / • = j { - l ± v / [ C - / ( l + 2A c ) 2 ]/(C-/)}
(2.3)
and, substituting into (2.2), im..= [(C0-C)/ilhc(hc X%l(m'
+ l)][(m' + n-) +
+ n') + (m'-n')s/(C-C,)/(C-Co)]
(m,-nl)y/{C^C\)/(C-C0)] + [(C-C0)/24l][l/(hc
+ \)]dim&,
(2.4)
where C0 = l,
C,=l(\+2hc)2.
(2.5)
The plus or minus sign ambiguity in eq. (2.3) corresponds to exchanging m and «, and is thus irrelevant. As we shall see later on, eq. (2.4) is the correct continuation of (2.2). Eq. (2.4) is the generalization of (1.4). The value C0 corresponds obviously to / free bosonic fields. It separates the region where eq. (2.4) gives positive or negative values for m' and n' all positive. As section 3 will show, with this choice formula (2.4) gives the highest weights of the null states. Thus, in the same way as for the standard case, C0 separates the region where all positive highest weight representations are unitary (C> C 0 ), from the region where this is true only for partic ular values of C, that is, presumably, for the series (2.1). Clearly C0 is larger than one except for SU (2). There fore, some of the members of the series (2.1) share this property. They are mathematically similar to the theories of the FQS series however. Indeed, their spectrum of highest weights coincides with a set of null states and their Green functions satisfy differential equations of the hypergeometric type, as was shown for the case of SU (3) [15] and very recently *' for SU (N) [17]. The complementary region C>Ca will be most naturally described from the generalized Liouville theory, called Toda field theory, to be discussed in section 3. The discrete series (2.1) is a particular case of the ansatz C=t{\+hc(h,
+ \)(r+s)2/rs]
, r, .s integers ,
(2.6)
that generalizes formula (1.6). This again leads to rational highest weights since, in this case, (C-Cl)/(C-C0)
= [(r-s)/(r+s)]2.
(2.7)
We shall show that the generalization of (1.3) is indeed given by eq. (2.6) with r positive and s equal to one. This last series lies in the range C> C,. Finally, for C'0< C< C,, a characteristic feature of the three values (1.2) is that they are equally spaced between C0 and C,. (This is also true for the supersymmetric Liouville theory where C0 = \ and C, = ^ ) . Thus we believe that the generalization of (1.2) is C=/[l+Wi c (Ac + l ) ] , ,J
y=l,2,3.
This preprint was circulated while the present work was being completed.
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(2.8)
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By analogy with SU (2) (Liouville), the spectrum of highest weights should be given by tm^
= l(4-v)m'9,lm>+iiVthc(hc
+ i) = t(m).
(2.9)
For the series (1.2) of SU (2), we pointed out [ 7,8 ] that the partition function associated with the highest weights, that is to (1.4) with m = — n, has special properties that are crucial in the building of the associated string dynamics. For a general group g, one has a similar situation. The basic point is that the partition function may be written as a sum over all weight lattice vectors w (the common length squared of all roots is taken equal to 2): Zo^I<72'<-)-2,<,)=I<7(4-""1. m
(2.10)
w
After a Jacobi transformation \n{q) In(i7) = (2n)2t this becomes the following sum over the root lattice:
£f/«->.
(2.11)
a
It only involves integer powers of q for v=2 and 3. For the Liouville Neveu-Schwarz-Ramond models, the equivalents of the last two choices give the Liouville superstring theories that are space-time supersymmetric in three and five dimensions, respectively [ 7,8 ]. The authors of ref. [16] have argued that C crll =2/(1+2A C + 2AC2).
(2.12)
Thus eq. (1.8) holds for any group. The formulae we just wrote are all such that the expressions recalled in section 1 correspond to g=SU(2). Indeed this group has a rank equal to one and a Coxeter number equal to two.
3. The Todafieldtheories Let us now consider the Toda field theories [13]. The action is given by S-jiodxUdrf'K^-VW)],
K(0)=Xexp(K„
(3.1)
where K„ is the Cartan matrix of g. The equations of motion are 6 + a_0'=exp(AO,0')
wilhx± = {(a±r)
, 31=a„±3, .
(3.2)
These Toda field theories are conformally invariant. They are essentially the only interacting bosonic two-di mensional field theories having this property. Indeed, for a field theory (3.1) with a general potential V, the Noether energy-momentum tensor Tm has a trace equal to 2 V. The improved energy-momentum tensor 0„, = 7-„, + (6„6„-»;„,a 2 )/(0)
(3.3)
istraceless (using the equations of motion (3.2)) provided (1) / i s a linear function of $:f— Y.
(3.4)
Hence the theory is conformally invariant if and only if V is either zero or an exponential of the fields. If (in the latter case) we further demand that the theory be integrable, one ends up with the Toda field theories (3.1), i.e. the matrix K,t must be the Cartan matrix of some group g. The general solution of the Toda field theories as given in ref. [13] makes use of the underlying group struc415
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ture encoded in the Cartan matrix. It relates the fields 0' to / arbitrary functions of x* and / others of x~, thus separating the left- and right-moving degrees of freedom. One has exp(-0') = ( < A , | [ A / + U + ) ] - | / n / / U + ) * ' ^ A / - ( j : - ) i / n / 7 ( x - ) » ^ | > l , > J .
(3.5)
The X, are the fundamental weights, defined as the basis which is dual to the one given by the simple roots. The M ± are matrices acting in the corresponding representation space. They are solutions of the differential equations Z.M*-=M*Ydf;-(z*)Etl,
(3.6)
y-i
where the Etl are the step operators acting along the directions of the simple roots. In the case of/= 1 (SU(2): Liouville) any two solutions are conformally equivalent, the arbitrariness of the two functions/ 1 being absorbed by appropriate conformal transformations of x ±. For higher / one thus expects that the arbitrariness in the choice of the 2/ functions/,1 corresponds to a bigger symmetry. We will indeed show that extended Virasoro symmetries appear. The general solution (3.S) is given by the scalar product of a left-moving and an analogous right-moving piece. It is sufficient to concentrate on one of them, say the right-moving one. We will simply write x instead of x~. To be definite we will choose in the following the case of the simply-laced algebras SU(Ar). Let us consider the construction of exp(—0'). X, is the heightest weight of the Af-dimensional defining representation. The right-moving piece of the solution is then an M-component vector depending on N— 1 arbitrary functions / - (x)=A'j(x) (primesdenote derivatives):
Y\A;(x)-9-M(x)U,y=n^M-91]
A,{x) /'dx,^U,Ml(x,) IH V> I/'(be, S''dx2As(x1)A-2(x2)A\(x,)
<3-7>
We now show that the y/, satisfy a linear differential equation of order N. First, the common factor UJA'J (x)_ '*"=Vi is precisely such that the wronskian of Vu ¥2 VN is equal to 1 as one may verify by explicit calculation: tf'i
¥2
•••
V'N
N-\
=i»f,-*=nKr,
0.8)
which coincides with the above value of i//\ since %=i(N-j)/N
fori^.
(3.9)
Next, each of the if/,,..., y/N is a solution of a linear differential equation of order N, obtained by writing that the wronskian of the v, and any linear combination i// of them is zero: Ci
-
v\N>
... i//tf'
VN
V
0. Developing with respect to v we obtain the differential equation 416
(3.10)
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(-V»> + Ua)V»-2>+U{,)df»-:"
PHYSICS LETTERS B
26 May 1988
+ ...+ UwW=0.
(3.11)
It may be seen that, conversely, any set of N independent solutions of this equation can be brought under the form (3.7). For this, one combines them in such a way as to eliminate the potentials UU). It is remarkable that (3.7) was first derived purely from the Lie algebra so that there appears an interesting relationship between linear differential equations and group theory. The coefficients U(i) are only functionalsof A" /A] = -p'(x) and of its derivatives. For N=2 (Liouville) eq. (3.11) is nothing but the associated Schrodinger equation intro duced by GN [8]. For general N, computing the potentials U0) is tedious but straightforward. Only U(2) has a simple expression: Vw = { I %(p'p' + NSudp'/dx).
(3.12)
The fields p' are the fundamental dynamical variables that separate the degrees of freedom. Using the Poisson brackets (A is a parameter that plays the role of Planck's constant) {P*(x),pJ(X-)} = 47thK,J6'(x-x') ,
(3.13)
one shows that Ul2 > 12ft generates the Virasoro algebra with a non-vanishing central charge even at the classical level: IN Cci.„=^-I».. = *(*2-l)/2ft.
(3.14)
From our experience with the case N = 2 (Liouville) it is clear that the Poisson bracket (3.13) leads to canonical Poisson brackets between 0' and its conjugate momentum Kv$'. The next potential l/ l3) contains term cubic in the p\ terms quadratic with one derivative and terms linear with second derivatives. We will only write it here explicitly in the case N= 3: Uw = 2LA2pl+p2){2p2+p,)(p,-Pl)
+ \(2pl+pi)p\+\(2p';+p';).
(3.15)
Its Poisson bracket with Ul2), is such that it transforms as a conformal field of weight 3, up to central terms. The Poisson bracket of Uai with itself has an interesting structure. It does not close in the usual Lie algebra sense, since its expression involves Ul2h V{i), and (l/< 21 ) 2 : Denoting by L„ the Fourier modes of U(2) /2ft, and by T„ those of C, 3, / 2 , / ^ T ft one finds ^{T„,T„}
= -2(n2-m2)T^m-Un-myL„„
+ 2h(¥)Hn-m)^LkLf,.„_k
+
(4/3ft)niS„._„. (3.16)
It is also possible to express the generators U0) in terms of the fields 0', 0'. For example, l/ (2) is nothing but the (—component of the) improved energy-momentum tensor as computed from the action (3.1). It gener ates the conformal symmetry of this action. In the same way we can compute the transformations of the fields 0' as induced by Poisson brackets with U,,t (0, 0). It is clear that these should be symmetries of the action, too. Hence it should be possible to exponentiate them. Therefore the Poisson bracket of any two potentials U0)
~np(n\,)p'0x)
with 417
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tfi) = ».„ tfo = %-».->./
forl
26 May 1988
(3.17)
The differential equation they satisfy can thus be written in a factorized form: Y\(-d+)i'l,)Pi)v",)
= 0.
(3.18)
Comparing eqs. (3.11) and (3.18), one immediately finds (C/(„)o~ ( - ) ' " '
I
/<<,,,-Vo,, *>$'•••/>£•
(3.19)
Going back to the case of non-constant p', we remark that, for Liouville [ 18], the factorized form (3.18) remains correct, with an appropriate ordering. We have checked that this generalizes to yV= 3. It is a conjecture that this is true for all N. Consider next the classical conformal family. By integration of A" /A', = -p' we reconstruct /i;=exp(-Jd>cV(*'))=exp[-'(;t)] ,
(3.20)
and hence obtain the solutions C'= I~I-<; "'"'=e*P( *./?/).
V2 = Vi j
(3.21)
They can be expressed in terms of the basic fields 0,=exp($,n),
/=l
JV-l
(3.22)
as y,~(0,_i)"'0, (with e o = 0 * = l ) . The basic fields d, generate the conformal family by taking products of n' fields*?,. Such a product (classically) has a conformal weight —NJ.,%n'/2. Let us now turn to the quantum case. The fundamental Poisson bracket (3.13) gets replaced by a commutator v/'— 1{ , } - » [ , ]. For the Fourier modes we have [p'„,P'„]=2hnK„6n._„.
(3.23)
The classical expressions for (/„, now have to be normal ordered. The Virasoro operators are L„=£„ + CQlm„/24: L„=^l%(l;:p'„P'„-„:-J:r\N6IJnp^+[N{N2-\)/4it1]S„,0,
(3.24)
and the quantum central charge is C=(N-\)[\+N(N+l)/2fi]=l[l+hc(hc
+ \)/2fi] .
(3.25)
As usual the pL„ create harmonic excitations on top of ground states labelled by their p'0 eigenvalue. These ground states are heighest weight states of the extended Virasoro algebra. We have to determine the spectrum of all possible zero-modes p'0. TheSL(2,C) invariant vacuum, i.e. the state annihilated by £<, and L ± 1 , haspj> = -x/^Tforali;=l,...,Ar-l. The quantum version of eq. (3.20) now reads A',= :exp( -t\\
dx'p'(x') j:= : e x p [ - w , ( x ) ] : .
(3.26)
The value of 7 is determined in such a way that all 1//, are conformally covariant operators. By eq. (3.21) we see that this is only the case provided A) has conformal weight 1. This fixes r\ to be a solution of 418
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2h)i2-ti+l=0^tit=(\/4fi)(\±s/i-ifi) .
(3.27)
There are two solutions i)± and the basic operators that generate the conformal family become $r= :exp(rit <3vq,y. , i= 1,..., N- 1 .
(3.28)
A general conformal operator of this family is obtained by taking products of n\ Sf and n'_ d,~ and removing the short-distance singularities. As can be explicitly seen from (3.23), (3.24) and (3.28) such an operator has a conformal weight A(»,M) = -h9uCi:j-lN9uC'.
f' = n' + >; + +'! , _»;_ ,
(3.29)
and, using (3.27), (1 denotes the vector (1, 1,..., 1)) J{H,m) = ((n + l,m+l),
(3.30)
where the right member coincides with (2.4). One may further write t(n,m)=(l/4fi)9„Pl0p>0
+ N(N2-\)/4&fi,
p'0(n,m) = -llJ^\[(n'+m')
+ (n<-m,)sJ\-M,),
(3.31)
showing what are the eigenvalues of p i in the quantum case. This determines the eigenvalues of Lo for all highest weight states, together with the eigenvalues of the zero modes of the higher spin operators. These are, in general, obtained by substituting (3.31) into (3.19). This general situation is very similar to the case of Liouville [8]. One thus expects that, here also, the classical differential equation (3.11) will carry over to the quantum case where it will lead to differential equations for correlators describing the decoupling of null vectors. Moreover, higher positive powers will also satisfy similar differential equations showing that formula (2.4) with m ' > 0 and n' > 0 does give the appropriate generalization of Kac's formula, as anticipated in section 2. This, of course, needs further study but the analogy with the Liouville case is compelling. Let us finally derive the generalization of the discrete series (1.3) of central charges, that is eq. (2.6) with s=l. This corresponds to the region C>C,, i.e. h< J andpo is purely imaginary. In this region which is con nected to the classical limit ft-»0 (where»;+ is singular) only */_ has to be used in constructing conformal fields. Hence only
p'0(l-l+m) = -yf^\[\ + \m>(\-J\-m]
(3.32)
are allowed. The SL(2,C) invariant vacuum p0 = —s/—l 1 corresponds to m=0. In analogy with the case N=2 (Liouville) it is clear that the local field exp( —0') shifts m' by two units. Starting from the SL(2,C) invariant vacuum, p0=-sp-\ 1, its conjugate Po = +\f—i 1 can only be reached if (r+l)(l-yi-8«) =2
(3.33)
for some positive integer r. This leads to the special values of ft: *=r/2(7-+l) 2 , r=integer>0,
(3.34)
which are the same for any group SU{N). In particular, (3.34) coincides with the series of the Liouville theory. If we use eq. (3.25) to reexpress ft in terms of the central charge C we get eq. (2.6) w i t h s = l as claimed in section 2. It is only for these special values of the central charge that we can consistently restrict ourselves to - 1 < >/^-T pi < 1 and hence to positive heighest weights.
Acknowledgement One of us (J.-L.G.) is grateful to Davd Olive for detailed discussions about the Toda field theories. 419
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References [ I ] D. Friedan, Z. Qiu and S. Shenker, in: Vertex operators in mathematics and physics (Springer, Berlin, 1984). [ 2 ] J.-L. Gervais and A. Neveu. Nucl. Phys. B 238 (1984) 125. [ 31 J.-L. Gervais and A. Neveu, Phys. Lett. B 151 (1985)271. [4) J.-L. Gervaisand A. Neveu, Nucl. Phys. B 257 [FS14] (1985)59. [ 51 J.-L. Gervais, in: Unified string theories, 1985 Santa Barbara Workshop, cds. M. Green and D. Gross. | 6 ] A. Belavin, A. Polyakov and A. Zamolodchikov, Nucl. Phys. B 241 (1980) 333. (7] A. Bilal and J.-L. Gervais, Phys. Lett. B 187 (1987) 39; Nucl. Phys. B 284 (1987) 397; B 293 (1987) I; B 295 [FS21 ] (1988) 277. [ 8 ] J.-L. Gervais, Liouville superstrings, LPTENS preprint 87/39, note of lectures Poiania Brasov summer school (Romania). 19 ] V. Dotsenko and V. Fateev, Nucl. Phys. B 240 [ FS12 ] (1984) 312. (10) J.-L. Gervais and A. Neveu, Nucl. Phys. B 238 (1984) 396. 111 ] A Bilal and J.-L. Gervais, preprint LPTENS 87/33, submitted to Nucl. Phys. B (12] P. Goddard, A. Kent and D. Olive, Commun. Math. Phys 103 (1986) 105. 113 ] See e.g. P. Mansfield, Nucl. Phys. B 208 (1982) 277, and references therein. 114] A.B. Zamolodchikov, Teor. Mat. Fiz. 99 (1985) 108. 115 ] V Fateev and A.B. Zamolodchikov, Nucl. Phys. B 280 | FS 181 (1987) 644. 116 ] F. Bais, P. Bouwknegt, M. Surridge and K. Schoutens, preprint ITFA 87-18, THU 87-21. 117 ] V. Fateev and S. Lykyanov, 1CTP preprint 6766/87. 118] J.-L. Gervaisand A. Neveu, Nucl. Phys. B 264 (1986) 557.
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Reprinted with permission from Communications in Mathematical Physics Vol. 123, pp. 627-639,1989 © 1989 Springer- Verlag
Higher Spin Fields and the Gelfand-Dickey Algebra I. Bakas*** Center for Relativity, The University of Texas at Austin, Austin, Texas 78712, USA
Abstract. We show that in 2-dimensional field theory, higher spin algebras are contained in the algebra of formal pseudodifferential operators introduced by Gelfand and Dickey to describe integrable nonlinear differential equations in Lax form. The spin 2 and 3 algebras are discussed in detail and the generalization to all higher spins is outlined. This provides a conformal field theory approach to the representation theory of Gelfand-Dickey algebras. 1. Introduction Recently Zamolodchikov investigated additional symmetries in 2-dimensional conformal field theory generated by higher spin local currents [1]. It is known that intwo dimensions the independent components of the stress energy tensor T(z), T(z), generate the (infinite) algebra of conformal transformations. The operator product expansion for the fields T(z) has the form TOW_
«
+"W+«W+....
2(z — w)* (z — wp
„,
z— w
where ••• denote all nonsingular terms. Introducing Fourier components L„{neZ), we obtain the Virasoro algebra [ A ^ J = (" - m)Ln+m + 23, (n3 - «)<Wo-
(2)
Primary conformal fields
* Supported in part by the NSF Grant PHY-84-04931 ** Address after 1 September 1988: Center for Theoretical Physics, The University of Maryland, College Park, MD 20742, USA
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I. Bakas
628
The complete set of local fields, occurring in a conformal theory consists of conformal families [
(4)
where A and A are the conformal weights appearing in the operator product expansions T{z)
(5)
are conserved, i.e., diJf(z) = 0. The simplest example (s= 1) was considered in [3], where the additional infinite dimensional symmetry algebras were identified with Kac-Moody current algebras that arise in the conformal field theory of nonlinear
(6a)
\.L„Lmi = (n-m)Ln+m + ^(n3-n)6n+mt0, LWn,Wm} = ^n(n2-\)(n2-4)5n
+ m,0
(6b)
+ b2(n-m)An+m
+ (n - m)\^(n + m + 2)(n + m + 3) - i(n + 2)(m + 2)]LB+m.
(6c)
In Eq. (6), the following identifications have been made: /l„=
+
f :LkL._k: + lx.Lm
x2, = (1 + /)(1-/); x 2(+ , = (2 + 0(1-/).
(7a)
(7c)
The highest weight representations of the operator algebra (6) were studied in [4], and as a result an infinite series of new conformal models that possess a global Z3 symmetry were constructed in two dimensions. Furthermore, it was found that
100
Higher Spin Fields and the Gelfand-Dickey Algebra
629
these new (minimal) models with central charge c
,8) - 2 ( ' - p T ^ T ) ) ; '-*■'•*■" have a hidden relation with the SL(3, R) Kac-Moody algebra, thus making it possible to prove the positivity theorem that guarantees their unitarity. The hope of obtaining a systematic description of all types of criticality in two dimensions by considering all higher spin algebras with integer (or half-integer) values of s was also expressed in [4]. It is the purpose of this paper to provide a framework in which to study higher spin operator algebras in connection with the theory of integrable nonlinear differential equations and the hidden afline Kac-Moody symmetries they contain. In particular, we show that the spin 3 algebra (6) is contained in the Gelfand-Dickey algebra of formal pseudodifferential operators introduced to describe 1 + 1 nonlinear differential equations, such as KdV and KP, in Hamiltonian (Lax) form. We shall also comment on the generalization of this approach to include all higher spin operator algebras. Incidentally, we mention that the Gelfand-Dickey algebra of formal pseudodifferential operators has been used in [5] to construct sheaves of Lie algebras on algebraic curves which provide globalized generalizations of the Virasoro algebra (in the sense that a central charge is associated to each point of a Riemann surface and each closed oriented curved on it). This constuction has stimulated many attempts to develop the operator formalism for conformal field theories defined on higher genus Riemann surfaces (see for instance [6]), as well as clarify further the role that the diffeomorphism group of the circle plays in Polyakov's approach to string theory. The crucial ingredient is that the Virasoro algebra can be embedded in the Gelfand-Dickey algebra in a natural way (see also [7]). We shall return to this point later on. Here is an outline of what follows. In Sect. 2 we review the basic theory of formal pseudodifferential operators and define the Gelfand-Dickey algebras of the type GD(SL(n)). In Sects. 3 and 4 we study in detail the Virasoro and spin 3 operator algebras, respectively, using the Gelfand-Dickey bracket of the second kind. Finally (Sect. S), we discuss the generalization to all higher spin fields and indicate possible applications of this approach to 2-dim conformal field theory and statistical mechanics.
2. The Algebra of Formal Pseudodifferential Operators Let us now present some basic facts from the theory of formal pseudodifferential operators (see for instance [8]). First, consider the ring of all differential operators L = 11.(2)3" +11,-^)3"- ' + ••• + u,(z)0 + u0(z).
(9)
(Here d denotes the derivative with respect to z.) The multiplication law is provided by the Leibniz rule
(o,(z)a').(*i(z)ao = I (' )ai(z)dkbJ{z)di+J-\
(io)
101
630
I. Balcas
which, from the point of view of one-dimensional quantum mechanics, is equivalent to the normal ordering prescription.1 Even more important is the ring of formal pseudodifferential operators that consists of the formal series L = u1I(z)d" + - + nl(r)d + iio(z)+
~£ uk{z)#.
(11)
For notational purposes, it would be convenient to use the identifications L+=L;
L_=
£
«*(*)*: resL = «_1(r),
(12)
* - - o o
where "res" stands for residue. The multiplication law for formal pseudodifferential operators is also provided by the Leibniz rule; for completeness, we mention that for all k> 0 the following identity is true:
d-'°a(z) = | p ( - l)'y_~j, ) ! Mz)d-k-'.
(13)
At this point notice that primary conformal fields have a natural interpretation in the ring of formal pseudodifferential operators. In particular, by introducing the bracket [L ls L2]:= LJOLJ — L2°L„ we observe that [£l(z)<5,£2(z)d] = (£l(z)£2(Z) - e\(z)£l(z))8
(14)
and l£(z)d,(p(z)dkmoddk-l]
= (e(z)(p'(z)-ke'(z)
(15)
Equation (14) implies that the Lie algebra of vector fields on the circle is contained in the algebra of formal pseudodifferential operators, while (15) suggests that the operator (p(z)^ mod d*~1 represents a primary field with conformal weight A = — k (cf. Eq. (31)). The commutator [Llt L2] of two formal pseudodifferential operators Lj and L2 with degrees n t and n2, respectively, has degree n1 + n2 — 1. Therefore, all formal pseudodifferential operators of negative degree only form an algebra with respect to [, ] also known as the Volterra algebra. For convenience, we drop the multiplication symbol °. From now on, we let
X=td-%(z)
(16)
(=i
represent a generic element (symbol) of the Volterra algebra—usually, only a finite number of x.'s will be taken to be nonzero. Then we may define a pairing between the space of differential operators L and elements of the Volterra algebra by the formula [8]:
(17)
This enables us to think of the space of differential operators L as being the 1
One may think of any such operator L as the normal ordered operator corresponding to the (classical) function u,[z)z" + u„_i(r)£"~ ' + ••• + Utiz'iz + u„(z) on the plane with canonical coordinates z and f
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Higher Spin Fields and the Gelfand-Dickey Algebra
631
(smooth) dual of the Volterra algebra. Since the residue of the commutator of any two (formal) pseudodifferential operators is always a total derivative, we have that
(18)
which defines the coadjoint representation of the Volterra algebra. For a given L = uH{z)
(19)
let Xf be the formal sum mthXi = j ^ - .
(20)
We can use the coadjoint representation of the Volterra algebra in order to define the Poisson bracket {f,g}2h.= ins(lL,X^ + Xg) (21) for any two functional/, g of u 0 ,...,!<„_!. Note that in Eq. (20) we have not included the i = n+l term allowed by the residue duality (17). This is justified because, in any case, [L,X/] + is a differential operator of degree at most n — 1; and so in computing the residue of [L, Xf~\ + Xr only terms with 1 ^ i ^ n will contribute. The Poisson bracket (21) associated with the space of differential operators (19) is the Gelfand-Dickey bracket of thefirstkind introduced to describe integrable nonlinear differential equations in Lax form (see for instance [8]). However, it is known that integrable systems in 1 + 1 dimensions are bi-Hamiltonian in the sense that they can be equivalently described using two different kind of Poisson brackets. The Gelfand-Dickey bracket of the second kind is defined [7,8] as {f,g}^:=iTes(VXf(L)Xt\
(22a)
where VXf(L) = L(XfLU - (LX,)+L.
(22b)
We note that the Gelfand-Dickey bracket of the second kind is more general than the first one, since an arbitrary shift of the form L-*L + k (where A is a constant) yields VX/(L)->VXf(L)-KL,X,l
+
,
(23)
i.e., [L, X] + behaves like a "coboundary" of VX(L). For this reason, in what follows, we choose to work with the Gelfand-Dickey bracket of the second kind. At this
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point, we note that VX(L) may be viewed as the coadjoint action operator of the algebra of formal series (16) with respect to a new commutator [, ]. The latter is determined by the equation {L,lX1,X2}y.=
iKs(VXl(L)X2),
(24)
thus generalizing (18). The algebra constructed this way from the space of differential operators (19), with [, ] as its bracket, is called the Gelfand-Dickey algebra GD(GL(n)), where GL(n) denotes the general linear algebra in n dimensions.2 It will be shown later on that this provides a natural generalization of the Virasoro algebra, while the associated operator VX(L) generalizes the coadjoint action operator of the Virasoro algebra (in the sense that AdJ/(L - d") = VXf(L)). Next, we restrict ourselves to G = SL{n) that arises as a special case of the GD(GL(n)) algebra. The GD(SL(n)) algebra is constructed from the space of all differential operators (19) with u,,., =0, i.e., L = d* + um-2(z)d"-2 + - + u0(z),
(25)
and as we shall see, it is most suitable for describing higher spin operator algebras. In analogy with the GD(GL(n)) algebra, we define the bracket of the second kind by Eq. (22). But since u„_ 2 = 0, the i = n term in the formal sum (20) is meaningless unless it is taken to be zero. In such case, straightforward calculation shows that the operator VXj(L) involves a term of degree n — 1 and so the choice u„.l = 0 does not seem to be invariant. This problem is resolved if one considers * / = I
1
^ i # - + d"n*..
(26)
with x„ determined by the requirement res [L, X/\ — 0—as it turns out, res [L, Xf~] is the coefficient of the term with degree n - 1 in VX/(L). Therefore, the GD(SL(n)) algebra is well defined provided that x„ is chosen appropriately. In what follows we show that the Virasoro, as well as higher spin operator algebras, are described in terms of GD(SL(n)) for all n = 2,3, 3. L = d2 + u and Spin 2 Following the general construction described above, we consider Xf = 8-l^+8-2x2
(27)
with x2 determined by the requirement res [L, X{~\ - 0. Explicit calculation shows that res [d2 + u, X/] = 2x'2 - (df/du)" and so the GD(SL(2)) algebra is well-defined provided that , 1 *2 = 2 2
(28)
Gelfand-Dickey algebras labeled by more general simple Lie algebras G, GD(G), have been introduced in [9] in connection with generalized hierarchies of nonlinear differential equations in 1 + 1 dimensions
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633
Furthermore, we find that in this case
ifsfy
V
*W — l\t)
, fdfX (bf
-2u[fu)-U\fu)-
(29)
Therefore, the Gelfand-Dickey bracket of the second kind takes the form {Mzngtom^-jdz-^G^-^,
(30a)
where Cu,f, = i ^ + « ( ^ + ^"(z).
(30b)
The Poisson bracket (30) has already been used in the Hamiltonian formulation of the KdV equation, as well as in 2-dim conformal field theory (see [10] and references therein). This is the bracket between any two functionals / , g defined on the dual of the Virasoro algebra. Moreover, the operator 6^ describes the conformal variation of the quadratic differentials u(£) and hence the coadjoint action of the Virasoro algebra. The commutation relations between the (coordinate) functionals u are easily found to be {u(z)Mz')f^„ = Hz) + " ( z W ( z - A +tf\%z~ z')-
(31)
This result is not surprising at all because the space of differential operators L = d2 + u is known to be isomorphic with the (smooth) dual of the Virasoro algebra (31). Recall that under arbitrary reparametnzations of the circle Z-KT(Z), the operators d2 + u transform as d1 + u^o,-it\d2
+ au)&-m,
(32a)
where 'u(z) = &McW) + \(^-\(£jy
(32b)
Also, it is known that the space of quadratic differentials is isomorphic with the (smooth) dual of the algebra of vector fields on the circle, and so the desired correspondence is established with the aid of densities of weight — \ [10]. The value of the central charge of the Virasoro algebra (31) is c = 6 (cf. Eq. (2)). This is because we chose to work with the differential operator L = d2 + u. Having chosen Xd2 + u instead (with constant X = c/6), the Gelfand-Dickey bracket of the second kind would have been described by (30) with (9U — c/1233 + ud + du. This way, we conclude that the GD(SL(2)) algebra provides a realization of the Virasoro algebra. We also remark that for d2 + u the Gelfand-Dickey bracket of the first kind is
{MzngW))}^
= idzJ-^l(-
23^-^1.
(33)
This gives only coboundary contributions (~ dzS(z — z')) to the commutation relations of the Virasoro algebra, as expected from Eq. (23) that relates the Gelfand-Dickey brackets of the first and second kind in the general case.
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4. L = d3 + utd + «0 and Spin 3 For any functional/[u^uj, let us consider the formal sum (cf. Eq. (26))
x^d-^
+ e-^+d-W
04)
3u0 du, In this case we find that res \_d3 + «,d + u0, Xf~\ = 3x'3 + (Sf/Su0)'" - 3(<5//<5u,)" + (ui(<5//<5u0))' and so, according to the general theory, the GD(SL(3)) algebra is well defined provided that x3 satisfies the equation
^(0-(0'-(»# Furthermore, we find by a straightforward (but lengthy) calculation that Vx (L) is given by VXf(d3 + uld + u0) = u1d + u0,
(36a)
where
-<0-<0-(^)"-«1(0-«o(0 + «„l ^)" + «,(«,£)' + Mlxi - (u, j£)' - 2 U l ( 0 - ( u o 0 , (36c)
and x 3 satisfies the requirement (35). The equation above describes the coadjoint action of the GD(SL(3)) algebra in the sense that AdXf(L-d3):= VXf(d3 + utd + u0) = u1d + u0. Comparison with Eq. (26) suggests that (36) generalizes the coadjoint action of the Virasoro algebra in a very interesting way. To be more precise, let us examine first the transformation properties of the operators d3 + u1(z)d + u0(z) under arbitrary reparametrizations of the circle z -»a{z). Explicit computation yields 83 + Ul(z)d + u0(z)^a'-2(83
+ °Ui(z)d + 'U0(Z))G'~ \
(37a)
where »u1(r) = <7'2u1((T(Z)) + 2Sff(z), 'u0(z) =
(37b) (37c)
Here, Sc(z) = (o"'/o')-{3/2)(o"/o')2 denotes the Schwartzian derivative of the diffeomorphism a. Note that u^z) transforms (up to the Schwartzian term) as a quadratic differential, while (37c) suggests the presence of a spin 3 field in the formalism. In particular, using (37b), (37c), we have that
106
Higher Spin Fields and the Gelfand-Dickey Algebra
535
*u0(z) - iX(z) = a'3 fu0(
^FU'MZ))
\
(38)
and so the combination u0(z) — \u\(z) transforms as a conformal field of weight 3. In establishing these results, we found it most useful to think of the operators L = d3 + uxd + u0 as acting on densities of weight —1 rather than on scalar functions. In fact, as we shall demonstrate later on, there is a natural generalization of the transformations (32) and (37) to any differential operator L = d" + u„ _ 2d""2 + —h u0 viewed as acting on densities of weight — (n — l)/2. At the moment, we would like to investigate the GD(SL(3)) algebra in more detail, since Eq. (37b) indicates that the Virasoro algebra is contained as a subalgebra in GD(SL(3)). For this, we make use of the Gelfand-Dickey bracket of the second kind that is associated with the space of differential operators d3 + utd + u0. Recalling Eq. (36) for the coadjoiqt action, we obtain the following expression for the bracket: {/(u1(z),uo(z)),0(«1(z'),«o(2'))}al Ja3+u,d+»o
- «oW(
ITTSY
Su0(z)J
- («i«>X77*Y " 4u0(z) \ Su^z)/ V
+ S5uo0(z)\ ^LA&^J
"VM*))
»■" K^sss)'" {""mf
+
5f 5M
O(2)
3VI(Z1K(ZV
~ (u°m£(
(39)
Note that the bracket between the (coordinate) functionals u, is equal to {uMuiWYXu^ = («i(*) + UiWWA* - A + 2d38(z - z'), (40) which shows that the Virasoro algebra is, indeed, contained in GD(SL(3)). However, thanks to all the terms that appear in Eq. (39), this is not the whole story. Further calculation shows that for w{z)'= u0(z) — \u\(z) the following is true: {Ul(z), H)}P+„ia+i(o = W) + 2w(*))dA* - A
(41)
i.e., w(z) transforms as a local field of conformal weight 3. Moreover, we find that the Gelfand-Dickey bracket for the fields w is given by Mz), wM$ +He+Uo = - R5<5(z - z') - i(ufo) + u\{f))dAz - zO)
-A("i(z)+«i(zm3*z-z') + i(ul(z) + u'l(z'))dAz-z')(42) Consequently, u^z) and w(z) form an algebra with quadratic determining relations
107
636
I. Bakas
(40H42). Here, the central charge of the Virasoro algebra (40) is c = 24. Note, however, that all other values of c are easily obtained by considering L = kd3 + Uid + u0 with A = c/24. For completeness, we mention that in this case the Gelfand-Dickey bracket of the first kind is equal to
"••^-'Ks&C+i&C)}
<431
Shifting u0(z) (and hence w(z)) by a constant is equivalent to modifying the Gelfand-Dickey bracket of the second kind by the expression (43). It can be readily checked that such modifications do not alter the commutation relations (40)-{42) at all. On the other hand, we may shift ut(z) by a constant (which is equivalent to redefining the vacuum expectation value of the stress-energy tensor of the theory). For u^-^u^z) — 1, the commutation relations (40)-(42) become K(z), Ul(z')} - («,(z) + 11,(20)3,** - z') + 2d}S(z - z') - ZdA* ~ A {Ml(z), w(z')} = Wz) + 2w(z'))d,6(z - z'), 3 {H
(44a) (44b)
- $(uftz) + u\(z'))dAz - z') + §(Ul(z) + Ul(z'))dAz ~ *') - £( U l (z) + utfWldiz - z') + i K ( z ) + u'fr'WAz - z')- (44c) (Here, for convenience, we have dropped the labels of the Gelfand-Dickey bracket.) Although the algebra (44) is not a Lie algebra, it has a very natural interpretation in the context of 2-dim conformal field theory. Comparison with the commutation relations (6) shows that the spin 3 operator algebra is a particular representation of (44). To illustrate this result in more detail, we point out that the quadratic terms appearing on the right-hand side of Eq. (44c) need to be regularized upon quantization. An appropriate regularization (which is also consistent with the algebra commutation relations) is acquired by assigning (A(z) + A(z'))dz6(z - z') + ^
5
- Sd3 + Ad^z - z') - [i(M,(z) +
- i(u,(z) + Ul(z'))dl + A("i(z) + uUWW
Ul(z'))dz
- z')
to the classical quantity (u\(z) + u\(z'))dz6(z — z'). In the expression above, A(z) is essentially the normal ordered operator that represents u\{z) with Fourier modes given by Eq. (7). This way, the right-hand side of Eq. (44c) assumes the form - \(dl - 583 + 4dz)d(z - z') - i(/l(z) + A(z'))dxd(z - z') -M5("i(z)
+ u,(z'))a23 - 3«(z) + u';(z')& - 8(u,(z) + u ^ z ' ) ) ^ ] ^ - z'),
and so Zamolodchikov's spin 3 operator algebra is a well defined representation of (44) with W(z)*->(i/v/3)w(z), T(Z)<-»M,(Z), and c = 24. In general, if we consider L = (c/24)d3 + uid + u0, the operator algebra (6) will result for all values of the central charge c.
108
Higher Spin Fields and the Gelfand-Dickey Algebra
637
5. Higher Spin Fields and Conclusions Next, we discuss briefly the relation between higher spin n operator algebras and the Gelfand-Dickey algebras GD(SL(n)) constructed from the space of differential operators L = 5" + uH-2{z)dH~2 H 1- u0(z). It is relatively easy to show that in this case the Gelfand-Dickey bracket of the second kind for the (coordinate) functionals u„_2 is equal to {uB-2(z), un-2(z')}™ = (uK.2(z) + uH.2(z'))dAz - z') + ^8(z
- z')
(45)
with cK = n(n— 1)(« + 1), which in turn implies that the Virasoro algebra is a subalgebra of GD(SL(n)) (see also ref. [5,7]). Alternatively, this result is established using the transformation properties of the operators d" + u,,_2(z)3""2 H h u0(z) under arbitrary reparametrizations z -*a{z). Explicit calculation shows that a" + «„.2(z)5"-2 + -+U 0 (z)^(7'- ( " +1,/:2 (5- + X - 2 ( ^ " 2 + -+'u 0 (z)K" < "" 1 ) / 2
(46a)
with X-2(Z) = °'2Un-2(°(z)) + T ^
:
~ ^ S M
(46b)
which generalizes the transformations (32) and (37) for all values of n. For clarity we note that under arbitrary reparametrization z -♦ a{z), the form of the operators L = dn + u„-2dn~2 H hu0 m a y n o t be preserved due to the occurrence of the term - ( « ( " - l)/2){ff"/a"'*1)ff'~i of degree n- 1. This will definitely be the case if we assume that the operators L act on scalar functions. However, if we think of them as acting on densities of weight — (n — l)/2 (as illustrated by (46a)), all terms of degree n — 1 cancel, which makes the choice u„_ t = 0 consistent. We point out that this is equivalent to the requirement res [Xf, L] = 0 imposed for well-definiteness of the GD(SL(n)) algebras earlier on. Further study of the transformation (46a) shows that up to Schwartzian terms, uH.2{z), u»_3(z),...,u0(z) (or appropriate combinations of them) behave as conformalfieldsof weight 2,3,..., n, respectively. For instance, forn = 4 wefindthat "Ml(z) = ff'^.Wz)) + 2&a"u2{o{z)) + SS'M X(z) =
(47a)
(47b)
In analogy with the n = 2,3 cases that we have already investigated, the GelfandDickey bracket for these fields would provide us with an algebra equivalent to the spin n operator algebra of 2-dim conformal field theory. This way, we identify the space of differential operators L = 5" + u„_25*"2H hu 0 with the (smooth) dual of the spin n operator algebra. Using the coadjoint action operator (22b), we may extend the methods of ref. [10] to all higher spin operator algebras and study the geometry of the resulting coadjoint orbits. Such orbits might be found useful
109
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I. Baku
for investigating the geometric role of higher spin fields. We intend to study this problem in more detail elsewhere. Moreover, highest weight representations of all spin n operator algebras are expected to be of paramount importance in quantum conformal field theory, as well as in statistical mechanics in 2 dimensions. According to the general philosophy of 2-dim critical phenomena, the investigation of critical singularities reduces to the problem of finding appropriate conformally invariant quantum field theory solutions (see [2,4] and references therein). Such conformal (minimal) models correspond to degenerate Verma module representations of the underlying sym metry algebra for discrete values of the central charge c. For the spin 2 algebra, the corresponding discrete values of c are given by 1 — (6/p(p +1)) w ' t n p = 3,4,5,... [11], while for the spin 3 operator algebra by Eq. (8). In generalizing these results to higher spin operator algebras, we realize that unitary representations of the GD(SL(n)) algebras play an important role. Taking into account the embedding of the Virasoro algebra in GD(SL(n)) described by Eqs. (45) and/or (46), wefind(as a result of some preliminary computations) that the following set of discrete values c = (n-l)(l-,^-^-\
p = n+l,n + 2,...
(48)
is associated with (minimal) models of spin n operator algebras. Details of the underlying calculations will be presented in [12]. However, it is worth mentioning here that the representations of affine Kac-Moody algebras are closely related with the theory of integrable nonlinear diferential equations and hence with the Gelfand-Dickey algebras (see, for instance, [13] and references therein). In particular, the GD(SL(n)) algebra may be viewed as a reduction of the SL(n) Kac-Moody algebra. This seems to provide the basic ingredient for understanding hidden relations between (minimal) conformal models of spin n operator algebras and highest weight representations of the SL(n) Kac-Moody algebras in favor of showing the positivity theorem that guarantees the unitarity of these models. Along these lines, it would be most interesting to generalize the Goddard-Kent-Olive construction [11] to all values of n in a well prescribed way. Finally, we note that it is possible to extend our results to superconformal (and more generally to higher half-integer spin) operator algebras by using the supersymmetric generalization of the Gelfand-Dickey algebra of formal pseudodifferential operators introduced in [14] to study the super KP hierarchy of nonlinear differential equations. This will be the subject of future publications [12]. For completeness we mention that certain results somewhat related to ours have also been discussed by others [15]. Acknowledgements. I am grateful to Prof. Y.-S. Wu for a stimulating conversation during the course of this work. I also thank the theorists at Syracuse University for their encouragement to present these results.
References 1. Zamolodchikov, A.B.: Theor. Math. Phys. 65, 1205 (1985) 2. Belavin, A.A., Polyakov, A.M., Zamolodchikov, A.B.: Nucl. Phys. B241, 333 (1984)
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Higher Spin Fields and the Gelfand-Dickey Algebra
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3. Knizhnik, V., Zamolodchikov, A. B.: NucL Phys. B247, 83; (1984); Gepner, D., Witten, E.: Nucl. Phys. B278, 493 (1986) 4. Zamolodchikov, A. B., Fateev, V. A.: Nucl. Phys. B280, [FS18], 644 (1987) 5. Beilinson, A. A., Manin, Yu. I., Schechtman, V. V.: preprint (1986) 6. Alvarez-Gaume, L., Gomez, G, Reina, G: Phys. Lett. B190, 55; (1987); Vafa, C: Phys. Lett. B190, 47 (1987); Witten, E.: Commun. Math. Phys. 113, 529 (1988) 7. Khovanova, T. G.: Funct. Anal. AppL 20, 332 (1986) 8. Gelfand, I. M., Dorfman, I.: Funct. Anal. Appl. 15,173 (1981); Lebedev, D. R., Manin, Yu. I.: Funct. Anal. Appl. 13, 268 (1979); Adler, M.: Invent. Math. 50, 219 (1979); Dickey, L. A.: Commun. Math. Phys. 87,127(1982); Manin, Yu. I.: J. Sov. Math. 11,1 (1979); Guillemin, V., Steinberg, S.: Symplectic techniques in physics. Cambridge: Cambridge University Press 1984 9. Drinfeld, V. G., Sokolov, V. V.: Sov. Math. Dokl. 23, 457 (1981) 10. Kirillov, A. A.: Funct. Anal. AppL 15, 301 (1981); Bakas, I.: NucL Phys. B302, 189 (1988); Witten, E.: Commun. Math. Phys. 144, 1 (1988) 11. Friedan, D., Qiu, Z, Shenker, S.: Phys. Rev. Lett. 52,1575 (1984); Goddard, P., Kent, A., Olive, D.: Phys. Lett. B152, 88 (1985) 12. Bakas, I.: in preparation 13. Drinfeld, V. G„ Sokolov, V. V.: J. Sov. Math. 30, 1975 (1985); Frenkel, I. B.: In: Lie algebras and related topics. Proceedings Lecture Notes in Mathematics vol. 933, p. 71 Berlin, Heidelberg, New York: Springer 1982; Jimbo, M., Miwa, T.: In: Integrable systems in statistical mechanics. D' Ariano, G. M. (ed.) et al.; Singapore: World Scientific, 1985 14. Manin, Yu. I., Radul, A. O.: Commun. Math. Phys. 98, 65 (1985) 15. Yamagishi, K.: Phys. Lett B205, 466 (1988); Bilal, A., Gervais, J.-.L.: Phys. Lett. B206, 412 (1988) ThierTy-Mieg, J.: DAMTP preprint (1987) Communicated by L. Alvarez-Gaume Received November 5, 1988 Note added in proof. Recently I became aware of reference [16] where Gelfand-Dickey algebras have also been used in the study of higher spin operator algebras. 16. Mathieu, P.: Phys. Lett. B208, 101 (1988)
Ill
Reprinted with permission from Annals of Physics Vol. 203, No. 1, October 1990 © 1990 Academic Press, Inc. (New York and London)
Toda Theory and ^-Algebra from a Gauged WZNW Point of View J. BALOG,* L. FEHfcR,1 AND L. O'RAIFEARTAIGH Dublin Institute for Advanced Studies, 10 Burlington Road, Dublin 4, Ireland P. FORGACS* Max-Planck-Institut fur Physik und Astrophysik (Wemer-Heisenberg-Institut fur Physik), P.O. Box 401212, Munich, Federal Republic of Germany AND A. WIPF Institutfur Theoretische Physik, ETH-Honggerberg, CH-8093 Zurich, Switzerland Received December 14, 1989
A new formulation of Toda theories is proposed by showing that they can be regarded as certain gauged Wess-Zumino-Novikov-Witten (WZNW) models. It is argued that the WZNW variables are the proper ones for Toda theory, since all the physically permitted Toda solutions are regular when expressed in these variables. A detailed study of classical Toda theories and their Tlf-algebras is carried out from this unified WZNW point of view. We con struct a primary field basis for the ♦'-algebra for any group, we obtain a new method for calculating the iV-algebra and its action on the Toda fields by constructing its Kac-Moody implementation, and we analyse the relationship between Tt^-algebras and Casimir algebras. The ^-algebra of G2 and the Casimir algebras for the classical groups are exhibited explicitly.
© 1990 Academic Pren, Inc.
I. INTRODUCTION
Two dimensional conformally invariant soluble field theories are based on various extensions of the chiral Virasoro algebras. The best known extension is the Kac-Moody (KM) extension [ 1 ] , whose most prominent Lagrangean realization is the Wess-Zumino-Novikov-Witten (WZNW) model [2]. There are various indications that the KM algebra may even underlie all the rational conformal field theories. For example, the Goddard-Kent-Olive (GKO) construction [3] * On leave from Central Research Institute for Physics, Budapest, Hungary. * On leave from Bolyai Institute, Szeged, Hungary.
112 TODA THEORY AND T^-ALGEBRA
77
generates a huge class of rational conformal field theories. Another extension is the so-called iF-extension, which is a polynomial extension of the Virasoro algebra by higher spin fields. The study of polynomial extensions of the Virasoro algebra was initiated by Zamolodchikov [4]. Later it was realized [5, 6] that a large class of polynomial extensions of the Virasoro algebra can be constructed by quantizing the second Gelfand-Dickey Poisson bracket structure of Lax operators, used in the theory of integrable systems. These ^-algebras proved very fruitful in analysing conformal field theories and they have become the subject of intense study [5-8]. Recently it has been found by Gervais and Bilal that Toda theories provide a realization of 1^-algebras [8,9]. Toda theories are important in the theory of integrable systems and include the ubiquitous Liouville theory, which, among other things, describes two dimensional induced gravity in the conformal gauge. There are a number of results suggesting that Toda theories must be closely related to WZNW models. First, in both cases the fields can be recovered from the generators of the respective extended Virasoro algebras (KM and iST-algebras) by means of linear differential equations [8]. Second, the Gelfand-Dickey Poisson bracket structure can be obtained by a Hamiltonian reduction from a KM phase space [10]. Finally, it has been shown by Polyakov [11] that two dimensional induced gravity (in the light cone gauge) exhibits (left-moving) SL(2, R) KM symmetry. In a recent letter [12] we have shown that the exact relationship is that Toda theories may be regarded as WZNW models (based on maximally non-compact, simple real Lie groups) reduced by certain conformally invariant constraints. To be more precise, Toda theory can be identified as the constrained WZNW model, modulo the left-moving upper triangular and right-moving lower triangular KM transformations, which are gauge transformations generated by the constraints. The advantages of treating Toda theory as a gauge theory embedded into a WZNW model are the following: First, the coordinate singularities of Toda theory disap pear by using the WZNW variables. Second, the ^-algebra of Toda theory arises immediately as the algebra formed by the gauge invariant polynomials of the con strained KM currents and their derivatives. Third, the general solution of the Toda field equations is easily obtained from the very simple WZNW solution. Finally, there are natural gauges which facilitate the analysis of the theory. In this paper we exploit the embedding of Toda theory into the WZNW model to obtain a number of new insights and results about the structure of Toda theory and iF-algebra. All our considerations are classical. We hope that their quantum generalizations will provide new constructions of quantum Toda theories [13] and ^-algebras. We first set up a Lagrangean framework for the WZNW-Toda reduction, namely we establish that Toda theories can be identified as the gauge invariant content of certain gauged WZNW models. Our gauged WZNW models differ from the usual gauged WZNW models [14] used in the path integral realization of the GKO con struction not only in the non-compactness of our groups, but also in that instead of a single diagonal subgroup we gauge two subgroups of the left x right WZNW group, the upper triangular maximal nilpotent subgroup on the left and the lower
113 78
BALOG ET AL.
triangular one on the right hand side. The nilpotency of the triangular subgroups is crucial to this ambidextrous generalization of the usual vector gauged WZNW models, and in fact the nilpotency of the gauge group is the reason for the appearance of the simple polynomial structures in Toda theory. The constrained WZNW model is recovered in this framework by an appropriate partial gauge fixing which leaves the left- and right-moving triangular gauge transformations mentioned earlier as a residual gauge symmetry. In most of our considerations we rely heavily on the use of a class of natural gauges used in studying the gauge invariant differential polynomials in the review paper [10] by Drinfeld and Sokolov. The basic property which makes the DS gauges convenient is that in each DS gauge the surviving components of the KM current serve as a basis for the #"-algebra. Working in the DS gauges, we give a simple algorithm to find the KM transfor mations which implement the canonical transformations generated by the i^-algebra. This provides us with a new method both for computing the iS^-algebra and for determining the action of the iF-algebra on the Toda fields. Our method crucially depends on using the embedding WZNW theory and its full, non-con strained KM algebra. We illustrate the method on the examples of A2 and B2 and demonstrate its power by computing the complete iF-algebra relations for the rather non-trivial example of G2. We find a DS gauge which enables us to construct a primary field basis of the iST-algebra. As far as we know a general algorithm for constructing primary ^-generators has not been known before, although such generators have been found in low dimensional examples [6]. We note that even the existence of a primary field basis is not completely trivial, since such a basis is constructed by a non-linear transformation [6] even if one starts from "^-generators transforming in a linear (inhomogeneous) manner under the Virasoro algebra. Our construction of the primary TiT-generators is based on a special SL(2, R) subgroup of the WZNW group, which plays an important role throughout the theory. The primary ^"-generators are associated in a natural way to the highest weight states of this SL(2, R) in the adjoint representation of the WZNW group. There have been attempts [15] at constructing polynomial extensions of the Virasoro algebra from a KM algebra by using the higher Casimirs of the underlying Lie algebra similar to the manner in which the second order Casimir is used in the Sugawara construction. On the quantum level these Casimir algebras close only under very restrictive conditions on the KM representation. We show that the leading terms (i.e., terms without derivatives) of the i^-generators are always Casimirs, and that the Poisson bracket version of the Casimir algebras always close. In fact, we prove that these classical Casimir algebras are obtained from the corresponding iS^-algebras by a certain truncation, and thus the Casimir algebras can be used to investigate the leading terms of the i^-algebras. For the classical Lie algebras A,, Bh and C, we give the explicit form of the Casimir algebra. We also consider the existence of quadratic relations for the Ti^-algebras. In the case of the Ah B,, and C, Lie algebras it is easy to display ^"-generators with quad-
114
TODA THEORY AND iF-ALGEBRA
79
ratic relations. The above mentioned relation between the Casimir and i^-algebras shows that for the other Lie algebras the ^-relations are necessarily of higher order. Finally, we investigate how the Toda fields can be reconstructed from the ^-generators. This reconstruction is a reduced version of the reconstruction of the group valued WZNW field from the KM currents, and this tells us that every Toda solution with regular iF-generators can be represented by a regular WZNW solu tion. The reconstruction problem leads us to studying the differential equations satisfied by the gauge invariant components of the constrained WZNW field. This way we recover the Lax operators studied in [10], which also appear in the generalized Schrodinger equations of Ref. [ 8 ] . For A,, Bh Ch and G2 the reconstruction problem can be reduced to solving a single ordinary differential equation of the order of the defining representation of the corresponding algebra, in all other cases one inevitably has a pseudo-differential equation. We will see that one has a single ordinary differential equation exactly when the representation in which the group valued WZNW field is taken is irreducible under the SL(2, R) sub group mentioned earlier, and that in general the structure of the pseudo-differential operator depends on the decomposition of this representation under the SL(2, R) subgroup. The plan of the paper is the following: In Section II we present a short review of the reduction of the WZNW model to Toda theory and describe the gauged WZNW framework. We elaborate on the role of the residual gauge invariance and on the gauge invariant quantities in Subsection II.2. The longest and most impor tant section is III. We start it with the definition of the liT-algebras. In Subsec tion III. 1 we present the construction of the Drinfeld-Sokolov gauges and observe that in these gauges the ^"-algebra reduces to the Dirac bracket algebra of the sur viving KM current components. In Subsection III.2 we exhibit a primary field basis of the "^-algebra and illusrate it with B2. In Subsection III.3 we give an algorithm to implement the action of the ^-algebra by means of KM transformations and illustrate the procedure with A2 and B2. In Subsection III.4 we first display a sub class of Drinfeld-Sokolov gauges where the ^-algebra relations are quadratic for A i, Bh and C,. Then we introduce the "diagonal" gauge, which is frequently used in Section IV, and briefly discuss the related Miura-transformation. Subsection IV.l contains a detailed analysis of the relation between the Casimir Poisson bracket algebras and the Ti^-algebras. In Subsection IV.2 we present the explicit Poisson bracket algebra of the Casimir operators of the classical Lie algebras Ah B,, and C,. In the last section, V, we study the differential and pseudo-differential operators which appear when the Toda-fields are reconstructed from the iS^-generators (or the constrained WZNW fields are reconstructed from the KM currents). There are three appendixes; Appendix A contains our conventions and some important group theoretical results, Appendix B contains the complete if(G2) algebra and Appendix C contains the details of the calculations of the Casimir algebras. We end the paper by summarizing the main results and giving some conclusions.
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BALOG ET AL.
II. TODA FIELD THEORY AS A GAUGE THEORY
In this section we first summarize the main points of the redution of WZNW models to Toda theories. Then we show how to set up a Lagrangean framework for the reduction, using an ambidextrous generalization of the usual vector gauged WZNW models. Then we elaborate on the concept of residual gauge transforma tions and on the corresponding gauge invariant quantities. In particular, we point out that in the WZNW framework 1^-algebras appear naturally as symmetry algebras of Toda theory. II. 1. Toda Theory as a Gauged WZNW Model The so called Toda field equations constitute a rather interesting set of integrable (soluble) equations. These equations appear naturally in various problems (cylindrically symmetric instantons [16], etc.) and they can also be thought of as a generalization of the ubiquitous Liouville equation: d+ d_
where M = const..
(2.1)
Now the Toda equations are given as a + <5_^ + ^|a| 2 A/"exp j i £ K ^
= 0,
(2.2)
where Krf is the Cartan matrix1 of a simple Lie algebra, A denotes the set of simple roots and the A/°"s are (positive) constants. The corresponding Lagrangean is
where K is the coupling constant of the theory. Clearly (2.2) reduces to the Liouville equation (2.1) by making the simplest choice for Kafi, namely the choice when K„f is just a number (corresponding to a rank one algebra). In fact Toda field theories are also distinguished by being the only two dimensional, nontrivial conformally invariant models which are soluble [8, 16] in the class of scalar theories without derivative couplings. These theories possess an imporved energy-momentum tensor
with vanishing trace, 8 + _ =0, on shell. Interestingly, the general solution of (2.2) can be written in closed form [16]. 1
Our conventions are collected in Appendix A.
116 TODA THEORY AND iST-ALGEBRA
81
Let us recall first, how Toda theories can be regarded as constrained WZNW models. We start with the WZNW action based on a connected real Lie group G (with maximally non-compact simple real Lie algebra (S)
+
isJ* Tr «'- , * ), >-
(15)
where g is a group-valued field and B3 is a three dimensional manifold whose boundary is Minkowski space-time. We choose the coupling constants K and k to be related by the equality k= —ATIK. This action possesses left and right KM symmetries. Their Noether currents associated to some Lie algebra element, A, are given as J=K(d+g)g~l
JW = Tr(lJ),
J=-Kgl(d_g).
7(A) = Tr(A.J),
Thefieldequations are equivalent to the conservation of the left and right currents: d_J = 0,
d + J=0.
(2.7)
Let now n" and v" (a e A) be arbitrary positive numbers and let us denote the set of positive roots by
J(£_J=-KV",
J(Ev) = 0,
7(£_„) = 0,
zeA
(2.8)
the equations of motion of the WZNW theory (2.7) reduce to the Toda field equa tions (2.2). To prove this result we start with the (local) Gauss decomposition g = ABC
(2.9a)
of the group-valued field g, where A = exp\ £ U *+
O'EX J
C = exp( £ U *+
c*E_\ J
(2.9b)
This group-valued Gauss decomposition is locally unique for Lie groups G with maximally non-compact Lie algebras.
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BALOG ET AL.
Now exploiting the fact that n* and v" are zero for all but the simple roots, the constraints (2.8) can be rewritten as /r'<5_/l=xi|a|2v"£.exp{ix 1 P J * 2 ( d + C ) C - ' = £ i|a| Ai"£_ a exp{i £
K^A J
(2.10)
K^A
Substituting (2.10) into thefieldequations (2.7) one indeed recovers the Toda equa tions (2.2) (with M" = \a\2 ft'v"). It can be shown that this reduction is canonical in the sense that the Poisson brackets of the Toda variables ^ and ^ can be calculated either from the Toda or from the WZNW action (as a requirement, this fixes the relationship between the coupling constants). We remark that the famous Leznov-Savaliev general solution of the Toda field equations [16] can be derived effortlessly from the general solution of the WZNW field equations (2.7), g(x\x-) = gL{x + ) . g R ( x
),
(2.11)
where gL and gR are arbitrary group-valued functions constrained only by the boundary conditions and there is an obvious constant-matrix ambiguity in the definition of gh and gR. The general solution of the Toda equations can be obtained from (2.11) by first imposing the constraints (2.8) and then decomposing the constrained WZNW solution according to (2.9) [12]. In Section V we shall show that it is equally easy to recover the solution of the Toda field equations in the form recently found by Gervais and Bilal [8] from (2.11). As the quantization of Liouville and Toda theories is expected to be simpler in the WZNW formulation, it is worthwhile to find a Lagrangean realization of the reduction of the WZNW model to the Toda theory. In the following we show that an ambidextrous generalization of gauged WZNW models [14] provides a natural framework to carry out this reduction. For example, gauged WZNW models turned out to be useful in the Lagrangean description of the Goddard-Kent-Olive coset construction (GK.O) [3]. We shall need the Polyakov-Wiegmann identity [17] expressing the WZNW action for the product of three matrices A, B, C as the sum of the respective actions for A, B, and C, modulo local terms: S(ABC) = S(A) + S(B) + S{C) + K | d2xTr{(A
' d _ A)(d +
+ (B~l d_B)(d+C)C~i
B)Bl
+ (A-1 d_A)B(8+C)C-lB~i}.
(2.12)
118 TODA THEORY AND 1^-ALGEBRA
83
Next we want to consider the gauged version of the WZNW theory, i.e., we are looking for an action invariant under the transformations, g^agp-1,
*eH,peft,
(2.13)
where a, fi are functions of both x+ and x~, and H, ft are two isomorphic subgroups of G. Let us first recall the "usual" gauged WZNW models [14]. In the standard case one gauges a diagonal (vector) subgroup, H, of the Kac-Moody group G L xG R . Now the transformation of g under the vector subgroup is given as
g^ygy-1,
y(x+,x)eH.
(2.14a)
It is easy to see that the action functional I(g,h,Ji) = S(hg7i-1)-S{h}i-1),
h,%eH
is gauge invariant, provided (2.14a) is supplemented with 7i->7iy-1.
h-+hy-\
(2.14b)
Using (2.12), I{g, h, %) can be rewritten as I(g,A_,A + ) = S(g) + K\d2xTT{A_(d+g)g-1 + A_gA+g~l-A_A
+
},
+ (g-id_g)A
+
(2.15)
where 5(g) is the WZNW action (2.5) and A_=hld_k,
A+=(d+%-x)%.
(2.16)
In the action functional (2.15) A_, A+ are regarded as the light-cone components of some "gauge field" belonging to the adjoint representation of H, transforming according to (2.16), and its gauge invariance is obvious from the above construc tion. The variation of this action with respect to the non-propagating gauge fields A ± provides constraints which classically set the currents of H to zero. It has been demonstrated [14] that a careful quantization of (2.15) yields the GKO coset construction. At first sight it seems impossible to generalize (2.15) to be invariant under the more general transformations (2.13), since now the only obvious candidate for an invariant action is just S(hgh ~') which is non-local in the gauge fields. However, in the rather degenerate case when H and ft are the subgroups of G generated by the step operators associated to the positive and negative roots, and denoted by A^
119 84
BALOG ET AL.
and N, respectively, their Lie algebras are nilpotent, and hence one has the crucial property that S(h) = S(h~) = 0.
(2.17)
So S(hgh~1) — S{g) is local, therefore the gauge fields A_, A+ in Eq. (2.16) (where now heN and HeN) can be used in this case in the same way as for the case of a diagonal subgroup to set the corresponding N and N currents to zero. Since the constraints we want to implement set certain currents to constants rather than to zero, we consider the action I(g,A_,A
+)
= S(g) + K\d2xTr{A_(d+g)g-i + A_gA+g-l-A_n-A
+ (g-id-g)A +
v},
+
(2.18)
where n, v are special (constant) matrices, given by v = Z ^|a| 2 v«£ a ,
/;=£
\\*\2n°E_a.
A_, A+ are now independent gauge fields in the adjoint representation of the sub groups N and N so they are nilpotent matrices. The invariance of the action (2.18) under the gauge transformations, g-ag/T1,
/f.^d.a-'+aa.a"1,
A + ^/J/l + / r ' + (d + P)p~l, (2.19a)
where <x = x(x+,x-)eN
and
p = p(x + ,x~)eN,
(2.19b)
is now not completely obvious because of the non-gauge-invariant looking terms, TT(A + v + A _ /i). However, these terms change by a total derivative under gauge transformations because of the special form of A +, A_ and because the matrix v (resp. n) contains only step operators corresponding to simple positive (resp. negative) roots. For example, under the transformation (2.19) with
/?(*+,*-) = exPr X * , £ _ , ] we have Tr{v(8
+
/?)/?-'}= I
v'a + ^ ,
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TODA THEORY AND Ti^-ALGEBRA
85
and the term Tr A + v indeed changes only by a total derivative. The equations of motion following from (2.18) are (with
+ g-lA_g)-lA
+
,g-l8_g
+ g-,A_g^
+ gA+g-l)+\_A_,d+gg-,
+ d_A
+
=0
+ gA + g-i] + d + A_=0 l
l
TrlE_v(g- d_g + g- A_g-vn = 0 l
1
TT\_E
= 0.
(2.20a) (2.20b) (2.20c) (2.20d)
Now making use of gauge invariance, A+ and A_ can be set equal to zero simultaneously and then we recover from (2.20) the equations of motion of the WZNW model (2.7) together with the constraints (2.8). Note, however, that setting A +, A _ to zero is not a complete gauge fixing. Indeed, it is clear that the condition A± =0 is invariant under chiral gauge transformations <x = a.(x + ) and f} = f}{x_) which are in the intersection of the gauge group and the KM symmetry group of the theory. Since in the A± = 0 gauge (2.20) reduces to (2.7) and (2.8), it follows that the residual gauge transformations g^xxgp-i,
where a =
(2.21)
must leave (2.8) invariant. This can also be verified by using the standard transfor mation property of the currents J and J under KM transformations: J-+oJz-l + K(d + a)(x-1
and
J-* pJp'1 + K(d_p)p~l.
(2.22)
Note that these chiral gauge transformations (2.21) form the complete residual gauge group of the gauge A ± = 0. From now on we stay in this gauge. Here we point out how the residual gauge transformations (2.21) arise from the Hamiltonian point of view. For this, as well as in the rest of the paper, we take the space of solutions, given by (2.11), of the WZNW theory as our phase space. This is convenient here because of the left-right factorized form of the general solution. The translation to the equivalent equal time canonical formalism could be made by parametrizing the solutions by their initial data and expressing the initial data in terms of the canonical variables. To make this translation as easy as possible, in this paper we use equal time Poisson brackets on the space of solutions. After these remarks, let us observe that the KM Poisson brackets of those current components which are to be constrained according to (2.8) vanish on the submanifold of the phase space defined by (2.8) (constraintsurface), i.e., we are dealing with first class constraints. Now first class constraints always generate such canonical transformations which leave the constraint-surface invariant, and it is easy to see that in our case these are naturally identified with the residual gauge transformations. II.2. Gauge-Invariant Quantities Clearly the Toda fields,
121
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BALOG ET AL.
fields constitute a complete system of independent invariants with respect to these transformations on the "constraint-surface." In other words, Toda theory can be identified, at least locally, with the constrained WZNW model modulo residual gauge transformations. From now on we shall refer to the residual gauge transfor mations (2.21-2.22) simply as gauge transformations. It is important to note, that (2.9) is valid only in a neighbourhood of the identity of G. As a consequence of this non-global nature of the Gauss decomposition, our reduction can generate singular Toda solutions from perfectly regular WZNW solutions. This is the basis of one of the most important properties of the WZNW setting of Toda theory, namely, that the physically allowed singularities of the Toda solutions are precisely those which disappear by using the WZNW variables. We have shown this in Ref. [12] in the special case of 5L(2, R) by proving that the requirement that a Liouville solution be obtained from a regular solution of the WZNW theory is equivalent to demanding that the associated energy-momentum tensor (2.4) be regular. In Section V we shall show that this generalizes for a rank / algebra where besides the energy-momentum tensor there are / — 1 additional ""^-densities." In that case the Toda solutions with regular iST-densities can be represented by regular WZNW solutions, even if they appear singular in terms of the original local Toda variables
(
gu ■ ■ ■
: gdi--gdd)
Su\
(2-23)
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TODA THEORY AND T^-ALGEBRA
87
of the matrix (g„) are all gauge-invariant quantities. It is also easy to see that in the Gauss decomposable case the Toda fields ^" can be recovered as linear com binations of logarithms of the &,. For example, let us consider A, and take G — SL(I+1, R) in the defining representation. Using the standard convention, in which Hai has 1 in its //-slot, — 1 in its (/+1)(/ + l)-slot, and O's elsewhere, for a Gauss decomposable g one obtains the simple formula, %=e-*>-'n,
where
(2.24)
The local Toda field ^ indeed becomes singular where the Gauss-decomposition ceases to be valid, that is where one of the sub-determinants % changes sign. In general the globally well-defined sub-determinants (2.23) yield an overcomplete system of invariants, but in each concrete case one can single out / independent ones. For example, for the defining representations of the classical groups, the last / sub-determinants starting from gM suffice. They can be used as global variables for the Toda theory, after imposing the constraints (2.8). Since these sub-determinants are polynomial in the components of the basic WZNW field, g, they appear better suited for quantizing Toda theories than the original Toda fields themselves. For later use we note that beside the sub-determinants, which are fully gaugeinvariant polynomial quantities, there are other important quantities, which are linear in g, but invariant under left (or right) gauge transformations only. These are simply the elements of the last row (column) of g (and of gL and gK in (2.11), respectively). As the KM algebra plays a central role in WZNW theories, it is clear that gaugeinvariant quantities formed out of the KM current / (and J) will also be important in the Toda theories. To illustrate this, we recall how the conformal invariance of the Toda theory appears in the WZNW framework. Here we restrict ourselves to the left-moving sector. It can be shown that there is a unique Virasoro algebra in the semidirect product formed by the KM algebra and its associated Sugawara Virasoro algebra, weakly commuting with the constraints (2.8). Since the residual gauge transformations are generated by these constraints, the energy-momentum density L = L'-Tr{J'p),
where U = ±-Tr{J2),
p=\
£
Ha
(2.25)
giving rise to this Virasoro algebra, becomes gauge invariant on the constraint-sur face. It follows that L must generate the conformal symmetry of the constrained WZNW, i.e., of Toda theory. (One can verify that, after imposing (2.8) and using the local coordinates defined by the Gauss decomposition (2.9), L indeed reduces to the improved energy-momentum tensor 0 + + (2.4).) Note that p in (2.25) has the property [p, £,] = £„,
when
aeJ,
(2.26)
123 88
BALOG ET AL.
and that the classical centre of the (Toda) Virasoro algebra is c=-12fcTr(p 2 ),
(2.27)
where k is the level of the underlying KM algebra. We will see in Section III that, besides L, there are other gauge-invariant polyno mial quantities formed out of the constrained KM current and its derivatives. These objects will be referred to as gauge-invariant differential polynomials. A crucial property (which we elaborate on in Section III) of the gauge-invariant differential polynomials is that they form a closed algebra under the KM Poisson bracket operation. That is, the Poisson bracket of two gauge-invariant differential polynomials is again expressible in terms of gauge-invariant differential polynomials and ^-distributions. This means that if the quantities W' form a basis in the ring of gauge-invariant differential polynomials then we have \W\x\ W^y)}=ldP'i(W)6{k)(xl-yl),
(2.28)
where the PiJk are polynomials of the W's and their derivatives. These Poisson bracket relations generate a non-linear algebra, reminiscent of a universal envelop ing algebra. This non-linear algebra of the gauge-invariant differential polynomials always contains the Virasoro algebra, hence it is a polynomial extension of it. This way one associates an extended conformal algebra to every Kac-Moody algebra based on maximally non-compact simple real Lie algebras, for any level k. It turns out that this polynomial algebra is always finitely generated, by / = rank (3?) elements. In the literature these algebras are referred to as classical 1^-algebras. The quantum analogues of these Poisson bracket algebras play an important role in conformal field theory [4-9]. It has recently been realized [5-6] that quantum T^-algebras can be constructed by quantizing the so-called second Gelfand-Dickey Poisson bracket algebra of pseudo-differential operators, which has been studied earlier in the theory of integrable systems and is known to be isomorphic to the algebra of gauge-invariant differential polynomials [10] mentioned above. It is worth noting that the differential operators which provide the bridge between the original Gelfand-Dickey construction and the KM approach to T^-algebras [10] (also constructed by an independent reasoning in [8]) appear naturally in our framework. They are nothing but the operators defining the differential equations satisfied by those (last row) components of gL which are invariant under left gauge transformations. These differential equations can be obtained as a consequence of the obvious relation (Kd+-J)gL
= 0,
(2.29)
where (2.29) is taken in the defining representation of the corresponding maximally non-compact real Lie algebra & (see Section V for more details).
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TODA THEORY AND T^-ALGEBRA
89
In their review paper [10] Drinfeld and Sokolov studied the algebra of gaugeinvariant differential polynomials by making use of the constrained KM algebra. We shall see that exploiting the full (unconstrained) embedding KM algebra yields further insight into the structure of classical ^-algebras and leads to new results.
III. THE T^-ALGEBRA
In this section we undertake a detailed analysis of the ^-algebra introduced in Section II. We first make the definition of the 1^-algebra more explicit. The basic objects we are dealing with are gauge-invariant differential polynomials, W\ defined on the space P of the constrained KM currents (i.e., currents J satisfying (2.8)). The Poisson brackets of the Wl are obtained by first extending their domain to the whole KM phase space, K, computing the Poisson brackets on K and then restricting to P. The Poisson brackets on K depend on the chosen extension of the W"s (denoted by W), but their restrictions to P, which are again gauge invariant, do not. This follows by using the standard properties of the Poisson bracket from the first class nature of the constraints, and from the fact that the W"s are invariant under the gauge transformations generated by the constraints (and from the assumption that the W are real analytic in a neighbourhood of P). There is no reason to expect that a generic extension of the W's closes under the Poisson bracket on K, but there is a trivial extension, which has the property that the Poisson brackets of the Wl,s not only close but have the same formal structure on K as on P, i.e., {W\x), W(y)} = £ P i ( W ) S ^ i x 1
-yl),
k
where the P'fs are the "structure differential polynomials" (2.28) of the 1^-algebra. This particular extension is constructed as follows. First one expands the general KM current JeK in the Cartan-Weyl basis and notes that in P the upper trian gular and Cartan components vary freely, while the lower triangular components are completely fixed by (2.8). The trivial extension W of W is then defined to be the one which simply does not depend on the lower triangular current components. Every element W of the ^-algebra generates canonical transformations on the KM phase space by the formula J-+J + d*J,
S*J= -C" dxl
a(x){W(x),J},
where ty(x) is any extension and a(x) is an arbitrary test function. (Note that our equal-time Poisson brackets and spatial S's are in fact equivalent to light-cone brackets and £'s. Prime everywhere means, even on <5's, "twice spatial-derivative"
125
90
BALOG ET AL.
and this reduces to d+ on quantities, J(x), W'(x), and our test functions, which depend on x = (x°, xl) through x + only.) Since the transformation S&- is canonical (preserves the KM-structure and hence the co-adjoint orbits in K), it follows that it can be represented as a field dependent KM transformation, i.e., Sn,J = dRJ=[R,J~\
+ KR\
where R(J) is some (/-dependent) element of the KM algebra. The transformation da- transforms P into itself, and in fact induces a transformation 8%, on the space M of the gauge-orbits in P. The transformations 3$, corresponding to different extensions ft'of W^ differ on P only by (field dependent) gauge transformations, and thus the induced transformation 5^ does not depend on the extension (only on W). Of course, the reduced phase space M carries its own Poisson bracket structure which is inherited from the Poisson bracket structure of K, and is described by the standard Dirac bracket formula if one parametrizes M with some section of the gauge orbits in P (gauge choice). The induced ^-transformations 5%, are canonical transformations on M with respect to this induced (Dirac) Poisson bracket. In Subsection III. 1 we introduce some convenient gauges (called DS gauges), which will be used to show that the i^-algebra has a finite (/-dimensional) basis and to exhibit some particular bases W' (/= 1 •••/). The particular iF-generators W will be the gauge-invariant extensions (from the gauge section to P) of those current components (called DS currents) which survive the gauge fixing. Thus, in these gauges the ^-algebra appears as the Dirac bracket algebra of the DS currents. This is the basic fact on which most of our results are based. In Subsection III.2 we exhibit a conformal field basis of the ^"-algebra. In Subsection III.3, working in a DS gauge, we shall present an algorithm for finding the field dependent KM transformations which implement the induced iT-transformations <5£,. This algorithm is our main result since it enables us to calculate the action of the iST-algebra on any gauge-invariant quantity. In the last section we deal with some particular gauges which facilitate the study of some properties of the i^-algebra. III. 1. Drinfeld-Sokolov Gauges In this section we recall the construction of a class of particularly convenient gauges in which the properties of the ^-algebra become apparent. This class of gauges has been introduced first by Drinfeld and Sokolov [10], so we call them DS gauges. First we consider a special 5/(2, R) subalgebra of &, y, which will play an impor tant role in what follows. This subalgebra is spanned by the Cartan element p in (2.25) and nilpotent generators I± such that [ / + , / - ] = 2p,
[p,/±] = ±/±.
(3.1)
126 TODA THEORY AND iF-ALGEBRA
91
The step operators are explicitly given by ' - = I *.£-,.
I+=l^Eai,
(3.2a)
where X, = \KH'\OL,\\
«, = 2 £ ( * " ' ) , .
(3.2b)
Note that since Tr(/_ Eai) = Kfi' any element of P, i.e., any current fulfilling the con straints (2.8) (with nai = ii'), has the form /(*) = / _ + £ 0"(*)tf„+
I
CWiv
(3.3)
The adjoint representation of # decomposes into if multiplets. Since p is an element of the Cartan subalgebra of If the step operators are p-eigenstates, rj5,£J = />(<*>)£*.
(3.4a)
where A(
>f <*>= £"»/<*/•
j-i
(3.4b)
/-i
Let *» be the eigensubspace of p of eigenvalue A. If A # 0, then dim 95k = number of roots of height A.
(3.5)
It can be shown [18, 10] that, if for 1
«A = dim^-dim^ + 1
(ln* = A
(3.6)
is not zero, then A is an exponent of <§ with multiplicity nh. We recall the meaning of the exponents and their multiplicities [18]: The ring of group-invariant polynomial functions on # is generated by / homogeneous elements whose degrees are determined by the exponents, A. More precisely, there are exactly nh independent generators of order A + 1. In other words, these generators define a complete set of independent Casimir operators. We note that A = 1 and A = h^ are always exponents. The multiplicity of the exponents is always 1, except for Dv, where there are two independent Casimirs of order 21. Note that for (A > — 1) /_ maps 9h + , into \ injectively, that is dim/_(9 ! , + 1) = dim9!A+1,
(3.7)
127
92
BALOG ET AL.
where I_(% + 1)= [/_,%+\\ For any exponent, h, let Vh be a linear complement of I_(% + 1) in 9h (dim KA = /i/,) and let us also introduce the direct sum V=®
Vh
(dim^=/).
(3.8)
We choose a basis F( (i = 1,..., /) in V in such a way that [p,/-,]=/«,./•,
(3.9a)
l=/»is$/i 2 < ••• *SA, = /J*
(3.9b)
holds, where
is the list of the exponents with possible multiplicities included (see Appendix A). The basic fact we need is that any constrained current of the form (3.3) can be uniquely gauge transformed into a current J(x) of the form + KA'(X) A~l{x) = /_ + £ Wl{x)Flt
J(x) = A{x) J{x) A-\x)
(3.10)
I— 1
and that the W(x) and the parameters av(x) of the gauge transformation ,!(*) = expT £
a*(x)E9]
are differential polynomials in the components of J(x). The proof of this statement [10] is actually easy. Using the fact that the gauge transformations are generated by upper triangular matrices, the inspection of (3.10) reveals that it is uniquely soluble in purely algebraic steps for both W(x) and av(x) in terms of J(x). Denote now by Mv the space, whose "points" are currents of the form (3.10). The previous statement tells us that Mv defines a complete gauge fixing. Moreover, it also follows immediately that the components, W'(x), of the unique intersection point of My with the gauge orbit passing through JeP define gauge-invariant dif ferential polynomials on P, which freely generate the "^-algebra. In other words, the ff"s form a basis in the algebra of gauge-invariant differential polynomials. On the other hand, a completely general element of the KM algebra K can be expanded as / ( * ) = £ (/'(x)f,+
£
r9(*)E-.+
I
^(x)U_,Ev-\
(3.11)
and My is obtained by first constraining the £~v(x) by imposing (2.8) and then also fixing the residual gauge freedom by setting the fix) to zero. The current components, U'(x), which are not affected by this two step restriction and the corresponding gauge-invariant differential polynomials, W(x), are related by U'(x\Mv = W'(x)lMy.
(3.12)
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TODA THEORY AND ^"-ALGEBRA
93
However, it should be stressed that conceptually the U'(x) (linear functions on K) and the W'(x) (gauge-invariant differential polynomials on P) are very different objects and must be carefully distinguished. To make this distinction even clearer we introduce a separate name for the £/'. From now on we shall refer to them as DS currents. It will turn out that most of our results are a consequence of (3.12). For example, this relation immediately implies that each differential polynomial W(x) contains a leading term, i.e., a term without derivatives. In Subsection IV. 1 we shall prove that the leading terms of any i^-basis are obtained by restricting Casimirs from K to P. Now we discuss how the ^-algebra appears in a DS gauge. Clearly Mv inherits a Poisson bracket structure from the embedding KM algebra. This induced Poisson bracket structure is given by the familiar Dirac bracket formula [19]
{/, g}* = {/. g} ~ Z
f2" f d*1 dyl{f, i'(x)}
xDafi(x,y){t<>(y),g},
(3.13)
which is valid for two arbitrary phase space functions (/and g are functions on the KM phase space but only their restriction to Mv really matters). In this formula the £" are the current components to be constrained (cf. (3.11)), and D„p(x, y) is the inverse of C*{x,y)={Z'{x),t>{y)},
(3.14)
which satisfies £
P dylC*(x,y)D»(y,z)
= 8;5(xl-zl),
(3.15)
for arbitrary a, ye
= {W\x),WJ(y)}
on Mv,
(3.16)
as a consequence of (3.12). As discussed earlier the Poisson brackets of the W"s are in principle calculated by first extending them to K and then restricting the Poisson brackets calculated on K to P. Because of the gauge in variance of the W"s, this is equivalent to calculating the Dirac brackets of the DS currents. To summarize, we see that if the space of gauge orbits M is parametrized by the
129
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BALOG ET AL.
gauge section My, then its Poisson bracket structure is naturally described by means of the Dirac brackets of the DS currents, and that the i^-algebra can in fact be regarded as the Dirac bracket algebra of the DS currents. It will be demonstrated in the rest of this section that the properties of the T^-algebra are most effectively studied by making use of the DS gauges. The family of DS gauges is parametrized by the possible choices of the linear space V in (3.8). It is easy to see that Ui()x)~ L(x) on Mv and therefore Wl(x)~ L(x) on the constraint-surface P, for any DS gauge. III.2. Conformal if-Generators The energy-momentum density of the Toda theory, L in (2.25), generates the action of the conformal group on the KM phase space. This conformal action operates as J->J + SLJ f2*
SLJ= -
J
(3-17) dxla(x){L(x),J}
= (aJ)' + Ka"p + a'\_p,J],
o
where JeK and a(x) is any test function. The main point of this section is the observation that the ^-generators associated to a certain DS gauge (highest weight gauge) are primary fields with respect to this conformal action. To demonstrate this it will be useful to describe the conformal action in terms of field dependent KM transformations. Let R(J) be a KM algebra valued function defined on the KM phase space. Then it generates an infinitesimal (field dependent) KM transformation: J^J
+ 5„J,
dRJ=s[R,J~\ + KR'.
(3.18)
Now it is not difficult to verify that the conformal action SL is implemented by the field dependent KM transformation generated by the particular KM valued function R0(a,J) = -aJ + a'p,
(3.19a)
that is one has SLJ^S^J
for any J.
(3.19b)
The conformal action (3.17) transforms the set of constrained KM currents, P, into itself. Another crucial property of 5 L is that on P it commutes (modulo gauge transformations) with the action of the gauge transformations (2.22). Therefore (3.17) induces a conformal action on the gauge equivalence classes of the con strained currents, which amounts to an action on the set of gauge fixed currents,
130
TODA THEORY AND T^-ALGEBRA
95
My, representing those equivalence classes, for any choice of V. Our purpose below is to describe this induced conformal action J-+J + 6V
(JeMy)
(3.20)
operating on M v. In general J + SLJ$My, and therefore to determine 8fJ we must find the compensating (unique) gauge transformation, r = r(a, J), such that J + 5LJ + 8rJeMv,
for any JsMv,
(3.21a)
and then we have dtJ = SLJ + d,J = 5RJ
with R = R(a,J) = R0(a,J) + r(a,J).
(3.21b)
Before trying to determine r(a, J) let us recall that Sf is a canonical transforma tion on the reduced phase space My, generated by L by means of the Dirac bracket, &*LJ= - C" dx1 a(x){L(x), J}* = - C" dxla(x){U1(x),J}*
(3.21c)
on My. Here the second equality holds provided we normalize the DS current Ul according to Ul(x) = L(x)
on My,
(3.22a)
which corresponds to the normalization of the basis vector Fy, TTF1I_=K.
(3.22b)
With this normalization, as an obvious consequence of (3.16) and (3.21c), we have SfU1 =a(U1)' + 2a'Ul -KTr{p2)a'".
(3.23)
Next we want to determine the induced conformal transformation of the U' for / > 2. First, for an arbitrary gauge fixed current /(*) = / _ + £ V\x)Ft
(3.24)
i— i
one easily sees that 3 « / = I [a(t/')'+ (/>, + !)*'C/']F,. + Ka"p,
(3.25)
i- 1
where A, is the height of the Lie algebra element F, according to (3.9a). The last term is "out of gauge" so one indeed needs a "compensating" gauge transformation.
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In principle it is a purely algebraic problem to find r(a, J), but in practice it is quite hard to produce an explicit formula for the solution in an arbitrary DS gauge for an arbitrary Lie algebra. However, one can find a special gauge in which the form of r(a,J) is particularly simple and the DS currents are primary with respect to the induced conformal action (3.21). The construction is based on the sl(2, R) subalgebra if introduced in the previous section. Since the adjoint representation of ^ decomposes into if mul tiples, it is natural to consider the corresponding highest weight states, i.e., those Lie algebra elements which commute with / + . It is easy to see that the highest weight states in % span a natural complement of / _ ( ^ + ,). Choosing this par ticular complement in the construction presented in Subsection III.l we obtain a particular DS gauge, which we call the highest weight gauge. By using the fact that the basis vectors F, of V in (3.8) now satisfy the condition F,~/+,
[/+,F,]=0,
i=2,...,/,
(3.26a)
one easily proves that in the case of the highest weight gauge the compensating gauge transformation r(a, J) is given by the simple formula r(a,7)=-|icfl*/+.
(3.26b)
The corresponding conformal variation of the DS currents U' then turns out to be <5J£/' = a(t/')' + (/>, + l ) a ' ^ '
for
i = 2,...,/,
(3.27)
i.e., they are indeed primary with respect to the induced conformal action (3.21). Equivalently, one can say that the corresponding gauge-invariant differential poly nomials, W\ are primary with respect to the original conformal action (3.17) (restricted to P). The conformal weights of the W's (t/"s) are (/i, + 1), i.e., they are in one-to-one correspondence with the orders of the independent Casimirs of 'S. To summarize, we have proven that the generators W (i = 2,..., /) defined by the highest weight gauge, together with L=Wl, constitute a natural, conformal field basis of the ^-algebra. This is one of our main results. As far as we know, an algo rithm to find a conformal T^-basis has not been known before in the general case, although conformal ^-generators were explicitly exhibited for some particular low dimensional examples [6]. We now illustrate the idea of both the DS and the highest weight gauges on the example of B2 = o(3, 2). We use the convention [20] in which this Lie algebra con sists of (5 x 5) matrices which are antisymmetric under reflection with respect to the "second diagonal." The Cartan subalgebra is spanned by the diagonal matrices in B2- In this convention the Lie algebras of N and N are represented by upper and lower triangular matrices, respectively. In particular, the E% for a e A have non-zero entries only in the first slanted row above the diagonal. The Cartan element p in (2.25) is then easily found to be p = diag(2, 1,0, - 1 , - 2 ) .
(3.28a)
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TODA THEORY AND Ti^-ALGEBRA
97
By a convenient choice of the parameters T, in (3.2) we can choose the step operators of y as '0 4 0 0 0^ 0 0 6 0 0 /+ = | 0 0 0 - 6 0 |, 0 0 0 0-4 ^0 0 0 0 0 /
/O 0
0 0 0 0 /_ -= |0 01 1 0 0 loo - 1 0 \0 0 0 -1
io
0 0 0 |. 0 0
(3.28b)
(Note that the value of the parameters T, is irrelevant since they can be redefined by rescaling the simple step-operators.) The elements of % are now those matrices in B2 that have non-zero entries h steps above the diagonal only. Before describing the general DS gauge, we need to know the image /_(#2)- In fact, an easy calcula tion yields that /_(#j) is the set of matrices of the form 0 x 0 0 0 -x 0 0 0 0 0 0 ^ 0 0 0
0 0 x 0 0
0 0 0
(3.29)
—x
0
Since dim 9j = 2, there is now a one parameter family of (one dimensional) linear sub-spaces Vx of #, which are complementary to /_(# 2 ) m ^i- These are nothing but the "lines" spanned by the vectors of the form /0 0 Ft = Fl(p) = 0 0 \ 0
p 0 0 0 K-p 0 0 0 p-K 0 0 0 0 0 0
0 0 0 |, -p 0
(3.30)
for any real p. Note that F, has been normalized according to (3.22b). (For the B, algebras Tr means half of ordinary matrix trace in the defining representation.) The general current in the "DS gauge of parameter p" is written as
J(x) = /_ + {/'(x)Fl + U2(x)F2=\
0 1 0 0 0
pUl 0 u2 l 0 qU 0 1 0 -qU> -qU1 0 -1 0 0 0 -1
0
-u2 0 l
-Pu
0
,
(3.31)
133
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where q = K — p. We designate this set of gauge fixed currents as Mp. Observe that for Sp = 2K the matrix F, is proportional to / + , so that this value of p corresponds to the highest weight gauge. It is not hard to calculate the compensating gauge transformation r(a, J) in (3.21) which cancels the last term in (3.25). The reader can check that the result is
(
0 0 y2 y,
0 \
0 0 0 0 -yA 0 0 0 0 -y2 , 0 0 0 0 0 / 0 0 0 0 0 /
(3.32a)
which reduces to (3.26b) in the case of the highest weight gauge, as it should. The with m corresponding yconformal variation of U2 onilMp is given y3 = X[ica""-a"U A = by K(2K - 5/>), (3.32b) 2 = Xa , which reduces to (3.26b) in the case of the highest weight gauge, as it should. The corresponding conformal variation of U2 on Mp is given by b*LU2 = 4a'U2 + a(U2)' - A((K - p) a'"Ul + K(a"U1)' - K2a'""). (3.33) Since U' generates the induced conformal action on Mp through the Dirac bracket, from (3.33), taking (3.16) also into account, we can read off the Poisson bracket of Wl with W2 (restricted to P), which is now given as { W\x), W2(y)} = iW2(x)' S(xl - yl) + AW\x)
S'(xl - yl)
+ X((p- K)( Wl5)'" - K( WlS')" + K2b'"").
(3.34)
For A = 0, that is for the highest weight gauge, the corresponding ^-generator, W2, is a conformal primary field of weight 4. The generator W2 = W2p) associated to any other DS gauge (of parameter p) transforms in a complicated, inhomogeneous manner under the conformal action. III.3. KM Implementation of
if-Transformations
Here our purpose is to study the canonical transformations defined (as discussed at the beginning of the section) by the liT-algebra on the space of gauge orbits M. For this we consider the transformation 8%, induced on M by the following ^-transformation d# (acting originally on K), J^J+5it,J,
5*J= - £ f " dxl aMifr'lx), J},
(3.35)
where the W(x) are some arbitrary extensions from P to K of the "^-generators W(x) associated to some DS gauge with gauge section My, and the at{x) are
134 TODA THEORY AND Ti^-ALGEBRA
99
arbitrary test functions. We parametrize M by Mv and in this parametnzation the transformation 5$, is generated by means of the Dirac bracket according to J^J+5*WJ,
6U=-{Q(a,J),J}*,
(3.36a)
with Q(a, J) = £ C" dx1 a,(x) U\x),
(3.36b)
where the U'(x) are the corresponding DS currents. Similar to the special case of the induced conformal transformation <5* discussed in the preceeding section, the induced ^-transformation Sfy can be implemented by some field dependent KM transformation R(a, J). Of course, this KM implementation is in principle possible in any gauge, but here we show that in the DS gauges there exists a simple, effective algorithm for actually computing the KM valued function R(a, J) which implements <$&< '-e-> which satisfies 8%.J=SKJ
for any JeMy.
(3.37)
This is immediately translated into the action of the i^-algebra on itself, since in the DS gauge the W(x) reduce to the current components U'(x). An extra bonus of the KM implementation is that the KM algebra acts also on the G-valued WZNW field g(x+, x~) and from that action we get S*wg = S*g,
that is,
{Q(a,J),g}*=-R(a,J)g,
(3.38)
where "dot" means ordinary matrix product. From this equation we can read off the action of the ^-algebra on the Toda fields, which are the sub-determinants off. In order to make the presentation more concrete, we consider as examples the ^-algebras of the rank 2 Lie algebras A2, B2, and G2. The A2 example, which is the simplest non-trivial case, is included for the purpose of illustration. The B2 example has some non-trivial features which will motivate some developments in subsequent subsections. Finally, G2 (in Appendix B) illustrates the power of the method, since it enables us to compute the very non-trivial structure polynomials of this iT-algebra. We start by presenting a general characterization of the tangential (gauge pre serving) KM transformations for an arbitrary DS gauge. First we pick a point, J0eMy, and consider the tangential KM transformations at JQ. In other words, we want to describe all elements R{J0) of the KM algebra, which map J0eMy into My, i.e., we want to solve the condition that JO + SKJ0 = J0+\.^JO1
+ KR'
is in My.
(3.39)
135 100
BALOG ET AL.
To give the general solution of this condition, it turns out to be useful to supple ment the decompositions introduced in Subsection III. 1, $=r*©/-(9U,),
h>l
(3.40)
by similar ones for the subspaces <S_h of $ corresponding to the negative roots (cf. (3.4)). Indeed, the decomposition we consider is induced by (3.40) as ^_A=F_„
©[/_„,
for h>\,
(3.41)
where V_h is the transpose of Vh, V.h={v'\v6V„},
(3.42a)
and U_h is the annihilator of Vh in cS_h with respect to the scalar product Tr: U_„={ue^_h\Tvuv
= 0, VveV„}.
(3.42b)
(The transpose in (3.42a) can be defined abstractly by means of the Cartan-Weyl basis as E'v = E_v, H'v = Hv, but in convenient conventions [20] it is the ordinary matrix transpose.) Having introduced the necessary definitions we now return to the study of (3.39) and decompose the quantities entering this condition as R(x)= I
(u_„(x) + v_h(x)) + £ yh(x),
(3.43a)
where u_h, v_h, and yh are in the subspaces U_h, V_h, and %, respectively, and Jo(x) = I-+Z
v°{x),
5RJ0(x)= £ vh(x),
(3.43b)
where both v% and vh must be in Vh. By analysing Eq. (3.39), one finds that if / 0 and all the v_h(x) are given, then the remaining components of R are uniquely determined differential polynomials in terms of these. Furthermore, it follows that the components of SRJ0 are differential polynomials of J0 and v_h as well. In fact, the differential polynomials, R and SRJ0, are linear in v_h(x), but in general non linear in J0. The above result provides us with a complete characterization of the tangential KM transformations at the arbitrarily chosen gauge-fixed current J0. To actually prove this, one has to consider Eq. (3.39) height by height, starting from below, and use the following two properties of our Lie algebra decomposition: First, for A>0, /_ maps 9h into ^,_, in a one-to-one manner and this map is in fact onto for those h which are not exponents. Second, for 1 ^h^(h^, — 1), /_ maps U_h onto #_*_ i also in a one-to-one manner. By using these properties of /_, it is not difficult to verify that condition (3.39)
136 TODA THEORY AND TiT-ALGEBRA
101
is indeed uniquely soluble for R(J0) and 8RJ0 by purely algebraic means at every height, once / 0 and the v_h are given, and that the solution is linear in v_h. Let us choose a basis {F~'} in 0 A V_h dual to the basis {Ft} in 0 * Vh F-^-^—r
(3.44a)
Tr F,F't Since we assume that F, e Vhj, the duality property (which we shall need later on) Since we assume that F, e Vhj, the duality property (which we shall need later on) Tr F,F-J=>6J„ (3.44b) is automatic in almost all cases, i.e., for those basis vectors which correspond to exponents A, #/», of multiplicity 1, and we can also ensure this by a choice in the case of those two basis vectors which correspond to that exceptional exponent h = (21 — 1) of D2i whose multiplicity is 2. Using this basis, we can now write R in (3.43) as R = R(a,J0)= £ a,(*)F-'+ £ u_h(x)+ £ yh(x), i-1
»>l
(3.45)
»J0
where the a,(;c) are arbitrary functions and the u_h and yh are differential polyno mials linear in the a„ but not necessarily in J0. It is important to emphasize that, since J0 was arbitrary in the construction, this equation defines an element R(a, J) of the KM algebra for any J and a,. According to its construction, at any fixed JeMy this KM valued function R(a, J) provides a parametrization of the set of tangential KM transformations at J, by the / arbitrary real functions a,(x). Hence it is clear that by varying J and at the same time promoting the parameters a, to functional of J one can write in the form R(a(J), J) the most general field dependent, gauge-preserving KM transformation on Mv. So, in particular, the field dependent KM transformation implementing the induced ^-transformation <5£, (3.37) can also be written in this form with some functionals a,(J). The result we prove is that the above constructed KM valued function R(a, J) when considered for fixed (/-independent) a, and varying J is the one which implements the induced lif-transformation 5%, according to (3.37) and (3.38). This result means that we in effect replaced the task of finding the inverse of the matrix Cap(x, y) (3.14) which enters the standard formula (3.13) of the Dirac bracket, by the much easier (as will be clear from the examples) task of solving Eq. (3.39). To justify our claim we now show that (S*f)(Jo)={f,Q}*(Jo)
(3.46)
holds for an arbitrary real function f(J), where R = R(a, J) is given by the above construction, Q = Q(a, J) is the moment of the DS currents defined in (3.36b) and
137
102
BALOG ET AL.
J0eMy is arbitrary. To accomplish this we first recall that any element R0 of the KM algebra defines a particular (field independent) KM transformation S^ on the full KM phase space K, which is an (infinitesimal) canonical transformation generated by means of the KM Poisson bracket by the function Q0(J) = C" dxl Tr R0(x) J(x). J o
(3.47)
This means that the relation SRoF(J)={F,Q0}(J)
(3.48)
is satisfied on the full KM phase space K, for any real function F(J). The trick is that now we take R0 to be R(a, J0) in (3.45) for fixed J0 and a. In this case we know that at J0 the variation 5,^ respects the constraints defining Mv (R(a,J0) was constructed by requiring this) and therefore at J0 the constraint-contributions drop out from the Dirac-bracket of Q0 (3.47) with any quantity. This way we derive {F,QoWo)={F,Qo}*(Jo).
(3.49)
On the other hand, it is easy to see that for R0 = R(a, J0) the functions Q0(J) (3.47) and Q(a, J) (3.36b) differ on Mv only by a constant. This implies that they can be interchanged on Mv under Dirac-bracket. Taking this into account we immediately obtain (3.46) by combining (3.48) and (3.49) and by taking FiMy=f^Mv. This finishes the proof. We now illustrate on the simplest non-trivial example, A2 = sl(3, R), how to calculate the iT-algebra by our algorithm. The TT"(/42)-algebra is well known but it is worth reconsidering it in the present framework as an illustration. We use again the conventions of [20]. The Cartan element of the speical 5/(2, R) is represented by p = diag( 1 , 0 , - 1 ) .
(3.50a)
Choosing T, = T2 = 1 in (3.2) the remaining generators of Zf are given by
/+ =
/0 2 0\ 0 0 2 \0 0 0/
and
/_ =
/0 0 0\ 10 0 . \0 1 0/
(3.50b)
As in the B2 example, there is a one parameter family of DS gauges, and the gauge fixed current in the "DS gauge of parameter p" is written as J(x) = I_ + Ul(x)Fl + U2(x)F2,
(3.51)
138 TODA THEORY AND "W-ALGEBRA
103
where we can take (Op 0 Fl = Fi(p) = 0 0 K-p | \0 0 0
and
F2 = | 0 0 0 ) .
(3.52)
Here F, is normalized according to (3.22b). The highest weight gauge corresponds to 2p = K, but here we choose to work in the "Wronskian gauge" p = K, which is the gauge usually considered in the literature [5-9] (the origin of the name "Wronskian gauge" will become clear in Section V). Our aim is to find the explicit form of R(a, J) in (3.45) in the Wronskian gauge. In this case 0 001 F-' = (1/K00|
F-2 = | 0 0 0 | ,
and
(3.53)
0 0 0, and [/_, in (3.42b) now consists of matrices for which only a32 is non-zero, while U_2 is trivial. The explicit form of R in (3.45) reads then as yo
^2 N
yi
R = R(at, a2, J) = | a,/ie (y0 - y0)
Pi |,
(3.54)
where the at are arbitrary functions and the other entries are to be determined by the condition that the variation 5RJ must leave J "form invariant." In our case this means that SRJ must be of the form SRJ=[R,J]
'0 K5U1 6U2S + KR' = \ 0 0 01, ,0
0
(3.55)
0
since in the Wronskian gauge
(3.56)
As is follows from our general result, substituting (3.54) and (3.56) into (3.55) one obtains a system of equations which is uniquely soluble in purely algebraic steps for both the component functions u_t ■■ -y2 of R and for the corresponding variation
139
104
BALOG ET AL.
of J. One has to consider (3.55) height by height, starting from below, and easily obtains the following formulae for the components of R(a, J): a, «_,=
, , yi=aiUl+a2Uz-Ky'0,
Ka'2,
yo = a\+j\_a2Ul-Kan,
y{ = a2U2-Ky'0,
y0 = 2y0-a\,
y2 = — U2 + Ky\.
(3.57)
K
Before proceeding let us note that R (a2 = 0) implements the induced conformal action in the Wronskian gauge, and in fact one can rewrite the above formula as J?(fl„a2 = 0,y) = r i a 1 y +
fli^l-icriflr/++KflrF2l,
(3.58)
which is consistent with (3.21) and (3.19a) describing the conformal action in general. The variation of J under the KM transformation 8R is found to be SUl = la^U1)' + la\ Ul - 2Ka?~\ + l2a2{U2)' + 3o2 U2 - K2(a2 Ul)" + K3a'2"'J
(3.59)
and 5U2 = [a,(f/ 2 )' + 3a\ U2 + K2a'[Ux -K3a'{"~\ + a2\_K2(U2)" + ]K3U1(U1)'
- §K4(£/')"']
+ a i C f ^ t / 1 ) 2 + 2K2(U2)' - 2K\U1)"~\ -2K4a'2,(Uly-^KAa'2"Ul + lKsa2"".
(3.60)
Now by combining Eqs. (3.36) and (3.37), it follows that SU'(x)= S
F dylaj(y){U'ix\
U\y)}*
(3.61)
>-"T,2 •*<>
holds, so from (3.59) and (3.60) one can read off the Dirac brackets of the DS currents, yielding immediately the Poisson brackets of Wl and W2 according to (3.16). (See Subsection IV. 1.) Observe that the W2 generator associated to the Wronskian gauge is not a primary field with respect to Wx = L. However, it is easy to see that the combina tion fV2-j(W1)'
(3.62)
140
TODA THEORY AND "^-ALGEBRA
105
defines a primary field of weight 3. By investigating the transformation rules between the 1^-bases corresponding to different DS gauges one can prove that (3.62) is precisely the 1^-generator associated to the highest weight gauge. Note also that in this example the components of R{a, J) in (3.57) are only linear functions of the current components, and as a consequence 5RJ is at most quad ratic in J, which implies that the Poisson brackets of the "^-generators are also (at most) quadratic polynomials. This is not always the case, as can be seen, e.g., in the example of B2. We now illustrate the action of the T^-generators on the components of the matrix-valued field g(x+, x ~) on this example. All we have to do is to use the results (3.57) for (3.54) and substitute this R{a, J) into (3.38). Let us discuss the conformal transformations first. For this case, we find *i S i / - * ! S u + («i U'-Ka'i)g2i
+ (^
U2-K2a'A g3l
(3.63a)
&ig2i = — gu-Ka"gji
(3.63b)
8ig3i = — g2t-a\gu-
(3.63c)
K
To simplify (3.63) we can make use of the relation between the currents and the matrix-valued fields, (2.6). In this example this gives g2t = Ktyi,
gu = K2d2il/i,
(3.64)
where ^, = £ 3 , and d = d/dx + . Equation (2.6) also gives a differential equation satisfied by i^, (see Section V), which we will not explicitly use here. Using (3.64), (3.63c) simplifies to ^ , = 0,3*,-a',*,,
(3.65)
which tells us that i/f, is a primary field with conformal spin — 1 , whereas the remaining equations in (3.63) describe the conformal transformation properties of the secondary fields (3.64). We now turn to the genuine "^-transformation generated by U2. Using (3.64) again, we find d2il,i = a2^K282-^Ui^i-K2a'2dipi
+^ a ^
i
.
(3.66)
Equation (3.66) can be thought of as the transformation rule for a "TiT-primary" field under the W^transformation (for the A2 "^-algebra). For the algebra B2 we have derived the conformal action in Subsection III.2. Thus it only remains to determine the canonical transformation generated by W2
141 106
BALOG ET AL.
to know the complete set of transformations generated by the iST-algebra in this case, from which we can of course again (as for A2) read off the iST-relations them selves. By applying the algorithm presented above one finds after lengthy but straightforward calculations that
{U2(x), U2(y)}* = \ Z VF2i+l(x) + F2i+i(yn x5(2i+i\xx-yl)-KsP5(1\xl-yl)
(3.67)
on Mp, where &l = Q\(U2)" + Q[UlU2 + Q\(W)m + Q\U\U1)", + Ql((uiy)2 + Ql6(ul)\ F3 = QlU2 + Ql(Ul)" + Ql(U1)2, P = p2 + {p-q)2,
and
P5 = Q5Ul.
(3.68)
q = K-p.
Here Q5, Q{ are polynomials of the parameter p, given explicitly as Q\=-2K2P, 2
Q2 = SP2-\6KP
Q\ = 2K (3p-q),
4
Q\=-2K [2P
+ 4K2,
Q\ = 2K\P+2pq-]
+ 3pql,
Ql6 = 2(q + K) pq2
(3.69a)
Ql=-K(q + K)2P-2K2(2q + K)pq Q5 = 2K3t(q + K)P+Kpq] Q\ = 2tc2(q + K)P + 2K2(q + 2K) pq
(3.69b)
Q\ = K\_3q2 + Anq + 2K 2 ]P + 2>c2{q + 2K) pq. Observe that unlike for the A2-mode\, there is now also a cubic term, (t/ 1 ) 3 in J^1. The coefficient Q\ of this single cubic term vanishes in the special cases when p = 0, K or p = 2K. In other words, the B2 T^-algebra is given by quadratic relations in that li^-bases which are associated to the particular DS gauges of parameter p = 0, K or p = 2K. These "quadratic gauges" could be useful in the quantization of the liT-algebra, since normal ordering is more complicated when the order of the poly nomials involved gets larger. In contrast, the conformal properties are hidden in these gauges and are not as transparent as in the highest weight gauge (which belongs to 5/» = 2K in the B2 example). III.4. Other Convenient Gauges In the previous subsections we have discussed the DS type gauges and have shown that choosing a DS gauge naturally leads to a corresponding choice of basis for the niT-algebra, by relating the iT-generators to the non-vanishing current com ponents in that gauge. The highest weight gauge plays a particular role because the
142
TODA THEORY AND 1^-ALGEBRA
107
corresponding "^-generators are conformal primary fields (with the exception of the conformal generator W'). In the examples of A2 and B2 (C2) we have shown that it is possible to choose such DS gauges in which the generating relations of the ^-algebra are quadratic. These gauges are also important because the quadratic closure of the algebra simplifies the quantization. In this section we show that such gauges exist for the algebras A,, B,, and C,. We will see in the next section that they are not available for the rest of the Lie algebras. We start by considering A,, i.e., sl(l+ 1, R) and will use the defining representa tion. Here (and also for Bh C,, and D, later) we shall use the conventions [20] in which the positive and negative step-operators are upper and lower triangular matrices, respectively, and the elements of the Cartan subalgebra are diagonal matrices. For simplicity, now we choose all T, in (3.2) to be equal to 1, and then the matrix /_ reads /0 0 0 ••• 0 0\ ' 1 0 0 ••• 0 0 /_ =
0 1 0 ■•• 0 0
(3.70)
i 0 0 0 ••• 0 0 , \ 0 0 0 ••• 1 0 / The elements of 1fh are matrices with non-zero entries only in the slanted row h steps above the diagonal. The image / _ ( ^ + 1 ) (for A>0) consists of those matrices in % for which the sum of the matrix elements is zero. Fixing a DS gauge means choosing a single matrix in % for which the sum of the matrix elements is different from zero. The simplest choice yields the " Wronskian" gauge defined by fo u1 ■■■ u'\
vo
o ... o .
This gauge is a special example of the more general block gauges for which
/=/_+, = / _ + Q
(3.72)
and U is a pxq block (p + q = l+l) containing the / DS currents. The "Wronskian" gauge is the special case when p = 1 and q = /. In general these "block" gauges are not unique: we are still free to distribute the DS currents in a number of different ways along the intersections of the slanted rows with the block. Now we are going to show that the TfT-algebra closes quadratically in any of these "block" gauges. According to the results developed in the previous subsection,
143 108
BALOGETAL.
we can derive the #"-relations by determining thefielddependent KM transforma tion R(a, J) in (3.45) which implements the induced ^-transformations on Mv. To do this we first rewrite the defining Eq. (3.39) of R(a, J) in the form [/?,/_ ]
(3.73)
+ KR' = SJ+U,RI
Now, since we know that the unique solution of (3.73) for R = R(a,J) and SJ is linear in the infinitesimal parameters of the transformation, i.e., in the functions a, introduced in (3.45), and polynomial in the given gaugefixedcurrent /_ +j, we can expand both R and 8J in powers of the DS currents {j), R = R0 + Rl + R2+ ■■■ <5/=(<5/)o +
(3.74)
(<5./)1 + (<5./)2+ •••
and solve (3.73) perturbatively, lRm,I^
+ KR'm = (SJ)m +[y,/J m _ 1 ],
m = 0,l,2,....
(3.75)
Since in the "block" gauge both J and SJ are upper triangular in the block sense,
If we write out (3.73) in "block" components it is not difficult to see that the first order solution must be of the form
•-G3
(3.77)
where the p x p block A and the q x q block C are further restricted by Api = 0
for i^p-l
and
C,,=0
for / > 2
(3.78) i
and that the second order solution is of the form
-Q
with Z>„ = £>.. = 0,i=1.2,..., p; j = 1, 2,.... q.
(3.79)
For the "block" gauges the expansion stops here and, by the results of Subsec tion III.3, this implies that the algebra of the ^-generators corresponding to any DS gauge from the family of block gauges closes quadratically indeed. Note that the "Wronskian" gauge is special since D = 0 in this case and thus the KM transformation R = R(a, j) is only linear in the DS currents. The algebra is still quadratic, since (SJ)2 = [ / ? „ y ] .
(3.80)
144 TODA THEORY AND li^-ALGEBRA
109
For the other matrix algebras, B, and C,, one can define analogous "block" gauges by embedding them into appropriate ^4-type algebras. For Ct~sp(2l,R) we can use the 2/-dimensional defining representation. We write the C, matrices in terms of four Ixl square blocks. In this notation the symplectic metric is given by (3.81) - ( - . : > where the only nonvanishing entries of e are in the second diagonal (the diagonal from bottom-left to top-right), and these entries are all 1. The elements of the Lie algebra are represented by matrices of the form K =
\r
21'
where
B = B>€ =
C
(3.82)
and ~ means reflection with respect to the second diagonal. Positive (negative) step-operators are again upper (lower) triangular matrices and elements of the Cartan subalgebra are diagonal. By a convenient choice of the (irrelevant) parameters T,, /_ is now given by the 2/x2/ matrix: 0 00 1 00 0 10
(3.83)
0 0 0 0 0 0
It has / 1 entries and (/— 1) ( — l)'s. The "block" gauges, in which the algebra closes quadratically are characterized by 7=/
- + (oo)
(184)
where U= U and it has non-vanishing components along every second slanted row, corresponding to the exponents of this algebra. Finally, for Bt~so(l + 1, /) we take the (2/+ 1 )-dimensional vector representa tion. In a 3 x 3 block matrix notation corresponding to the partition / + 1 + / the Lorentzian metric is (3.85)
145 110
BALOG ET AL.
and the elements of the Lie-algebra are of the form K=\ Y'
0
-X'\,
where S=-B,
C=-C.
(3.86)
The matrix /_ is again similar to (3.83) but it is now a (2/+ 1) x (2/+ 1) matrix and has / upper entries 1 and / lower entries (-1). The "block" gauges for this algebra are defined by (3.87)
where 5= —b and the DS currents are again distributed along every second slanted row. An other convenient gauge is what we will call the diagonal gauge. It is defined by J(x) = F_+t
6>,(x)//,,
(3.88)
i = i
(Here we choose the {//,} to form an orthonormal basis for the Cartan subalgebra.) Note that this is a new type of gauge fixing, not a member of the family of the DS gauges, but it will turn out to be very useful in applications and it is most useful in the quantum theory. Before we start discussing the gauge choice (3.88) in detail, we mention two difficulties connected with it. We will illustrate these difficulties on the simplest example, 5/(2, R). In this case the gauged fixed current in the diagonal gauge is parametrized by a single real field 8(x), 6 0
•/<.,* = ( . i
J -e
(3.89)
and it is easy to see that the transformation from the "Wronskian" gauge
to the diagonal gauge amounts to solving the Riccati equation 92-K0'
= U.
(3.91)
Now, if we require all fields to be periodic and integrate the Riccati equation over
146 TODA THEORY AND TiT-ALGEBRA
111
the period, the derivative term drops out and we see that (3.91) has no solution unless f " U(x)dxx>0.
(3.92)
In other words, the diagonal gauge can only be reached from that part of the phase space where (3.92) is satisfied. A related difficulty is that when the Riccati equation can be solved, its solution is not unique, it in fact has two independent solutions. (For an arbitrary Lie algebra, the number of independent solutions of the analogous equations is equal to the order of the Weyl-group.) However, note that when available the diagonal gauge is locally well defined (the ambiguities mentioned above correspond to finite gauge transformations) and therefore the corresponding Dirac brackets are also well defined. Since the i^-algebra is determined by polynomial relations, its structure can be analysed by restricting the considerations to that part of the phase space where the diagonal gauge is available and we will see that this is often convenient. Expanding the general KM current, /, in the Cartan-Weyl basis as J= £
r * £ - , + I 0tH,+
£
C'£„
(3-93)
the set of constraints defining the diagonal gauge can naturally be divided into two parts, * = ([)•
(3.94)
The diagonal gauge is defined by constraining the £~9 by imposing the original constraints (2.8) and, in addition, setting the f to 0. Since on the corresponding constraint surface K,?}=0
and
{C,C}=0,
(3.95)
the C operator, whose inverse enters the formula for the Dirac bracket can schematically be written as C = { X , * } * ( _ ° B o),
(3-96)
where B= {
(3.97)
147
112
BALOG ET AL.
The important property of the diagonal fields O^x) that makes the diagonal gauge extremely simple is that they (weakly) commute with the additional constraints (*": {0,(x),C}*O.
(3.98)
Because of (3.98), the Dirac bracket of two diagonal currents is the same as their original KM Poisson bracket: {0M.6j(y)}**{0i(x),ejiy)} = K5v8'(x1-yl).
(3.99)
In other words, the diagonal components of the current are a set of free fields. Therefore in the diagonal gauge the 1^-generators are given as differential poly nomials in free fields and these differential polynomials are simply obtained by restricting the full (gauge-invariant) differential polynomials to the "diagonal currents" of the form (3.88). This free-field representation of the iF-generators is called the Miura-transformation and has been used to quantize the theory [5].
IV. CASIMIR ALGEBRA
IV. 1. Leading Terms and Casimir Algebra We have already seen that any DS gauge defines a basis of the li^-algebra, and that there is a one-to-one correspondence between the conformal weights of the ^-generators associated to the highest weight gauge (or the scale dimensions of the "^-generators associated to any DS gauge) and the orders of the independent Casimirs of the underlying simple Lie algebra. In this section we shall elaborate on this connection further, by showing that the leading terms of the ^-generators (i.e., terms without any derivatives) are always Casimirs (restricted to P). Then we demonstrate that the Casimirs themselves form a polynomial algebra under the Poisson bracket, which is a truncated version of the full 1^-algebra. This Casimir algebra, in its quantum version, has been studied in [15]. We shall denote the leading terms of the "^-generators, W>, by W{. Since these leading terms contain no derivatives, they are invariant under rigid gauge transfor mations, that is Wi(JA) = W]0(J)
for AeN, where JA = AJA ~'
for any constrained current (JeP). On the other hand, an arbitrary Casimir C' is a group-invariant polynomial, that is, for any KM current J and an arbitrary Be G one has Cj(JB) = CJ\J),
where
JB =
BJBl.
148
TODA THEORY AND 1^-ALGEBRA
113
First we want to show that the leading terms of the "^"-generators are restricted Casimirs, or in other words that Wi(J) = CJ(J),
JeP
(4.1)
for some CJ. To do this we shall use the theorem of Chevalley from the theory of invariant polynomials [18], which we now recall. This theorem states that there is a one-toone correspondence between the Casimirs and the Weyl-invariant polynomials on the Cartan subalgebra, and that the correspondence is simply given by restriction. That is, first, if CJ(J) is an arbitrary group invariant polynomial (Casimir) on #, then its restriction to the Cartan subalgebra, CJ\H), is a Weyl-invariant polyno mial. (We shall denote the Cartan subalgebra by Jf and the restriction of any func tion to 3HC by an overbar.) Conversely, from any given Weyl-invariant polynomial on Jf, a corresponding full group invariant can be reconstructed in a unique way. For later use we also recall that the uniqueness of the reconstruction is proven by "diagonalization." First note that for any Lie algebra element J in the compact form of # there exists a group element g e G that "diagonalizes" /: J* = gJg-l = H(J)eX. (The use of the compact form is justified here since the problem is purely algebraic.) Using the group invariance of the Casimir CJ we see that C\J) = CJ(JS) = CJ(H(J)) = Cj{H(J)) so CJ determines the full Casimir CJ uniquely indeed. By using Chevalley's theorem, (4.1) will follow if we can prove that the restriction of Wl(J) to currents / in the diagonal gauge (cf. (3.88)) is a Weyl-invariant polyno mial of the Cartan components of J. To do this we only have to show that for any "diagonal" constrained current J it its possible to find such rigid gauge transforma tions AeN, whose action on the Cartan components 0, of J coincide with the action of the Weyl-group on the 0,. To show this, let us choose a simple root
with a = wE:,k
(4.2a)
on a constrained current JeP, J^J^
= eaJe-a = J+\_a,J'\ + \\_a, [ a , 7 ] ] + •••,
(4.2b)
where a> is an arbitrary real parameter. Parametrizing the constrained current JeP
J = I + I 0,H« + I £,£„,+£ tvEv, f'= 1
1 = 1
(p
149
114
BALOGETAL.
where
a* l j
t'
where the precise form of the coefficients V w and
which implies that the transformation (4.2) applied to the "diagonal" current / i= I
takes it into another current which is also in the diagonal gauge. Moreover, with this choice of co the action of the gauge transformation A = e" (4.2a) on the the Cartan components 0, of this particular diagonal current is
I «* I
j
which is precisely the same as the effect of the Weyl-reflection corresponding to the simple root a* on the Cartan components 0,. This implies that every Weyl-transformation of the Cartan components of the diagonal currents can indeed be implemen ted by rigid gauge transformations. (Since the Weyl-group is not a subgroup of N, the particular rigid gauge transformation A which "implements" a given Weyltransformation on the components 0, of a "diagonal" current ydjag must depend on the particular current on which it acts, and is really field-dependent according to the above construction.) Since the leading term W0 is invariant under rigid gauge transformations, it follows that its restriction WJ0 to the diagonal gauge is a Weylinvariant polynomial of the current components 0,. Chevalley's theorem then tells us that W'0 is the restriction of a uniquely determined Casimir CJ to the diagonal currents (note that /_ has no contribution in CJ(JdMg) because of the neutrality of
150 TODA THEORY AND ^-ALGEBRA
115
the group invariant CJ). To finish the proof of (4.1) one has to show that the leading term WJ0 itself is the restriction of the same Casimir CJ to P. This last step follows from the fact that WJ0 and the restriction of C' to P are the same (namely W{) when restricted to "diagonal" currents, since an TV-invariant on P can uniquely be reconstructed from its Weyl-invariant restriction to the space of diagonal currents. (The uniqueness of this reconstruction can be shown by an argument similar to the one that was used in the case of the Chevalley theorem.) It is not hard to see that the Casimirs {CJ} corresponding to the leading terms of a i^-basis {WJ} form a basis in the ring of group-invariant polynomials. (It is enough to prove this for a i^-basis constructed by means of some DS gauge, but in this case these / Casimirs are independent even if restricted to the gauge section Mv, where they simply coincide with the / DS currents {Uj}.) So we can associate a Casimir basis to any i
y= 1,2,...,/.
(4.3)
Then we can define ^-generators corresponding to these Casimirs by the formula 7+1 where J=AJA1
+
KA'A-1
is the representative of the gauge orbit of the constrained current JeP in some particular DS gauge. (Remember that both JeMy and the gauge transformation A are uniquely determined by JeP. ) It follows that we have WJ
X
--TT JJ+X =^—Tt{J+KA-lA')J+i ^ - T r / ' + 1 + •••, (4.4) J+l J+l 7+1 J that is the leading terms of the W are indeed the Casimirs CJ. It is also easy to see that the {W'\ associated by this method to a set of independent Casimirs form a basis of "^-algebra. (The ^-generators associated to a given Casimir by means of different DS gauges differ in their derivative, non-leading terms.) In the SL(3, R) example, choosing the "Wronskian" gauge / 0 Wl W1 /= 1 0 0 \0 1 0
151 116
BALOGETAL.
we have Wl = \lxJ2
W2 = \TxP.
and
(4.5)
By using the results of Subsection III.3 on the A2 example we can derive the relations {W'(*), W\y)} = K( W1)' (X) b + 2KW\X)
b' - 2K3 b'"
{Wl(x), W2(y)} = 2K(W2)' (X) b + 3KW2{X) 6' -K2[W1{X)5]" 2
2
+ K*5"" 1
1
K(W2)"-IK2(W1)'"](X)S
{W (x), W (y)} = K\_1(W )' W + + Kll(Wi)2 + -2K\W1)'
(X)
2K(W2y-2K2(W1)"l(x)6' 5"-^W^x)
S'" + %KS 5'""
where <5 = d(xl — yl) and x° = y°. On the other hand, it is not difficult to verify that the corresponding Casimirs Cl = {lxJ2
and
C2 = i T r / 3
(4.7)
satisfy the following algebra under Poisson bracket, {Cl(x),Ci(y)}
= K(Cl)'(x)d + 2KCl(x)5'
{C'ix), C2(y)} = 2K{C2)' (X) b + 3KC2(X) b' 2
2
(4.8) 2
{C (x), C (y)} = K [ § ( C ' ) ' C'](x) S + K [ | ( C ' ) ] ( X ) S'y which is nothing but the leading term (in K) of the full liT-algebra for 51.(3, R). In fact we will show that in general, if the TT-generators W' and WJ satisfy {Wi{x),Wi(y)}=Y,fA{W)(x)b«\xx-yi\ A
A
where the "structure functions" f (W) are differential polynomials in {Wj}, then the corresponding Casimirs C and C satisfy the simplified (truncated) algebra {C'(x), CJ(y)}=rt(C)(x)b,+f°l(C)(x)b,
(4.9a)
where fl0 and f\ are the leading terms of / ' and f° in the number of derivatives, which are 0 and 1, respectively. To show this, let us first note that from the form of the KM Poisson brackets and group-invariance of the Casimirs it already follows that the commutator (4.9a) must be of the form {C'W, 0{y)} = gi(J)(x) b' + *?(/, J')(x) b
(4.9b)
152 TODA THEORY AND HiT-ALGEBRA
117
with some group-invariant functions gl and g°. (g° is polynomial in J, but is linear in J'.) Now we have to demonstrate that go(J) = fo(C(J))
and
g?(J, •/')=/?(C(/)).
(4.10)
We will make use of the diagonal gauge and the Chevalley theorem once more. In the diagonal gauge the leading terms of W' and C' coincide and therefore we have gtiH) = fl0(€(H))
and
fi(H,H')=f°(C(H)).
(4.11)
Now applying the Chevalley theorem to g^, the first equation in (4.10) follows from the first one in (4.11). Before one is able to apply the theorem also to g°, one first has to generalize it for the case of operators containing one derivative. This is possible and the proof is basically the same as for operators without any derivatives. Let us define the group invariant <5°(J, / ' ) by g°l(J,J')=f°i(C(J)) + S0l(J,J'). From the second equation in (4.11) we see that d°x(H, H') vanishes, but then the full (5°(7, J) must vanish too since «?(/, J') = <5?(//(/), (J')') = *?(#(/), (//')*) = <5°(//(/), (/T)«) = 0, where the second step follows from the neutrality of the group-invariant 5°. This way we have shown that the set of Casimirs closes to form a polynomial algebra under the Poisson bracket and that this algebra is a truncated version of the corresponding "^-algebra. Since the completely local Casimirs {C} are more elementary objects than the {W) which contain derivatives as well, one can ask wether the closure of the Casimir algebra can be shown without any reference to the more complicated ^-algebra. In other words, one has to show that (4.9a) holds with some functions fl0 and f°. It is trivial that gl in (4.9b) depends on J only through the Casimirs, since this merely expresses the fact that the {C} form a basis for the completely local group-invariants. To show that g° is also a function of the Casimirs we go to the diagonal gauge again. In this gauge the restriction of g°t must be of the form * ? ( # , # ' ) = I Afi\,
(4.12)
;= 1
where the {0,} are coordinates with respect to some basis in the Cartan subalgebra and the coefficients {^4,} can be considered as an /-component vector in the Cartan subalgebra and can be expanded as
153 118
BALOG ET AL.
simply because the / vectors {dCJ/dd,} are linearly independent. (This is the analytic expression of the fact that the / invariants {C7} are functionally independent.) Substituting (4.13) into (4.12) we find
and we see that the coefficients Bj must be Weyl-invariants: g°(ff, H') = I j - 1 —
Bt(C{H))[C\H)-y.
Now using the generalized Chevalley theorem for g° again we have
*?< y ' J>) =I irrr Bj(c(j))ia(j)J. After this digression we return to the question of the quadratic closure of the T^-algebra. We have shown in the previous section that the nT-algebras for A,, Bh and C, are quadratic in a suitably chosen basis. As an application of the relation between the ^-algebras and the algebras of the corresponding Casimirs we now prove that no such basis exists for £>, and the exceptional algebras. In fact we show this for the Casimir algebras, from which the analogous result for the li^-algebras immediately follows. Let CH be the highest order Casimir, of order H (see Appendix A), and let us consider the Poisson bracket of CH with itself, {C„{x), CH{y)} = r2H_2(C)(x)3' + kr2H_2(C)(x)3.
(4.14)
(Here the two structure functions are not independent of each other due to the antisymmetry of the Poisson bracket.) The structure function r2H_2(C) is a Casimir of order (2H — 2) and by inspecting the list of group-invariants for the case of the exceptional groups it is easy to see that it can never be expressed as a quadratic function of the basic Casimirs {CJ} for these groups. The situation for D, is more complicated. Here we can show that the set of Casimirs {C\ C2,..., C'} defined by
d e t ( l - ^ 7 ) = l - t Hncn>
( 415 )
n= 1
where the determinant is taken in the 2/-dimensional vector representation of Dh forms a quadratic algebra under Poisson bracket. (This is actually the same algebra as is formed by the corresponding Casimirs of the B, and C, groups.) However, as
154
TODA THEORY AND iS^-ALGEBRA
119
is well known, (4.15) is not a correct choice of basic Casimirs for D,, the latter is given by the set {C\ C 2 ,..., C ' " 1 ; Ca = sfc'}. By introducing the "spinorial" invariant C„, we destroy the quadratic property of the algebra. We find that r4/_6, the structure function in the commutator of two highest Casimirs C'~l is given by (see Appendix C) r4/_6=-12K(CJ2C'-3-4icC/-1C/-2
(4.16)
which is indeed cubic for / > 3. IV.2. Explicit Casimir Algebras In Subsection IV. 1 we have shown that the Casimir operators, C , form a closed, polynomial algebra under Poisson bracket, which is a truncated version of the ^-algebra. These Casimir algebras are interesting in their own right and they are also useful for studying the related "^-algebras. In this subsection we exhibit their structure in some detail. First, it is obvious that the Casimirs are conformal primary fields with respect to the Sugawara energy-momentum tensor. Next we want to determine the non-trivial Poisson bracket relations describing this algebra. What we are actually going to calculate is the Poisson bracket of the generating polynomials / £ fin+iC"(x)
A(n,x) = dct(l-iiJ(x))=l-
(4.17a)
«= i
and B(n, x) = det(l - J~n Ax)) = 1 - 1
fi"C(x)
(4.17b)
n- 1
for the / independent Casimirs C 1 ,..., C of the A, and B, (C,) algebras, respectively. One first observes that the overcomplete set of group-invariant polynomials « = 2,3,...
Q"(X) = -TTJ"(X),
(4.18)
n which are related to the / independent Casimirs C" via Id"
/
°°
for
A,,
»-0■ o
c
Id"
"=-^
exp
f
2
°°
e2
\
(- ,?/ v
for p-0
B„ C„
155
120
BALOG ET AL.
satisfy the Poisson brackets (see Appendix C)
{Qn(x),Q'"(y)}=KUp-2)Q''-2-^Q"-,Qm-l](x)S' + KUm-l)(Q"-2y~^Q"-l(Q"'-ly^{x)d,
(4.19)
where S stands for <5(JC' - yl) as before, p = n + m, q = (n - 1 )(m - 1), and N is the dimension of the defining representation. Note in particular that for the B and C algebras both n and m must be even integers (since for odd n the Q" vanish identi cally) and, as a consequence, the quadratic terms on the right hand side of (4.19) are automatically absent. However, formula (4.19) is only the first step in finding the explicit Casimir algebras. For example, in the case of A2 one obtains
{Q\x), Q\y)} = K ( V - \ Q2Q2) &' + 1 ( 4 ( 2 4 - \ Q2Q2)' 8 and only after expressing Q* in terms of the independent Casimirs Q2 and (?3 via 2Q* = (Q2)2 does one find the result (4.8) (note that Q2 = C1 and Q3 = C2 there). More generally, if one computes the Poisson brackets of the highest Casimirs for an algebra of rank /, one has to use the characteristic polynomial 0(1/2) times to express the right hand side of (4.19) in terms of the independent Casimirs. Clearly this method becomes soon cumbersome and another algorithm is needed. As a first step to calculate the Poisson bracket of the generating polynomial (with itself) we expand its logarithm, oo
log det( 1 - nJ(x)) = - X /i"C"(x)
(4.20)
n= 2
and use (4.19) to calculate the Poisson bracket of logdet(l — nJ). This then allows for the computation of the Poisson brackets of the determinant. After some algebra one finds that this Poisson bracket can be reexpressed in terms of the determinant and its derivatives. For the details of the derivation we refer the reader to Appendix C. The final results are A, algebras: {A(fi, x), A(v, y)} = K / iV (^~-v (dv - ^ ) - j-J-j- d„ 8^ A(ii, x) A(v, x) S' + K/iV ((0, - d„) - ~ - - ^ d„ 3 y ) A(n, x) BxA(v, x) 8 + - ^ - L2 j (A(n, x) dxA{v, x) - A(v, x) dxA(n, x)) S, (H-v)
(4.21)
156
TOD A THEORY AND "W- ALGEBRA
121
Bh C, algebras: {B{\i, x), B(v, y)}=4Knv
( v 5 v - ^ ) B(n, x) B(v, x)8' fi — V
+
4K//V(V5V
- iidj
(B(/i, x) dxB(v, x)) 3 fl—V
+ 2K/iv /
+ V
(fi-v)2
.2 (B(n, x) dxB(v, x)- B(v, x) dxB(ti, x)) d. (4.22)
The algebra of the Casimirs can now be computed by inserting the expansions (4.17) into both sides of (4.21), resp. (4.22), and comparing coefficients in the resulting polynomials in n and v. One sees, in particular, that with respect to the Casimirs defined by the determinant the algebras close always quadratically. For example, for the highest Casimirs of A,, 1^2 one obtains {C'(jc),C'O0} = Ka / (x)*' + ! f l ; ( x ) $ (4.23) 2
1 2
a/ = - 2 C ' C ' - 0 ( / - 3 ) + - — r ( C ' - ) and for the highest Casimirs of B, and Ct with / > 2 one finds {C\x\
C'(y)} =
-4KC'C'-
'
8'-2K(C'C'-1)'
S.
(4.24)
The corresponding results for the lower Casimirs are presented in Appendix C.
V. DIFFERENTIAL AND PSEUDO-DIFFERENTIAL OPERATORS AND TODA FIELDS
The aim of this last section is to demonstrate that the differential and pseudo-dif ferential operators studied in [10], and taken as a starting point for the quantiza tion of ^-algebra in [ 5 ] , arise naturally in our framework. These operators appear in the differential equations satisfied by the gauge-invariant components of the WZNW field. Let us recall that the solution of the field equations for the group-valued field g is g(x\x-)
= gL(x
+
)gR(x-)
(5.1)
with gLgL1=J
and
gilg'*
=Z
(5.2)
157 122
BALOGETAL.
where the currents J and J are subject to the constraints (2.8). (In this section prime means 2K d/dxl.) We will consider the simplest case, SL(n, R) first, and concentrate on the left-moving part of the theory. (We omit the subscript L.) In order to reconstruct the group-valued field g(x+) from the current J(x+) (satisfying the constraints (2.8)), one has to solve the set of linear differential equations g' = Jg-
(5.3)
Obviously this is a separate set of equations for each column-vector of the matrix g, which are of the form
=( / - + » . •
(5.4)
Solving (5.4) is the simplest in the "Wronskian" gauge, (3.71). In this gauge one can easily express all components of g in terms of the bottom components, gnj, denoted by i^,, gin-1)1
=
^
(5.5)
leading to a single nth-order differential equation satisfied by tpn
,/,(«>= £ uty—J
".
(5.6)
J-I
The group-valued field g can now be built from the n independent solutions of (5.6),
^1
"h
•"
4>n
where the set of solutions {i/^,} must satisfy the Wronskian constraint (hence the name of the gauge): detg=l in order that the matrix g be an element of the group SL(n, R).
(5.8)
158 TODA THEORY AND iF-ALGEBRA
123
We note that if the DS currents {UJ} are regular functions then so are the solu tions {\pt} of the generalized Schrodinger equation (5.6). By combining gL given by (5.7) with the similarly constructed right-moving solution g R , the resulting WZNW field g(x+,x~) is also regular, as are the globally defined Toda fields, being subdeterminants of the latter (according to (2.23)). Furthermore, if the niT-generators corresponding to a given (say, the "Wronskian") DS gauge are given by regular functions for a Toda solution, then by this procedure one can always construct a regular WZNW representative of that Toda solution, whether or not the solution appears to be regular in terms of the traditional local Toda variables,
\^-x
vxJ
= W-X')WX)-W-X){>I>X')
(5-9)
(rr r-x' r-x\ e-*-«2=®„_2=deti r-xK r-x' r-x\ =(r-x")(r-x'M-x)+--where *-X«5>rZ„
r-X = Y.r-Xi,
(5-10)
and so on. In fact Eq. (5.9) was the starting point of the analysis of Toda theory in [8]. Without going into details we note that the above results can easily be generalized for the B, and C, series. So far we have studied (5.4) in a definite DS gauge. Let us now try to solve it for g without gauge-fixing the current J. It is easy to see that starting from the bottom row, it is always possible to eliminate all higher components of g successively, even without any gauge fixing. This elimination leads to a differential equation of the form n— 1
^ V , . = 5 V , - Z Wi\_J(x + )-\d"-i-^i
= Q.
(5.11)
y-i
Here d = K d/dx + and the coefficient functions { W'} are automatically obtained as some differential polynomials in the current components. Moreover, they are gauge invariant, since the original equation (5.3) was gauge-covariant and the bottom components gni — ^t are gauge-invariant (with respect to left-moving upper
159 124
BALOGETAL.
triangular gauge transformations). This implies that the WJ'& in (5.11) are nothing but the ^-generators associated to the "Wronskian" gauge, since they reduce to the DS currents {UJ} in this gauge. To summarize, if the 1^-densities associated to a DS gauge (here the "Wronskian" gauge) are known, then one can reconstruct the corresponding WZNW solution by solving (5.2) for g = gLgR in that DS gauge. In the reconstruction procedure one obtains a higher order differential equation (here (5.6)) satisfied by the gauge-invariant (bottom row) components of gL (and an analogous equation for the last column of gK). The same equation can also be derived from (5.4) by elimination without any gauge fixing. Since the resulting dif ferential equation is gauge-invariant, one can read off the explicit formula of the ^"-generators corresponding to the given DS gauge by comparing the coefficients in the differential equations obtained with and without gauge-fixing. By a similar argument, one can also establish the transformation rules relating the iC-bases corresponding to different DS gauges. The elimination is also simple in the diagonal gauge. In this gauge
(
0, 0 ... 0 (5.12)
0 0 2 ••• 0 and the differential operator takes the form 0 0 .. d„ and the differential operator takes the form By rearranging this product as a sum corresponding to (5.11), one can read off the ^)=(d-e (5.13) i)(d-e2)---(d-dn). By rearranging this product as a sum corresponding to (5.11), one can read off the expression of the iF-generators in this gauge. Note that the diagonal fields (5.12) are not independent, because 0, + 02 + ■■■ + 0„ = 0. This is the original form of the Miura-transformation [21] and the operator (5.13) is the starting point for the Lukyanov-Fateev free-field construction of quantized T^-algebra [ 5 ] . The derivation of the gauge-invariant higher order differential operators and the reconstruction of the matrix-valued field g from the constrained currents (or from iT-generators) proceeds analogously for the Lie algebras B„ and C„. The resulting gauge-invariant differential operators are of order (2« + 1) and (2/i), respectively, according to the dimensions of the defining representations. Due to the restrictions (3.86) and (3.82), the differential operators 3i(nB) and 2>l,C) are (formally) antiselfadjoint and selfadjoint, respectively. Without going into detail, we give these operators in the factorized form corresponding to the diagonal gauge: ®inB) = (d-0l)(d-02)...(d-e„)d(d + d„)--(d + 82)(d + dl) (5.14a)
&nC) = (d-el)(d-e2)...(d-9„\d
Here the 0/s are independent free fields.
+ en).-(d + 92)(d + ei).
(5.i4b)
160
TODA THEORY AND 1^-ALGEBRA
125
The case of the algebras D„ is more complicated. As an example, let us consider D3 first. We use the six dimensional vector representation and go to the diagonal gauge, where (with a convenient choice of the T,)
J=I_+J=\
0, i 0 n 0 0 0
0 0 0 0 0 e2 0 0 0 0 0 0 0 1 03 \ t n n 0 -03 0 n0 1 0 0 - 1 - 1 -02 0 - 1 -0. 0 0
•
(5.15)
If we write out (5.4) in components we have (suppressing the index i) g5=-(d
+ 9l)g6
(5.16a)
£3 + £4 =~(d + 92)g5
(5.16b)
g2 = (d + 03)g4
(5.16c)
g2 = (d-d3)g,
(5.16d)
gi = (8-e2)g2
(5.16c)
O = (3-0,)g,.
(5.16f)
From (5.16) we see that the elimination is blocked here after the second step, since the combination g3 — g4 never occurs on the left hand side. On the other hand, its derivative can be expressed, combining (5.16c) and (5.16d), as d(g3-g*)
= e3(g3 + g4).
(5.17)
One can go on with the elimination by integrating (5.17) (formally) using the "antiderivation" symbol d~l: (gi-g4)
= d-%(g3
+ g4).
(5.18)
One then finds &3D) = (d-dl)(d-82)(d-03d-lO3)(d+
6^(8 + 6^
= (d- 0,)(3 - 62)(d - 03) d~\d + 93)(d + e2)(d + 0,).
(5.19)
Similarly, by performing the elimination in the (2«)-dimensional vector representa tion, one can associate a pseudo-differential operator to any £>„ algebra:
®inD) = (d-ei)(d-e2)---(d-en)d-\d
+ en)..-(d + e2)(d + el).
(5.20)
This not only shows that it is impossible to obtain a differential operator for D„ in the vector representation, but from the example of D3 ~ A3 we also see that the type
161 126
BALOG ET AL.
of pseudo-differential operator depends on the representation in which (5.4) is taken. (For Z)3 there is an ordinary differential operator corresponding to the four dimensional representation, but this is the spinor of Z)3.) For the case of A„, B„, and C„ what makes the elimination simple is that the matrix /_ (see (3.70) and (3.83)) has non-zero entries immediately below the diagonal and only there. Since /_ is the negative step-operator of the special 5/(2, R) subalgebra Sf introduced in Subsection III.l, this fact means that the defining representations of these algebras are still irreducible with respect to this 5/(2, R) subalgebra. For D„, the vector representation is reducible with respect to £f with branching 2n = (2/i- 1)+ 1. This is why one has a pseudo-differential, rather than a differen tial, operator after eliminating the higher components from the system of first order differential equations (5.4). (The spinor representations of D„ are even worse from this point of view, except for n = 3.) Turning to the exceptional algebras, we find that the seven dimensional represen tation of G2 is irreducible with respect to if and therefore the elimination for G2 will result in a 7th order differential operator (see Appendix B). The corresponding branching rule for FA is [22] 26 = 17 + 9, so in this case we have a pseudo-differen tial operator, containing one integration. Finally, for E6, E7, and Es the branching rules are [22] E6: 27 = 17 + 9 + 1 £ 7 : 56 = 28 + 18+10
(5.21)
£ 8 : 248 = 59 + 47 + 39 + 35 + 27 + 23 + 15 + 3 and therefore in these cases the elimination leads to pseudo-differential operators, containing 2, 2, and 7 integrations, respectively. VI. CONCLUSIONS
In this paper we have shown that extended conformal algebras, "^"-algebras arise naturally in the constrained WZNW formulation of Toda field theories. Our main results are the following: We have given an ambidextrous generalization of the usual gauged WZNW models to derive Toda theories. Using the embedding WZNW phase space, we have shown how to implement the action of the ^-algebra generators as certain field dependent Kac-Moody transformations. This led us to a powerful algorithm to calculate the iT-algebra relations. Using this algorithm we calculated the so far unknown Poisson bracket algebra of ifr(G2) explicitly. We exhibited a particular basis where all the ^-generators are conformal primary fields. We have also shown that for the A, B, C series there is always a basis in which the iS^-algebra closes quadratically, and that is not true for the rest
162
TODA THEORY AND "W-ALGEBRA
127
of the simple Lie algebras. Finally we have proved that the leading terms of the ^-generators (i.e., terms without derivatives) are restricted Casimir operators. We exhibited the Casimir algebra relations in detail for the A, B, and C series and have given a general proof of closure of their Poisson bracket algebra for any simple Lie algebra. As found in [15] the quantum version of the Casimir algebra does not close in general (it has been shown to close for SU{3) only when the level is equal to one) hence it is natural to ask whether an extension of the nT-generators to the full KacMoody phase space (in the sense discussed in the introduction of Section III) exists, with the full, unrestricted Casimirs as leading terms. If one could find such an extension it would make it possible to associate a representation of the T^-algebra in terms of unrestricted Kac-Moody generators to any Kac-Moody algebra. As such an extension would also be a deformation of the Casimir algebra, it could possibly survive quantization. This problem is certainly very interesting as it would also clarify the origin of li^-algebras, without making reference to any particular model. A detailed investigation of such deformations of the Casimir algebras is out side the scope of this paper. After some preliminary investigation of the problem we found that at least for A2 one cannot extend the ^-algebra to the whole phase space of the (chiral) Kac-Moody currents, at least with the assumption of the W"s being differential polynomials with unrestricted Casimirs as leading terms. However, by giving up the polynomial nature of the W"s we have found such an extension of the generators of the 1^-algebra for A2. In fact this result can be generalized for an arbitrary A„ algebra. This problem is under investigation.
APPENDIX A: CONVENTIONS
Here we give our conventions and present some formulae which are used in the paper. Space-Time and Poisson Brackets. »foo= —1n = l.
x±={(x°±xl),
d±=80±dl.
(A.1)
We use equal time Poisson brackets and spatial ^-distributions. At fixed x° all quantities are supposed to be periodic with period 2n. Prime means "twice spatial derivative" everywhere, even on Dirac <5's. Note that this is equal to d+ on quantities depending on x through x+ only. Conformal Primary Fields. The left-moving conformal transformations are generated by the conserved moments Qa=f
dxia(x)L(x)
(A.2)
of the Virasoro density L(x) = & + +(x), for any periodic test function a(x) for
163
128
BALOGETAL.
which d_a(x) = 0. A conformal primary field W of left conformal weight A trans forms as (SL
+ Jny)d
+ a(y).
(A.3)
If d _ V = 0 then this is equivalent to {L(x),ny)}ixo.yo
= A.nx)S'(xl-yl)
+ (A-l).(d+nx))d(xl-yl).
(A.4)
Lie Algebras. Let #c be a complex simple Lie algebra, <& the set of roots with respect to some Cartan subalgebra, and A a set of simple roots. There is a Cartan element Hv associated to every
where Tr is the usual matrix trace multiplied by an appropriate normalization con stant, which ensures that |a long | 2 = 2. For example, for the defining representations of the orthogonal Lie algebras B, and D, this normalization constant is £, and it is 1 for the defining representations of At and Ct. For any positive root a e # + we choose step operators £ ± J s o that we have
for a, /? e
for a, fie A.
(A.7)
In our Cartan-Weyl basis H„ (aeA), E±v (
Exponents 1,2,...,/ 1,3 2/-1 1,3 2/-1 1,3, . . . , 2 / - 3 ; / - l 1,5 1,5,7,11 1,4,5,7,8,11 1,5,7,9,11,13,17 1,7,11,13,17,19,23,29
164
129
TODA THEORY AND T^-ALGEBRA
Kac-Moody Algebras. We denote the space of ^-valued left-moving currents by K. The KM Poisson brackets of the components of J(x) = J"{x) Ta are given as {Ja(x),Jb(y)}{xo.)P=ffnx)d(xl-yl)
+ Kga''S'(xl-y1)>
(A.8)
where the/f" are the structure constants, the KM level k is -4mc, and Lie algebra indices are raised and lowered by using the metric gab = TT(Ta-Tb).
(A.9)
APPENDIX B: G2 1^-ALGEBRA
In this appendix, as a non-trivial example, we compute the Poisson-bracket relations of the ^-algebra corresponding to G2 explicitly, using the tangential Kac-Moody method introduced in Subsection III.3. We will work in the seven dimensional representation of G2 and choose the following matrix representation for the two simple step operators:
r
0 0 0 / o0 0 E = 0 0 0 0 0 0 0 0 \
0 0 10 00 0 0 00 0 0 00
/0 1 0 0 /O 0 0 0 0 0 0 yjl
0 0 0 0 0 0 0
£,=
0 0 \ 0 \0
0 0 0 0
0 0 0 0
0 0 0 0
0 0 0
0 0 0
-v^O 0 0 0
0 0 0
0 0 0 0 0 -1 0
(B.l)
Choosing T, = x2 = 1, the generators of the special sl(2, R) subalgebra are / _ = £ { , + ££,
/ + = 10£. + 6£„
P = hU+J-\
(B.2)
where p is a diagonal matrix with diagonal elements 3, 2, 1,0, — 1, —2, - 3 , respec tively. Since there is no "quadratic" gauge for G2, the only distinguished gauge is the "highest weight" DS gauge and we will work in this gauge. We denote the two DS fields by L and Z, which are the coefficients of j / + and the step operator for the highest root, respectively:
J=
0 0 0
0 3L 0 1 0 5L 0 1 0
0 0
o o 72
0
-3V2L
-v/2 0 0
0 -1 0
0 0 0 0 0 0
0 0 0
z
0
0 -z 0 0 0 0 -5L 0 0 -3L -1 0
(B.3)
165 130
BALOG ET AL.
On the other hand, a general Lie algebra element can be parametrized as
Ax H2 / " a2 b R = \ Jlc -Jib c 0 -e \ o / ">
B A2 H3 Jla, 0 -c -d
D JlC -JIB C 0 JlAx 0 -JIAX -Jlax -H3 Jib -a2 -b -Jlc
E 0 -C
JIB
0 V -E \ -D \
-JIC
-A2 -H2
-B -A,
-a,
-Hx
,
(B.4)
1
/
where H{ = H2 + H3. Now we have to solve the equation bJ=[R,J] + KR'
(B.5)
for the variations bL, bZ parametrizing bJ in terms of the independent parameters of R, which are the parameter e and a certain linear combination of a, and a2, which correspond to the variations generated by Z and L, respectively. Let us discuss the conformal variation first. Using (3.22b), we see that the properly normalized conformal generator is 14 A= — L.
(B.6)
K
The conformal variations, generated by the conformal "charge"
r
QX=C* dxl<x(x)A(x)
(B.7)
Jo
(through Dirac-brackets) are obtained by solving (B.5) with e= 0
and
at=a2 = -<x.
(B.8)
K
We find
K £?,}* = <M = **' + 2*'A -14Ka'" {Z,Qa}* = b3Z = <xZ' + 6a'Z.
(B.9)
From (B.9) we see that the central charge of the Virasoro algebra is c=-168* and that the field Z is a conformal primary field with conformal spin 6.
(B.10)
166
TODA THEORY AND if- ALGEBRA
131
The only non-trivial ^-transformation is generated by Qe=CX dxie(x)Z(x).
(B.ll)
The corresponding variations can be found by solving (B.5) now with e#0
and
9a, + 5a2 = 0.
(B.12)
After a lengthy computation we find {Z,Qe}* = SeZ ^ { - K ' V ' + X
/c2'+I[(eQ2,+ 1)(2' + 1> + e<2'+1>G2,.+ l ] } ,
(B.13)
where S, = -4576L 2 Z-
7 5 6 K 2 L " Z - 1850K 2 L'Z'
+ 230400L5 + 407392K 2 L 3 L" +
-
860K 2 LZ"
1514056K 2 L 2 (L') 2
-
74K 4 Z"" 1956K*L2L""
+ 11
+ 1010254K 4 LL'L'" + 797637K 4 L(L") 2 + 1648812K 4 (L') 2 L" + 21 196K 6 LL ( 6 )
+ 138201 K6L'L'"" + 36443 IK6L"L"" + 2 3 = 1240LZ+
120K2Z"-
- 3487(k4Z.L"" -
168608L4-
157520K 4 L'L'"
Q5 = -52Z + 30580L3 +
\1226K2LL"
*^K6{L'")2
+
2073K8Z.,8>,
184316>C 2 L 2 L"-457655K: 2 L(L') 2
+
124443K 4 (L") 2 ^K2(L')2
+
-
3410K 6 L <6) ,
1683K4Z,"",
C7=-2046L2-396K:2L"(
Q9 = 55L. Note that it is a non-trivial check on our result for SrZ that it can be written in the form (B.13), which follows from the antisymmetry of the {Z,Z}* Dirac-bracket hidden in {Z, Qe}*. Finally, by introducing an orthonormal basis {H{, H2} in the Cartan subalgebra defined by \_E«,E'J=J2H1,
lEll,E'^=—^=Hl+^=H2 V
2
(B.14) V
6
and going to the diagonal gauge where J=I_+6tHl
+ 82H2
(B.15)
167
132
BALOGETAL.
we can easily write down the 7th-order differential operator discussed in Section V:
•^*-;^ ri ->-;75 , 'X ri -> + 75' 1 ) ■^"^••-ji'fa+ji^ji'fa+ji''}
(B 16,
•
APPENDIX C: EXPLICIT CASIMIR CALCULATIONS
In this appendix we present the arguments leading to the Poisson brackets (4.21) and (4.22). We then use these results to derive explicit formulae for the Poisson brackets of the Casimirs C as defined in (4.17). First we need the Poisson brackets of the group invariant objects, Q", defined in (4.18). We observe that due to the invariance of the trace under cyclic permutations / f l A c y T r ( y r ) = Tr(y"[7) r 4 ]) = Tr(./" + I r 6 - / " r t / ) = 0,
(C.l)
the Poisson brackets of the Qms are given by {Qn(x),Qm(y)}
= Kgai,Tr(Jn-lT°)(Tr{Jm-1Tb)(x)d'
+ Tr(Jm-lT")'
(x)S),
(C.2)
where the argument of 5 and S' is (xl — y1). Now by using the identity Jn = Ti(JnTa)Ta + ^-Q", N
(C.3)
valid for the A, B, and C series, we find gab TT(J"Ta) Tx(JmT") = (n + m) Q" + " - ^ Q"Qm N gab
TT(J»T°)
T r ( / T * ) ' = m(QT + m )' - ^
Q"(Qm)'.
Together with (C.2) this leads to the Poisson brackets (4.19). Now we are ready to calculate the Poisson brackets for the generating function for the A, algebras
/ t o *) = log det(l-M*))-
(C4)
168
TODA THEORY AND iST-ALGEBRA
133
By using the power expansion (4.20) and the Poisson brackets (4.19) one arrives at {f(^x),f(v,y)}
=K
linvm((p-2)Q"-2-j-Q'-lQ"-1\(x)5'
£
finvm((m-l)(Q"-2)'-lQ'-\Qm-ly)(x)5,
+K X
(C.5) where p = m + n and q = (n — 1 )(m — 1). The sums quadratic in the Q" are readily expressed in terms of / and its derivatives and we turn to the more difficult task of expressing the two remaining sums linear in the Q" in terms of/ In the first sum X
(p-2)ii'vmQ>-2=
£ (p-2)(nv)"/2Q"-2
n,m>2
p^A
£
(/i/v)*"-^ 2
m + n—p
we insert the identity
Z
a„n-m
'a
'^-a3"' a-l/a
and then the remaining sum over p can be written in terms of/ and its derivatives as YJ(p-2)fi»vmQ>-2
= ^(dJ-dJ).
(C.6)
In the second non-trivial sum in (C.5) X(m-l) / x"v m (0 p - 2 )' = I ( / i v ) ' / 2 ( e ' ' - 2 ) '
^
( W -l)( / Vv) ( "-" 0 / 2
m + n —p
we insert <x'-2-a2-' X(m-l)a" — = (a-l/a)2
T7-xr-(p-2)-
'
a-l/a
and the remaining sum over p can again be written in term of/and its derivatives as 2 2
2 2
I(m-l)^"(C2'-7 =^5,ay/+^3j^ax(/(v)-/(/i)).
(C.7)
169
134
BALOGETAL.
Finally, using (C.6) and (C.7) in (C.5) yields
K/1V
1-NV>
1°*]-°»J \H-v 2
-dxdj
+ K/Z
V
~h>
llfdxd.
+
1 (H-v)2
W(v)-/(/i)] (C8)
. / ) & ■
From this equation one immediately obtains the Poisson brackets (4.21) of the generating polynomial A(ix, x) = exp(/(/i, x)) for the A -series. The Poisson brackets for the generating polynomial of the B and C series can be calculated in a similar manner. The only difference is that instead of formulae (C.6) and (C.7) one needs the identities £
2(/>-l)/iV"02(p-1, = - e L ( v d v g - ^ p S )
(C9)
and £
(2m-\)^v"Q«>-»
= ^v-^-2(g(V)-g(»))
+ -^vd,g
(C.10)
to derive the Poisson brackets (4.22). (Here g(n, x) = log fl(/i, x).) The Poisson brackets of the generating polynomials contain all information about the Casimir algebra. For example, by using the expansion (4.17a) in (4.21) one obtains for A, {Ck(x),Ck(y)}
= Kak(x)S'(xl-yl)
+ ^Ka'k(x)S(xl-yl),
k = 1,2,...,/,
(C.ll)
where 2k9(l+l-2k)C2k-'+e(k-2)-k(l--^-\(Ck-1)2
ak = k-i
-20(k-3)
£
0 ( / - I - * X I + 1)C*+ 'C*-'-2,
i=0
and by using the expansion (4.17b) in (4.22) one obtains for the B, and C, algebras {C(x),
C(y)} » xbk(x) 6'(xl -yl)
+ | Kb'k(x) S(xl - / ) ,
* = 1, 2,..., /, (C.12)
170
TODA THEORY AND -f-ALGEBRA
135
where bk = 4(2* - 1) 9(1 + 1 - 2k)C2* " ' - 48{k - 2) k-2
x j ] 0(/-i-*)(2i+l)C*
+
'C*-'-'.
In particular, for the highest Casimirs the Poisson brackets simplify to (4.23) and (4.24). ACKNOWLEDGMENT
A. Wipf thanks the Max-Planck-Institut (Werner Heisenberg Institut) where he spent most of the time during which this work was done.
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172 Reprinted with permission Cram Nuclear Physics B Vol. 357, pp. 632-654,1991 © 1991 FJsevier Science Publishers B. V. (North-Holland)
COVARIANTLY COUPLED CHIRAL ALGEBRAS F.A. BAIS, T. TJIN and P. van DRIEL Insliluul voor Theoretische Fysica, Valckenierstraat 65, 1018 XE Amsterdam, The Netherlands Received 10 December 1990
New extended conformal algebras are constructed by conformal reductions of %\N WZWN models. These are associated with the inequrvalent sl2 embeddings into s\N. Among other things, the conformal weights of the generators and the occurrence of Kac-Moody and W„ subalgebras are determined by the branching rules of the adjoint representation for the particular embedding. For some representative classes the algebras are constructed explicitly. In general they are coupled chiral algebras suggesting that they correspond to the symmetries of certain interacting conformal field theories. Moreover we find that a (minimal) covariant coupling is present which is related to a generalized Gelfand-Dickii structure. Some aspects of the quantization are addressed, in particular the c-values are determined. We introduce a new hybrid realization of KM algebras which interpolates between a realization of currents and of free fields, in which the constraints can be imposed in a very natural way.
1. Introduction Bosonic extensions of the conformal algebra have been the object of extensive study recently. Initially these were the Kac-Moody and the so called W„ algebras, which occurred as the symmetries of the WZNW and Toda models respectively [1]. Furthermore a relation between these models could be established. On the one hand the W„ algebras could be obtained from A(^'_, KM algebras, exploiting the coset construction [2]. On the other hand the Toda field theories have been identified as the Drinfeld-Sokolov hamiltonian reduction of the slw WZWN models [3,4]. In this work it became clear that the Toda theories have a stressenergy tensor which consists of the original quadratic Sugawara tensor improved by a linear term corresponding to the Cartan element of the principal sl2 subalgebra of sl/y. This program bears a striking resemblance to the seemingly unrelated problem of constructing spherically symmetric solutions to the self-dual SU(A0 Yang-Mills equations [5]. Indeed, by imposing spherical symmetry with respect to an improved angular momentum operator Limpr = L + T, where L generates the ordinary rota tions and T denotes the principal su(2) subalgebra of su(N), the self-dual equa tions reduce to the Toda equations. In fact there is no reason to restrict oneself to the principal su(2) subalgebra. Other inequivalent su(2) embeddings T were
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considered in ref. [6] where it was shown that they give rise to generalized Toda theories which are integrable and conformally invariant. Bearing this in mind it is to be expected that other sl^ reductions of the WZNW model based on non-prin cipal si2 embeddings should exist. It is this problem that we analyse in this paper. The outline of this paper is as follows. In sect. 2 we fix notation and review some properties of Kac-Moody (KM) algebras and the Virasoro algebras associated with them. Sect. 3 starts with a review of some basic facts concerning the Dirac constraint formalism [7]. Then, using arguments similar to the ones given by Balog et al. [4], it is shown that it is possible to associate an extended conformal algebra to every sl2 embedding into slN. Finally a method to explicitly construct the algebras is given. In sect. 4 we determine whether the reduced algebras have KM and/or W„ subalgebras. A crucial role in this is played by the branching rules of the adjoint representation of slN with respect to the embedded sl2 subalgebra and its centralizer. In sect. 5 representative examples are considered in detail. In particular all possible sl3 and sl4 reductions are calculated. Also some hierarchies of reductions are constructed, the simplest of which leads to a bosonic version of the N = 2 superconformal algebra coupled to an sIN KM algebra. In the final section we discuss the quantization of the newly obtained extended algebras. In particular we calculate the central charges. Also a hybrid realization of the KM algebra interpolating between a current algebra and a free field realization is introduced.
2. Generalities Consider the Kac-Moody algebra L belonging to the simple Lie algebra L. This algebra is realized as the central extension of the algebra of loops in L. The Lie bracket structure of this KM algebra reads [(/,a),(g,/3)]=([/,g]L,^/o2wd0(/(0),g'(^)))'
(1)
where /, g : S1 -> L, a, fi e R, and (.,.) is the Killing form on L. On L there exists a unique invariant symmetric bilinear form (/,g)L=^/2Wd<M/(4>),g(4>)).
(2)
2.TT ■'0
The dual L* of L is defined with respect to this pairing. On L* there is a canonical Poisson bracket, called the Kostant-Kirillov-Lie bracket. It reads
{F,G}U)-U,[dn,,dGU]) L ,
(3)
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where F and G are C°° functions on L*. dF\^ and dG\^ are elements of L** = L determined by F(f + 8f) = F(jr) + (dF\J,,Sjr). Let's choose a basis {TX-\ in the underlying finite dimensional Lie algebra L. An arbitrary element / e L * can then be written as fix) = Ja(x)(f)Ta where J"(x):L* -* U is the function that adjoins to f its components (x,a). The Poisson brackets between the functions {Ja(x))xeS\ (a = 1 , . . . , n) can be calculated using eq. (3) and read {ja{x),Jb{y)}=Kg°»8\x-y)+rbcJc{y)8{x-y),
(4)
where gab is the inverse of the matrix Tr(TaTb) = gab and fab are the structure constants of L in the basis {Ta)"_v Furthermore K is some real number. The algebra (4) is well known as the current algebra of the classical WZNW model, {/"(*)} being the currents. Using eq. (4) the infinitesimal action on L* induced by the charge Q" = (dxa(x)J"(x) can easily be calculated (8J»(y))Tb=
-{Q\Jh(y)Th)
= \a(y)g°dTdj\y)Tb\
+ Ka'(y)g°
which means that the transformations generated by the charges Q" have a KM implementation. In fact, the right hand side of eq. (5) is the infinitesimal version of the coadjoint action of the KM group on L* ad*Jr = gfg-l+Kdgg-i,
(6)
where g e KM group and / e L * . As is well known, the quantity L^{x)
= {\/2K)Tx{f1{x))
(7)
is a Virasoro density, i.e. {L^(x),Ls»\y))
= 2l}»\y)8'{x-y)-{Ls»*)'{y)8{x-y).
(8)
The currents {/"(*)} are primary fields of conformal weight 1 with respect to LSu* i.e. {L^{x),J"{y)}=J\y)8\x-y)-{Ja)\y)8{x-y).
(9)
However, the quantities L impr (jt) =LSu*(x) where fix)
=Ja(x)Ta,
+Tr(XdJ-(x)),
(10)
a e U and A e L, are all Virasoros. Due to the linear
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improvement term, the Poisson bracket of L'mr"(x) with itself picks up a central term. The bracket reads explicitly [L'mp'(x),L"npr{y)}=
-K2Tr(\2)8m
+ 2L'mpr(y)8' -dL,mp'(y)8.
(11)
In this paper we are interested in extended conformal algebras that are reductions of the KM current algebra. By an extended conformal algebra we mean an extension of the Virasoro algebra by a finite set of primary fields with positive (half-)integer conformal weight, whose Poisson algebra closes on polynomials of the fields and their derivatives. This means that these algebras in general need not be Lie algebras.
3. Constraints and reduction In this section it will be shown that it is possible to obtain extended conformal algebras by putting constraints on the KM current algebra. We will restrict ourselves to linear constraints where some of the currents are fixed by a relation of the form J°(x)= / A
(12)
where fi" is some constant. Putting constraints on a system may generate gauge invariances. (In constrained classical dynamical systems these gauge invariances are responsible for undeterministic flows on the phase space, as was shown by Dirac.) This gauge invariance is generated by the first-class constraints, which are those constraints that commute weakly with all other constraints (i.e. that commute after imposing the constraints). The true phase space is the set of gauge equivalence classes of elements on the constrained surface. In practice we "construct" this space by fixing the gauge, which amounts to choosing in every gauge orbit an element to represent the entire orbit. Needless to say that the set of these elements must itself be a smooth manifold. In certain favourable circumstances (to which we will come in a moment) the Poisson bracket on L* induces a Poisson bracket on the set of gauge-fixed elements. This induced bracket is the so called Dirac bracket. How does this come about? Well, consider an arbitrary Poisson manifold (M,{-, •}) and a set of independent functions {<£,} on M. The set Z = {p e MI$,(/?) = 0; / = 1,..., r) is then a submanifold of M. Now, if det({^,^}(/7));.,1#0
(13)
for all p G Z then {•, •} induces a Poisson bracket on Z. The explicit form of this
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bracket is {f, gf = {f,g)-{f,<{>;)*%,
g},
(14)
where A'' is the inverse on Z of the matrix 4> ={*/,*;}.
(15)
and /, g are the restrictions of / and g to Z. We see immediately that if there are first-class constraints present, then eq. (13) cannot hold because whole rows of A will vanish. Therefore in order for the Dirac bracket to exist, all constraints must be second-class. In general however there may be some first-class constraints. As stated before, we deal with them by adding more constraints (gauge fixing) such that the total set of constraints becomes second-class. This means that one has eliminated all first-class constraints and for that matter all gauge freedom. It is then clear that on the set of gauge-fixed elements there lives a Dirac bracket. If {0,(x)} is a set of second-class constraints, then the field theoretic analogue of the Dirac bracket is {F,G)* = {F,G}-jjdxdy{F,
(16)
where A'Kx, y) is the inverse of Au(x, y) = {$,(*), <£,(y)}, i.e. fdyAlk(x,y)Akj(y,z)=8ljS(x-z).
(17)
Let us consider the infinitesimal transformations generated by this Dirac bracket. Consider the situation where we have put a set of constraints on the system. Among these there may be first- and second-class constraints. The constraint surface will be denoted by P. Again we eliminate the unphysical degrees of freedom by fixing the gauge. Let's denote the set of gauge-fixed currents by M. M is then a subset of P such that every gauge orbit in P has one point in common with M. Suppose there is a gauge-invariant function H on the current algebra that commutes weakly with all constraints i.e. {//,0(x)}| P = O.
(18)
This means geometrically that the infinitesimal transformations generated by H via the PB leave P invariant. It does not mean however that M is left invariant. An element f of M will in general be transformed into an element f of P not belonging to M. However we can use the gauge freedom to transform this element
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637
into an element f" of M. The Dirac bracket then has the property that it transforms f into f" i.e. f" =f + &$,/ where 8*Hf= {H,f}*.
(19)
As was stated earlier, the purpose of this article is to obtain extended conformal algebras by reduction of the KM current algebra. It is clear from the foregoing that the reduced algebras will be Dirac bracket algebras. The requirement that the reduced algebras must be conformal leads one to consider constraints that are conformally invariant. By this we mean constraints that weakly commute with one of the (improved) Virasoro densities considered in the previous paragraph. If this is the case then the (conformal) transformations generated by this Virasoro preserve the constraint surface P. Put differently, in order to preserve conformal invariance, we may only constrain currents that are conformal scalars with respect to some improved Sugawara density. The improvement terms considered in the previous paragraph contain an arbitrary Lie algebra element A. We will consider the cases where A is the Cartan element of an sl2 embedding into s\N (if the KM current algebra we consider is an sl/y current algebra). The reason for this restriction is that in those cases it can be shown that there exist reductions that yield extended conformal algebras. Further more it turns out that by using group theory alone one is able to describe the resulting algebras in considerable detail. Let's consider the slN KM current algebra together with an embedding T={T„T+,T_}
(20)
of si 2 in sl/y. We will denote the ^-dimensional representation of s\M by dM (if M = 2 we delete the suffix). The adjoint representation of s\M will be denoted by ad M . Under the adjoint action of T, s\N decomposes into multiplets of irreducible si2 reps, with spin jk ad„= 0 2jk + 1.
(21)
k
This means that every element f of the current algebra can be written as A*)=
E
E
Uk'm(x)Tk,m,
(22)
k = 1 m = -jk
where Tk meslN is an element of an irreducible representation with spin jk and grade m. Here we always take 7, , = T+, 7\ 0 = T3 and r, _, = T_. Consider an improvement of the Sugawara density by the element TriT^djf) = t/1,0(jc). As can easily be checked, the currents Uk~l(x) are conformal scalars
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with respect to this improved Sugawara density. This means that they can be constrained to constants. For reasons that will become clear in a moment we impose the following constraints Ul-l(x)
= l,
(23)
!/*•-'(*) = 0
(V* = 2 , . . . , p ) .
(24)
The currents Uk,m with m < - 1 have negative conformal weights with respect to the improved Sugawara. Of course we must constrain these fields on physical grounds. There is only one way to do this if we want to preserve conformal invariance, namely we must put them to zero (since these currents are not conformal scalars they only commute weakly with the improved Sugawara density if they are zero). The set of primary constraints we therefore impose is <j>1-\x) = U1-1(x)-l=0, 0 * . - i ( x ) = !/*.-!(,) = 0 Ukm(x)=0
(25) (V* = 2 , . . . , p ) ,
(V*,Vm<-l).
(26) (27)
By construction this is a set of first-class constraints which implies that they generate gauge transformations. From eq. (5) we conclude that the gauge freedom generated by a first-class constraint involving a current of weight h can be fixed by adding a constraint involving a current of weight —h + 1. Therefore if all grades are integer the total gauge freedom is enough to bring the constrained currents into the form ^(x)
= T_+ZUk'k(x)Tktk,
(28)
k
because we can eliminate grade by grade until we end up with the highest weights. In those cases we take P to be the subset of KM currents specified by the constraints (25). Unfortunately, whenever a grade - 1 / 2 appears it requires secondary constraints to bring f(x) into the highest weight gauge. The reason is that it requires a grade - 1 / 2 field to eliminate a grade - 1 / 2 field. These secondary constraints are second-class, since the commutator of two of these constraints will be of grade - 1 . In terms of conformal weights this amounts to the statement that a constraint is second-class if and only if it has conformal weight 1/2. In other words, if the branching of the adjoint representation of slN contains half-integer spin representations of the sl2 subalgebra, then second-class con-
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639
straints are necessary. In those cases the vector 8 whose elements are given by «.- = (n)i..--( 7 "3)/ + ..,- + .
(i = h...,N-\).
(29)
will contain half-integer components (28 is the so called "defining vector" used by Dynkin [8] to characterize the embedding). Therefore, the constraints are all first-class if and only if the vector 8 contains only zeros and ones. The distinction between the two types of constraints is essential if we are to consider quantization of the algebras, because second-class constraints involve auxiliary fields (see e.g. ref. [9]). The status at this point is the following: we have a constrained surface P and we have identified a set of gauge fixed elements M (the set of elements of the form (28)). We show next that the currents Uk,k(x) are primary fields of spin jk + 1 with respect to the induced conformal action on M. Consider the following generator Q'empr of conformal transformations on the current algebra QTP'= fdxe(x)Limpr(x).
(30)
An explicit calculation using eq. (16) yields
s,Ax(y) = -{Gimpr,A,x(y)} = (^f i x)' + ^'T 3 + E'[7'3,Ax]-
(3i)
We know (by construction) that these transformations leave P invariant because Qiimpr c o m m u t e s weakly with the constraints. As stated earlier, <2™pr then gener ates a (conformal) action on M. In order to calculate this action we must calculate the compensating gauge transformations. Let ffiX be an arbitrary element of M. Inserting the explicit form of f^ into eq. (31) we find S £ A x = L(e(Uk-ky
+ (jk+l)sVk-k)Tk:k+Ks"T,.
(32)
k
We see that ,/ fb( + 8tS(ix is no longer in M because of the last term. We can "correct" this however by applying the infinitesimal gauge transformation gener ated by r= -KS"T+, i.e. 8rSra=[r,Sra
]+xr',
(33)
such that S,*Ax = S, A x + 8 r / n x
= (£((/'•■)' + 2e'U1-1 - « V " ) r i t l + £ (e(Ukk)'
+(jk+
l)e'Uk-k)Tkli,
* =2
(34)
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from which it follows that the currents Uk'k for k > 1 are primary fields with respect to the conformal action induced by L'mpr on M 8?Uk'k = e{Uk-ky + (jk + l)e'Uk-k.
(35)
In the calculations leading to eq. (34) explicit use has been made of the fact that [T+,Tk k] = 0. Also the particular form of the elements of M (notably the fact that Ul'l(x) = 1) is crucial. Since Ul'° = 0 on M the improvement term of L'mpr is zero on M. It can easily be checked using the relation (34) that the quantity (l/2K)Tr(^x)|M
(36)
is a Virasoro density with respect to the Dirac bracket on M. From this we conclude that by performing the reduction in the way described above we can associate an extended conformal algebra to every sl2 embedding. In order to calculate the entire algebra we need to evaluate the Dirac brackets between the currents Uk,k(x). A glance at eq. (16) makes it clear that this calculation would be very messy. Fortunately in ref. [4] a clever method was developed to calculate these Dirac brackets in the case of the principal embedding. It is not hard to show though, that it generalizes to arbitrary embeddings, even to arbitrary second-class submanifolds. We will now summarize this method. Let M be again the space of currents of the form (28). Consider the variation %
.,>U"'k(y)=-{Qlai
k
ap),U
-"(y)}\
(37)
where
G(fll
ap> = fd*L"l(x)UU(x),
(38)
/ and (al,...,ap) are arbitrary test functions. Now, also consider all elements R of the KM algebra i.e. *(*)=£ k
R(xtmTk,m
t m =
(39)
-jk
such that for all fhx e M we have Tr(^ fix ( x)R( x)) = Lak(x)Ukk(x)
+ C(x)
(40)
k
where C(x) are terms not depending on ffix. Of course R(x) will depend on the functions a,-(*). The relation (40) does not fix R completely. A crucial statement is
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that for any fVn e M there exists a unique element R(a, fViy) (i) R(a, ffa) satisfies eq. (40) for all flm e M,
641
such that
(ii) Sn* + W«> A«). Sr«\ + **'(«• A x > e M. Finding R boils down to solving two algebraic equations. This element R then has the following property [R{a,Sr*),Sra]+KR\a,Sr»)=T.8Wk'k<-x)Tk.k
(41)
k
= -I/fdyak(y)[U''(y),Ukk(x)}*Tll.
(42)
Since the left hand side of this equation is known we can "read o f f the Dirac brackets in the expression on the right. In the remainder of this article we will denote 8*Uk-k(y)
= -fdxai(x){U''(x),Ukk(y)}*.
(43)
4. Kac-Moody and WN subalgebras By construction the residual conformal algebras, which will be denoted by J/ red , contain a Virasoro generator with respect to which all other fields are primary. j / r e d may also contain a KM as well as W^ subalgebras. The residual KM algebra will correspond to the centralizer C of T in sl N . This follows from the observation that the generators of C, being singlets and hence highest weight vectors under T, survive in fixx (28). This means that the associated currents survive the reduction and obtain unit conformal weights. It is easily verified (using the algorithm) that these currents will indeed form a KM current subalgebra, since for the currents corresponding to C the Dirac bracket is the same as the original bracket. To obtain the W^ subalgebras of s/ied we have to consider the embedding in more detail. The sl 2 embeddings in s\N (are up to conjugacy) determined by the branching of the fundamental representation N_N. This implies that the number of inequivalent embeddings is given by the number of partitions of N. Let the branching of T in si N, in terms of sl 2 representations of spin j , be given by NN^
© N,{2j+1),
(44)
(;}
then C is of the form* C= © g l
v
* In the following it is understood that the overall U(l) factor is to be neglected.
(45)
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F.A. Bais el al. / Chiral algebras
In other words under C ® sl 2 the decomposition reads N_N^
© N,92j+l. 0) —
(46)
Hence for the branching of the adjoint representation ^NSQL9N)N-1,
(47)
we have a d „ + 1 -> © (A/;. ® AT) ® (2/ + 1 ® 2j + 1)
= © (ad/vy + I ) ® ( I © 3 e ... © 4 / + 1 ) 0) © IN, ® AT) ® (2|/ - / I + 1 © . . . 2 \ i + j \ + 1).
(48)
The relevant subalgebras are contained in the first term, which becomes first term = © (ad* + 1 ) ® 1 © 1 ® ( 3 © . . . © 4 / + 1 ) 0>
'
U)
© (adyvj ® (3 © ... © 4j + 1). 0')
(49)
The terms in this expression have the following interpretation. The first term corresponds to the aforementioned KM subalgebra (i.e. a direct sum of gl N KM subalgebras). In the second term all singlets under C have been collected. By definition these singlets generate the centralizer P of T in sl^. In fact up to U(l) factors we have P = © sl 2 ,- +1 ,
(50)
{/}
as follows directly from eq. (44). As can be seen from eq. (34) for each j value the term 1 ®(3©...©4/ + l)
(51)
corresponds to a subalgebra of fields with conformal weights which run from 2 up to 2) + 1. Using the fact that the embedding T is principal in P and that principal embeddings yield W t reduced algebras [4] we conclude that the second term in (49) corresponds to a direct sum of (mutually commutative) W 2j + 1 subalgebras. These W2, + , subalgebras also commute with the KM subalgebra in j ^ r e d .
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643
The third term in eq. (49) corresponds for every / to a direct sum of multiplets, with conformal weights that run from 2 up to 2/ + 1. These multiplets form adjoint representations of the slN KM subalgebras. The remaining terms in eq. (48) correspond to multiplets of fields that transform non-trivially under both C and P. The corresponding currents that survive in /Vyx should be primary fields both with respect to the KM and Wt subalgebras. To illustrate the structure of the algebras that emerge after reduction, we now turn to a detailed discussion of some examples. 5. Examples In this section we will consider some representative examples of reductions associated to sl2 embeddings. 5.1. THE TRIVIAL EMBEDDING N->N-l
A trivial example of an embedding of sl2 in s\N is provided by HN^N-1.
(52)
In this case, T = 0. Therefore we cannot constrain the currents, and we are left with a chiral algebra which is the original Kac-Moody algebra. Indeed, this is consistent with the observation that T is centralized by slN itself. 5.2. PRINCIPAL EMBEDDINGS N->N
Another well-studied example is the reduction associated to the principal embedding of sl2 in sl^ NN^N.
(53)
Under this embedding, the adjoint of s\N decomposes into N - 1 representations with spins ranging from 1 to N— 1. The resulting conformal algebra consists of N - 1 fields with conformal weights ranging from 2 to N, and it coincides with the WN algebra, as was already shown in ref. [3]. In the next examples we will study some new classes of algebras that have the generic feature that they contain coupled Wn and KM subalgebras. 5.3. "SUM'-EMBEDDINGS M + N->M + N-l
Let us first consider the embedding 2 + 7V-> 2 + N • 1. The centralizer of the corresponding T with 7 3 = (1/2,0,...,0, - 1 / 2 ) is of course sI^eUG), i.e. in terms of representations of the centralizer C we have N+2„^->(lQ2) + (N„9l).
(54)
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Under this embedding the adjoint decomposes as follows ^N
+
2^(^N®I)
+
( ^ ® 2 ) + (5A,®2) + (1®3) + (1®1).
(55)
Using the results of the previous section we conclude that the resulting algebra j / r e d contains (i) an slN KM current subalgebra (due to (ad N ® 1)\ (ii) a multiplet of N spin 3/2 fields that will transform in the fundamental representation of the slyv KM current subalgebra (due to (N N ® 2)), (iii) a multiplet of N spin 3/2 fields that will transform in the conjugate fundamental representation of the slN KM current subalgebra (due to ~N_N ® 2)). (iv) a spin 2 field (due to (1 ® 3)). Since it is a singlet representation of the KM current subalgebra, it will commute with it. (v) a spin 1 current (due to (1 ® p), that will commute with the KM current algebra as well. For N = I this corresponds to the embedding 3 -> 2 + 1., which together with the principal and the trivial embedding exhaust the reductions of sl3. For N = 1 the s\N subalgebra is absent, which leaves only the fields {j,G,G,T}. This algebra has been anticipated in ref. [5] and was studied in ref. [9]. Let us now turn to the explicit construction of s/ted for arbitrary N. The gauge-fixed form of f in the highest weight gauge looks in blockform like j
G
T
0 fN-(l/N)j
G
1
0
(56)
j
Here fN = (AaX/a where {A0} is a basis of %\N. It is these currents that will generate the sl^, KM current subalgebra of -s/ted. G(G) is a column(row) of what will become weight 3/2 fields. The grade - 1 / 2 fields have been set to zero according to the discussion in sect. 3. These are second-class constraints. The constraint ./bottom-left = 1 is first-class, but the gauge freedom generated by it has been eliminated by the constraint ,/,0p_ieft =^bottom-right- Finally, the field T is a weight 2 field. For the calculation of the algebra the matrix # that satisfies eq. (40) has to be constructed. Again in blockform it reads
R=
I t
RN~(2/N)r
(57) r - c o/
such that Q = Tr(SraR)
= Tr(SNRN)
+ g-G + G g + (T + (N + 2/N)rj + c\.
(58)
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F.A. Bais el al. / Chiral algebras
645
Here r, g, g, t and RN play the role of a,, a 2 , . . . in eq. (40). They correspond to the currents j , G, G, T and fN respectively. The parameters c 0 , c,, c 2 and c 3 can be solved explicitly by imposing 1
8j Vfix = [ ^ A J + ^ = 0 0
8G 8fN-{2/N)8j 0
8T^ 8G
(59)
5/
for the constrained currents. Inserting the expressions thus obtained for c, into the expressions for the variations 8j, 8G, 8G, 8T and 8fN we find the reduced algebra s/ied. For instance, one easily checks that *SN = [RN,SN]+dRN-G-g
+ g-G.
(60)
Since eq. (60) contains neither r nor t, fN commutes both with / and with T. The first two terms are recognized to amount to the anticipated Kac-Moody algebra, while the latter two fix G and G to transform in the two fundamental representa tions {j°(x),Gt(y)}=-(\°)uGl(y)8(x-y),
(61)
{j"(x),Gi(y)}
(62)
= (nA(y)8(x-y).
In fact, upon rescaling j with ^(N + 2)/N the index a can be made to in clude j as the 0th component J0 of a gl(AO current algebra, with (A°),; = - i/(N + 2)/2N8,j. From now on we denote \A = (A°, A") and f = JA\A. The variation of T with respect to t is easily shown to be the familiar Virasoro variation 8,T= -\d3t + 2Tdt + (dT)t.
(63)
However, as was shown in sect. 3, the Virasoro with respect to which all fields /, G, G and Ja are primary is L = \lx{fl) = T+\Tr{f*).
(64)
The only remaining non-vanishing variation is the variation of G due to G. Upon defining 9 = d-f,
(65)
this variation reads 8gG = (-S2+T)g.
(66)
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From this it is straightforward to reconstruct the Poisson algebra [Gi,Gj}=-8iJ8"(x-y)
+
2(\°)uJa(y)S'(x-y)
+ (-L8ij-^BJAJB(y)-(\)?jdJA(y))8(x-y),
(67)
where P I ^ = (A^ f l ) ( 7 + (ABA^),7 + g ^ 5 , 7 .
(68)
In this form the similarity with the N = 2 super conformal algebra coupled to SU(N) is prominent (see e.g. ref. [10]), but again we are dealing with a bosonic version of it. At this point it is worth discussing the role of the covariant derivative (65). Firstly, this operator appears generically whenever we organize the variations (43) according to the subalgebra and multiplet structures in the reduced algebra (see for example (60) and (66)). The description of the algebras in this way is much more elegant and transparent since it reveals structure rather than detail. Secondly, there is a striking similarity between the operator S?=3>2 -T in the r.h.s. of eq. (66) and the so called Hill operator obtained by setting 3l = d. The Hill operator plays an essential role in the hamiltonian formulation of the Kortewegde Vries (KdV) hierarchy, in the sense that the Hamilton operators of the hierarchy are known to be formal powers of this operator. In particular it is found that // 1 = (-^'/ 2 ) + = ^ , (69) H7l^{5fi/2)
3
+ =3
-2T3i-3iT,
(70)
are the basic Hamilton operators in the bi-hamiltonian structure. We note the remarkable fact that the variations 8R frn and 8tT are exactly given by the expressions (69) and (70), where it is understood that the covariant derivative is taken in the appropriate representation A of gl(A0. It is expected that new integrable hierarchies will be associated with the new extended algebras we constructed. Our observation suggests that the covariant derivative (65) shows up in the hamiltonian structure of these hierarchies. Here much further research is needed, however, this is outside the scope of the present paper. The hierarchy of algebras discussed above is easily generalized to Ww algebras with higher M. For instance, let us consider generalization of the previous example to the embedding N + 3-» 3 + N ■ 1. An important difference with the previous example is that the grading is now integer (as it will be for all odd M) such that the constraints can be imposed using first class constraints only. The resulting algebra consists of an s\N Kac-Moody algebra, a W3 algebra commuting with the Kac-Moody subalgebra, plus one U(l) current. Finally there are two sets of AT
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primary fields with conformal weight 2, denoted by W2 and W2. The fields W2 and W2 have opposite U(l) charge and transform in the fundamental representa tions of the residual Kac-Moody subalgebra. Both the W2 and the W2 commute among themselves. What remains is again the variation of W2 with respect to W2. In terms of the covariant derivative (where now (A°),; = - TJ(N + 3)/2N8u) this variation reads 8wiW2 = (9!i-2T3t-(®T)-W)w2.
(71)
The densities T and W are the spin 2 and 3 currents of the W3 subalgebra. This subalgebra commutes with the Kac-Moody subalgebra.
5.4. "PRODUCT'-EMBEDDING
MN--MN
Let us consider the first non-trivial "product"-embedding, namely 7V2->N2.
(72)
The centralizer of the corresponding 7" where now T3 = ( 1 / 2 , . . . , 1/2, — 1 / 2 , . . . , - 1/2) is sl/y, such that the adjoint decomposes as follows 5d2yv-*(5dAf®i)
+
(adA,®3) + ( l ® 3 ) .
(73)
Using the results of the previous section we conclude that the resulting algebra j / r e d contains (i) an sl N KM current algebra due to (ad^, l j (ii) a multiplet of N2 - 1 spin 2 fields that will transform in the adjoint representation of the KM current subalgebra (due to (ad N ® 3)). (iii) a spin 2 field due to (1 ® 3). Since it is a singlet representation of the KM current algebra, it will commute with it. In N X N blocks, the gauge fixed current reads J T . J
A x = L1
.
(74)
where 1 is the NxN unit matrix. It is easily checked that 2J is indeed an sl^ current algebra. The trace of T is the (singlet) Virasoro density that commutes with the Kac-Moody algebra. The traceless part of T is the multiplet of conformal weight 2 fields. All fields are primary with respect to the Virasoro ^ = l T r ( ^ ) = 5Tr(T)+Tr(J2).
(75)
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The variation of T with respect to T is given by 25,T= -3>H + 2[T,3H]
+
+ [S>T,t]+ ,
(76)
where [ , ] + denotes the ordinary matrix anti-commutator. Note that this algebra is nothing but the "scalar" W2 algebra minimally coupled to the sl N KM current algebra. This generalizes for higher M as well. The algebras will be Ww algebras minimally coupled to an s\N KM current subalgebra. The explicit form of this algebra is given in appendix A. 6. Quantization In the previous sections our considerations concerned classical constrained current algebras. As a first step towards quantization we compute the central charges of these algebras. The central charge of the unconstrained algebra is the Sugawara charge, which for an sl^ KM algebra of level k reads k dimG Sug
k+N - dim G - 12
P jk + N
where p is half the sum of the positive roots and where we have used the strange formula 12|p| 2 = NdimG. The linear improvement term (10) yields a contribution c impr = -6k Ind where Ind is the index of the embedding of T in si N. The index is easily calculated once T3 is given. In this case it is just given by Ind = 2Trace(r 3 2 ) = 2 | 8 | 2 .
(77)
If we are dealing with first-class constraints, then we only need to add the ghost contribution c ghosl which for a constraint for weight A amounts to a contribution of -2(6A2-6A + 1). Adding these contributions we come to the total contribution [21] 2
c = dim s/red - 12
Jk + N
-y/k+Nb
(78)
where dim j / r e d is the number of generators of the reduced algebra. However, if the algebra is second-class, quantization is not so straightforward. In particular the current algebra first needs to be extended with auxiliary fields such
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that the constraints can be imposed using first-class constraints only. This method was applied in ref. [9] to quantize the algebra associated to the reduction 3 -* 2 + 1., It also easily applies to the embedding N + 2-> 2 + N• 1. Apart from the first class constraint, there are 2N second-class constraints of weight 1/2. In this case this amounts to 2N auxiliary (bosonic) fields x, a r , d Xt since every second-class constraint has only one non-vanishing commutator. Therefore the total contribu tion of the auxiliary fields is 2 A f x ( - l / 2 ) , and the ghost central charge is now ( 1 / 2 , 1 / 2 ) for every spin 1/2 constraint, such that we arrive at the sum total of c = c^k-6k
+ N-2.
(79)
Another, certainly more laborious way of arriving at this central charge is imposing associativity. Similar to the calculation that has been done for the N = 2 superconformal algebras [10] it has been verified that the central charge of the algebra indeed agrees with eq. (79). Of course, this calculation yields more information than just the central charge, in particular the relation between the level in eq. (79) and the level of the KM subalgebra, and we hope to come back to this in a future publication [12]. Another important tool in the quantization of conformal algebras is the free field realization. In particular using the Wakimoto realization of sl^, a great deal has been learned about correlators [13], quantum group structures [14] and also the representation theory of WN algebra as reduced versions of sI N using BRST quantization [15]. In a sense, the Wakimoto realization is related to the principal embedding, which is most prominently clear from the point of view of the gaussian decomposi tion. Roughly speaking, to every positive (negative) root a bosonic ghost field W (X) is associated, whereas to every element of the Cartan subalgebra a free scalar field $ is associated. The scalar fields have a background charge Q such that the stress-energy tensor is of the form T^f^-WdX+^dtf
+ Qd2*.
(80)
This background charge has a value such that the total central charge c free fiC|d is equal to the central charge of the Sugawara density c Sug . The appealing feature of explicit realizations is that once the classical realization is found the quantization is an in principal straightforward procedure as it involves free fields only. Since we are interested in the generalization of the Drinfeld-Sokolov reduction to arbitrary embeddings it is no big surprise that parallel to the reduction an alternative "free"-field realization can be found. Since the resulting algebras in general have residual Kac-Moody symmetries, the realizations will interpolate between a current algebra and the Wakimoto free-field realization. The resulting realizations will therefore be referred to as hybrid field realizations.
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Rather than trying to develop the hybrid field realization in general, the example that is closely related to the familiar sl2 Wakimoto realizations will be discussed, which is the "producf'-embedding 2JV-> N2. Consider the decomposi tion of an arbitrary group element of sl2 into NxN blocks
- c ; « : : ) ( : *)• The diagonal elements g, and g2 are in principle gl(A0 valued. Calculating the current Jr = (dg)g~l yields
H"1 £)■
(82)
where //,=-XW + J,-/1,
(83)
// 2 = WX + J 2 + ; 1 ,
(84)
j+= - x w x - x j 2 + j , x + ax-2yi,
(85)
y_=W,
(86)
where we have redefined W = g 2 ' dVg, and J^ is the traceless part of (dQA)gA', while j is equal to the trace of ( d g ^ ^ 1 . Note that this realization is the spitting image of the one derived for sl2 (see e.g. ref. [13]), only now the fields are non-commuting in the matrix sense. From the WZNW action the canonical brackets can be derived. In terms of the matrix elements of X, W and JA they read {Xu,Wkl} = 8itSJk8, {(JA)u,UA)kl} = Sjk(JA)il8-Sll(JA)ki8 {)J)=8',
(87) + (8u8Jk-N-l8u8kl)8',
(88) (89)
where all level parameters are set to unity. All other brackets vanish, so in particular the algebra contains two commuting sl^ subalgebras. Using these brackets it is straightforward to check that f as it is defined in eq. (82) satisfies the sl2/v Poisson algebra. When it comes to quantizing, the different levels do get an intrinsic meaning. Replacing the Poisson brackets by the relevant operator product expansion one
191 FA. Baisetal. / Chiral algebras
651
finds 1 Xu(z)Wkl{z')~8u8jk
z-z 1
(JA)u(zKJA)kl(z')~8jk(JA)il-^—-8u(JA)ki: z-z +
z-z
Jz~^f[S"S'k~N8^'J'
(z-z) Since in eq. (82) products of fields are involved one has to be careful about the quantum equivalent of f in terms of the hybrid fields. However, it is straightfor ward to check that using the normal ordered expressions
//1=-(xw) + j1-9yi, // 2 = (wx) + j 2
+9yi,
y+= -(xwx)-xj 2 + j1x + *2A,ax-29;x, y_=w,
(9i)
we have a realization of the sl2A, algebra if and only if the different parameters are related through kN = k2N + N,
g2=
2N
■
(92)
The Sugawara in terms of the hybrid fields can be expressed as L*fi,kM = 2 Z * X + L*h°st + L^',
(93)
where LghosI is just the familiar expression TKWdX) and if0*1*' is the stress-energy tensor of a boson with background charge N. Using these relations it is easy to check that the total central charge indeed adds up to the correct value (N2-l)k„ , N , k2N((2N)2-l) C ^2-i^jr+2N'+,-6I^2Nk°N'= t „ + 2W •
<94)
The constraints (74) can now very easily be imposed. First W is put to 1, and secondly the induced gauge freedom is eliminated by solving for X such that
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H1-H2. The result can entirely be expressed in the two commuting sl^ subalgebras J = i ( J , + J2),
T = j2+9J,
(95), (96)
where we have denoted J = (J, - J 2 )/2 - qj and where the covariant derivative 9 = d + J acts on J in the adjoint representation. Using this realization it is straightforward to calculate that in particular (96) is a realization of (76). It may be interesting to note that this realization of the extended algebra can also be derived using a hybrid version of the Miura transformation. Consider instead of the form (74) the block diagonal choice of gauge
1
-H' °)-
(97)
The J, generate two commuting Kac-Moody algebras. The action of the operator d +f on a 2-vector (t/r,,t/f2) (with t/», an N-vector) is block diagonalized by (3 + J,)(a + J 2 ) ,
(98)
while (74) is block diagonalized by (d + J)(d + J ) - T .
(99)
Since the two operators are gauge equivalent, we can equate them, which immedi ately results in eq. (96). Another way of arriving at eq. (96) is by making use of the effective action which one can derive for the field equations after imposing the constraints for both the left and the right chiral algebra. In ref. [11] it was shown that this action contains the (scalar) Liouville action, essentially due to the fact that the grading element T3 centralizes P. Extending this argument to the complete centralizer of P we expect a covariant Liouville action, minimally coupled to an sl^ WZNW model.
7. Conclusion and outlook We have discussed the classical reduction of sIN WZNW models with respect to si 2 embeddings, resulting in new extended conformal algebras. It turned out that these algebras have a remarkable covariant structure. In some representative examples we also considered the quantization problem. Central values of some "first-class" examples were given and a hybrid realization, partially in terms of currents and partially in terms of free fields, was introduced which facilitated imposing the constraints.
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FA. Bats et at. / Chiral algebras
653
There are a number of questions that arise at this point, of which we would like to mention a few. (i) It is known that the W^ algebras can be obtained in a number of different ways: (a) Through imposing associativity. This method was originally employed by Zamolodchikov [16]. (b) By exploiting the coset construction as in ref. [2]. (c) By quantizing the second Gelfand-Dickii Poisson bracket [3]. For the algebras ob tained in this paper one would in particular like to know how they can be understood in terms of a coset construction, appropriately generalizing the ap proach of ref. [2]. Secondly, if we are using the hybrid realization we can easily construct actions which have the corresponding symmetries. Our examples indicate that one class of models exhibiting these symmetries are Toda theories covariantly coupled to WZNW models. (ii) It is known that the Virasoro and W^ algebras play a crucial role in the construction of hierarchies of non-linear partial differential equations of the KdV type. As we indicated in sect. 5 the hamiltonian structure of these hierarchies seems to be related to a covariant generalization of the Hill operator. This idea deserves further investigation. There is also an alternative way of looking at hierarchies in which the relation with the extended algebras is particularly manifest. This is the Hirota bilinear formulation as was pointed out in ref. [17]. Indeed once the relation with the coset construction for the new algebras is established, the construction of new hierar chies in bilinear form should be straightforward. It is an interesting fact that in the case of the principal embedding the field equations of the reduced theory (Toda) can be exactly solved by reducing the general WZNW solutions [18]. This implies that the field theories associated to the extended conformal algebras constructed in this paper are also exactly solvable. This interesting point was first made in ref. [6] and more recently in ref. [11]. (iii) Finally, it is worth extending this program to algebras other than sl^. In particular, reduction of superalgebras analogous to the one studied in ref. [20] might yield the fermionic N = 2 superalgebra, rather than its bosonic counterpart encountered in this paper. We would like to thank P. Bouwknegt and J. Fuchs for useful discussions and comments. P.v.D. is financially supported by the "Stichting voor Fundamenteel Onderzoek der Materie" (FOM).
Appendix A For convenience of the reader, we give in this section the explicit form of the Poisson algebra associated to the embedding 27V-»N2. However, it is merely a
194 654
FA. Bais el al. / Chiral algebras
demonstration of the powerful way of describing the algebras using the variation in terms of covariant derivatives. {Ju> hi) = 8uSjk8' + SjkJus ~ 8u hi8» Vu> Tki) = 8jk Tu8 ~ 8u
T
kj8>
{TtJ, Tkl) = 8u8Jk8m + (8uJki - 8ikJa)8" + (25,., Tkj + 28JkTu -38udJkJ + 38jkdJu - 38it JkmJmj + 6JitJkj - 38Jk JimJml)8' + - dTkj8lt - dTuSik - 8H d2 Jkj - 8jk d% - 33(JuJkJ) + 2(dJim)Jml8kj +JimdJml8ki + (dhm)Jmj8„ + 2JkmdJmJ8il +
hn^nm^mi8il
~ {hmTmj
+
~ ^hlhm^mj
+ TkmJmj)8il
+
^'im-'ml-'kj ~
+ UinJml
+
Jimhnhl8jk
T
imJml)8jk
2{J„Tki-TilJkj)8. References
[1] D. Gepner and E. Witten, Nucl. Phys. B278 (1986) 493; J.-L. Gervais and A. Bilal, Nucl. Phys. B238 (1984) 125 [2] F.A. Bais, P. Bouwknegt, M. Surridge and K. Schouten, Nucl. Phys. B304 (1988) 348, 371 [3] V. Drinfeld and V. Sokolov, Journal of Soviet mathematics 30 (1984) 1975; V.A. Fateev and S.L. Lukyanov, Int. J. Mod. Phys. 3 (1988) 507 [4] J. Balog, L. Feher, L. O'Raifeartaigh, P. Forgac and A. Wipf, Ann. Phys. (N.Y.) 203 (1990) 76 [5] A. Polyakov, Int. J. Mod. Phys. A5 (1990) 833 [6] F.A. Bais and W.P.G. van Velthoven, Physica 139A (1986) 326 [7] P.A.M. Dirac, Lectures on quantum mechanics (Yeshiva, New York, 1964); K. Sundermeyer, Lecture Notes in Physics 169 (Springer, Berlin, 1982); Sudarshan, Mukunda, Classical dynamics, a modern perspective (Wiley, New York, 1974) [8] E.B. Dynkin, Amer. Math. Soc. Transl. 6[2] (1967) 111 [9] M. Bershadsky, Conformal field theories via hamiltonian reduction, IASSNS-HEP-90/44 [10] K. Schoutens, A. Sevrin and P. van Nieuwenhuizen, Commun. Math. Phys. 124 (1989) 87 [11] L. O'Raifeartaigh and A. Wipf, Dublin preprint DIAS-STP 90-19 [12] F.A. Bais, J. Fuchs, T. Tjin and P. van Driel, to be published [13] A. Gerasimov, A. Morozov, M. Olshanetsky, A. Marshakov and S. Shatashvili, Int. J. Mod. Phys. A5 (1990) 2495 [14] P. Bouwknegt, J. McCarthy and K. Pilch, MIT preprint CTP#1898 [15] M. Bershadsky and H. Ooguri, Commun. Math. Phys. 63 (1985) 1205 [16] A.B. Zamolodchikov, Theor. Math. Phys. 65 (1985) 347 [17] F.A. Bais and K. de Vos, The algebraic structure of integrable hierarchies in bilinear form, ITFA 90-04 [18] P. Forgac, A. Wipf, J. Balog, L. Feher and L. O'Raifeartaigh, Phys. Lett. B227 (1989) 214 [19] A. Polyakov, Mod. Phys. Lett. A2 (1987) 893 [20] G.M.T. Watts, Ph.D. thesis, DAMPT, 1990 [21] P. Bouwknegt, J. Math. Phys. 30 (1989) 571
195
Reprinted with permission from Communications in Mathematical Physics Vol. 146, pp. 403-426,1992 01992 Springer- Verlag
Super-Toda Theories and W-Algebras from Superspace Wess-Zumino-Witten Models F. Dddoc1, E. Ragoacy2, and P. Sorba1 2 1 Laboratoire de Physique Theorique, ENS Lyon, 46 Alice d'ltalie, F-69364 Lyon Cedex 07, France 2 Laboratoire de Physique Theorique, LAPP, Chemin de Bellevue, BP 110, F-74941 Annecy-le-Vieux Cedex, France
Received October 20, 1991
Abstract Using a superspace approach, it is proved that a N= 1 Super-Toda theory can be seen as a constrained WZW model based on a supergroup. The gauge transformations which survive the constraints are then used a la Drinfeld Sokolov to determine explicitly the super- Walgebra underlying this theory. The conformal spin content of any such super- H-'algebra is provided in the general case. 1. Introduction Rather recently, it has been remarked and exploited that Toda theories can be identified with some gauged Wess-Zumino-Witten (WZW) theories [1]. More precisely, a Toda theory can be seen as a WZW theory with constrained KacMoody currents, these constraints generating gauge transformations of special interest. Such a property is interesting for at least two reasons. First, because it relates two cornerstones of two dimensional conformal field theories, namely WZW models and Toda theories. Secondly, since this connection provides a direct method for the construction of W-algebra in Toda theories, the W-generators showing up as gauge invariant polynomials in the constrained currents and their derivatives. It is the generalization of such properties to the N = 1 supersymmetnc case, namely the possible relation between supersymmetnc Toda theories and superWZW models that we propose to examine in this paper. As is well known, a superToda theory is based on a simple superalgebra admitting a simple root system (S.R.S.) made only of fermionic roots [2]. Properties of super-Toda theories and some consequences for super- Walgebras have already been considered [3-5]. A first approach to recognize super-Toda theories in constrained super-WZW models based on supergroups has also been proposed in [6]. However, in this paper the WZW action is not explicitly supersymmetnc, and the treatment, not * URA 14-36 du CNRS, associee a l'E.N.S. de Lyon, et au L.A.P.P.
1%
404
F. Delduc et al.
being based on superfields but rather in their components, does not seem to be well adapted for the construction of super- W algebras. Hereafter, we will start from a manifestly supersymmetric WZW action associated with a supergroup (S. Mimicking the non-supersymmetric case, and imposing constraints on the supercurrent components associated with fermionic simple roots, we will obtain the N = l super Toda theories. In order to make complete this gauge theory approach, we consider in a special paragraph the "component action," and recover the action given in [6] as the one associated to a Wess-Zumino gauge, obviously not covariant under supersymmetry (Sect. 2). The general construction of ^components is considered in Sect. 3. Once again, we will develop a method analogous to the one used in [1] for the nonsupersymmetric case. The new feature here is that a super Toda theory based on a Lie superalgebra si involves the superprincipal embedding of OSp(l 12)- we denote it OSp(l|2)ppal - instead of the principal embedding of Sl(2) as it appears in a Toda theory based on an algebra. General formulas for the decomposition of any simple Lie superalgebra s/ with a completely fermionic S.R.S. into repre sentations of its OSp(l|2)pptl are established in Sect. 4. From such tables, one can deduce the spin content of the W-generators associated with a j^-super-Toda theory (Sect. 5). Then, in Sect. 6, we illustrate our results on a few simple cases, before discussing further developments in the conclusion. 2. W.Z.W. Action with a Supergroup, and Gauge Constraints We start this section by fixing some notations. Then, we write explicitly the W.Z.W. Lagrangian based on a supergroup in a manifestly supersymmetric framework. The adjunction of a second term to this expression will lead to the complete gauge invariant supersymmetric action associated with N = \ superToda theories. Finally, examining in some detail the components of the involved superfields, we can prove that the treatment presented in [6] and denoted "hidden supersymmetry" is obtained from an action through the use of a Wess-Zumino gauge. 2.1. Some General Notations and Properties Super-Toda theories imply the use of special simple Lie superalgebras namely superalgebras s/ equipped with a completely fermionic simple root system (SRS) and admitting an OSp(l |2) principal embedding (see Sect. 3.2). They are of the following type [2, 7]: Sl(n + l|n), OSp(2n + l|2n), OSp(2n|2n), OSp(2n + 2|2n) n ^ l and D(2, 1; a) a+0, - 1 . For brevity, we will call these superalgebras "fermionic" superalgebras1. By <, > we denote in s/ the unique (up to a constant factor) non-degenerate, invariant, supersymmetric bilinear form; such a form exists for any contragredient - or basic - simple Lie superalgebra [7]. In the Chevalley basis, the Cartan generators H,(i — 1,..., r = rank(^4)) and the fermionic generatorsE±at associated to 1 Note that although each superalgebra PSl(n|n)=Sl(n[n)/t/(l), n # 1, possesses a fermionic SRS, it does not give rise to an OSp(l|2) principal embedding
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the simple root system J + ={a 1 ) ...,a r } satisfy the Commutation Relations (C.R.):
{£+„,, £_.,} = JyHi. [H J t Hj]=0,
(2.1)
where X is the (symmetric [8]) Cartan matrix defined by Xy=(o,,a / )s
(2.2)
Moreover one has <»„£*.,>«<£*„, E ± „>=0, <£„,£_„> = *„. We will denote by K the entries of the inverse Cartan matrix, i.e.:
(2.3)
iJ
KiJKJk=S[.
(2.4)
General results on superalgebras and their Dynkin diagrams can also be found in [9]. 2.2. Gauged Wess-Zumino-Witten Action The hght-cone coordinates of the world-sheet (1,1) superspace will be denoted by x ++ ,x"",J7 + ,>;".The index refers to the Lorentz weigh t carried by the coordinate. The supersymmetric covariant derivatives D± satisfy (D±)2 = i3 ± ± , {D+,Z)_}=0. The superfield G(x, n) belongs to a supergroup *§ such that the corresponding superalgebra sd admits a set of simple roots all fermionic. We shall denote by A the automorphism of the superalgebra sd which changes the sign of anticommuting generators and leaves commuting generators unchanged. The same notation will be used for the corresponding automorphism of the supergroup. The starting point is the WZW action S0(G) = fKxd2»;[<(G-1D+(?),(C-1D_G)> + Jdt<(G-1atG),((G"1r>+(5)(G-1D_G)+(G-1D_G)(G-1D+G))>]. v(2 5) The corresponding equations of motion read ' ' D_(G _ 1 D + G)=0oD + (D_GG- 1 )=0.
(2.6)
The action (2.5) satisfies the Polyakov-Wiegmann relation S0(G1G2) = S0(G1)+S0(G2) + Kjd2xd27<(Gr1fi+G1)) (D.G2G^)}.
(2.7)
We denote by s/+ (respectively s/-) the superalgebras spanned by the generators of J / corresponding to positive (respectively negative) roots with respect to the Cartan subalgebra Jtf. The supergroups corresponding to sf+(s/-) will be denoted by #+(#_). In order to gauge the left action of 9+ and the right action of
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F. Delduc et al.
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#_, we make the transformation G-+aGp, where a andfiare superfields belonging respectively to'S + and # _. Then one finds: S0(xGp) = S0(G)+Kld2xd2r,\_«a-lD+&\ (D.GG"1)) + <(G-1Z)+G),(D_/?r,)> +
(2.8)
One can introduce the gauge superfields A+=a-iD+&es/+,A-=D-Pp-1es*-Moreover, we introduce the constant elements fxes/- and ves/+ which have non-zero elements along (fermionic) simple roots only: A«= I ft£-.,.v= £>,£„. (-1
(2.9)
(=1
Then the complete gauge-invariant superspace action which leads to the supersymmetric Toda models is S(G, A+, A _)=S0(G)+K\d2xd2n [{A+, (D_ GG~l -fi)) + <(G-1D+(5-v), X_> +
(2.10)
and the infinitesimal gauge transformations of the superfields are SAtl}G = AG + Gi2, dAt(p= -aA=>SAtaA+ = -D+A + AA+ -A+A,
(2.11)
&A,aP= -QP=>fiA.oA- = -D-Q+A-Q-fiA-, where the superfield A belongs to the algebra s/+ and the superfield Q belongs to jtf_. 23. Component Action When turning to components, we shall use the superspace gauge freedom to eliminate all components of the superfields which transform into a supergauge parameter without space-time derivatives. Thus, from the transformation laws Kt>A + \n=o = I>+A=o+-,&A.n(D-A+)\,=0
=
(D-D+A)\ll=0+...,
we deduce that one can find a gauge such that i4 + |,_ 0 =0,(D-i4 + )|,_o=0.
(2.12)
In the same way, one can choose A_|,_ o =0,(D + A_)l,-o=0. We are then left with the physical gauge fields defined by A++(x) = (D+A+)\,,0,A__(x)
= (D.A_X=0,
and with the auxiliary fields Z+=(D-D+A+)\,=0,Z-=(D_D+A-)\,=0.
(2.13)
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Then we define the components of the superfield G(x, TJ) by g(x) = G | , = 0 ) V - = ( i ) _ G G - % = 0 > V + = ( G - 1 Z ) + < 5 ) | , = 0 . The auxiliary fields at the second level in t\ play no role in the sequel and will be ignored. The gauge transformation laws of y _ and \p+ are as follows: These components of the superfield parameters have not been used in (2.12,2.13), and one can thus choose a gauge such that V-L*=0,V+L-=0.
(2.14)
We have now used all the parameters of the supergauge transformations beside the ordinary gauge parameters X{x)=A\^=0 and
(2.15)
As a result of (2.14, 2.15), tp_ and y+ reduce to where x + and x - belong to the Cartan subalgebra Jf. Then the component form of the action is
s=|^ 2 x
2
(id..gg-l-fi2
+ [x-, |i])>
1
-2<(«g- 3 + + g + v - [ z + , v]), X__>-2
(2.16)
with the following gauge transformation laws: <5-i.<0«=^g + g<». $z.
(2.17)
where 1 (respectively a>) is the restriction of X (respectively GO) to anticommuting generators corresponding to positive (respectively negative) simple roots. The action (2.16) coincides with the one given in [6]. In particular, the constraints derived from the A + + equations of motion are «a._gg-1|J,.=iUM-[z-,M]-g^--g-1. (2.18) In the gauge A _ _ = 0, we recover the constraints of [6] including the fermions X-, in which the non-zero currents correspond to the anticommutators of two simple roots. Thus, the origin of the supersymmetry of their action is now clear: it is just an ordinary supersymmetric action in a gauge which is not covariant with respect to supersymmetry. The supersymmetry transformations of the fields are easily
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obtained from the transformations of the superfields. One finds
5 v _ = £ " ( i 3 _ _ g g " 1 + g ^ _ _ g " 1 ) | ^ , ^V'+=« + 0'g" 1 3 + + g + g" 1 >4 ++ g)| J r. 6A + + =e-(\p.A+
+
-A+
+v_)L,,
8A-- = - £ + ( v + / l _ _ -A._v+)L.
• (2.19)
It takes some time to check that these transformations are an invariance of the action (2.16), and also that the commutator of two such transformations with parameters £ and e' closes, up to field equations, on a translation and on a field dependent gauge transformation [^<5']g = 2i(e'-e-3__g + e' + e + a + + g)-l-^, 0 ) g with X=-2e'-e-{id__gg-l+gA-_g-l)\J,. + +
l
a>=-2e' e (ig- d++g
+
+ 2e'+e+A+
+
,
1
g- A++g)\J,_+2e'-e-A--.
3. Super-Toda Theories and Super- W Algebras Here we will use the gauge invariance properties of the action given in Eq. (2.10) to recognize the N=1 Super-Toda theories. Then the construction of the ^elements associated to such theories will be achieved by generalizing in the supersymmetnc case the Drinfeld-Sokolov gauge used in [10]. 3.1. Constraints and Super-Toda Action Coming back to the gauged WZW action (2.10), one can write down the corresponding equations of motion. Then, making use of the gauge invariance and setting A+ = A_ =0, one gets as Euler equations those of the super-WZW model Z)_(J)=0oD+(J)=0,
(3.1)
where J and J are the supercurrents J=KD.GG-1,J=KG-1D+G
(3.2)
together with the constraints <£.,D_GG-1-/i>=0, <£_., G - 1 D + G + v > = 0
(3.3)
for any ae77 + =set of positive (bosonic and fennionic) roots. That is also, using relations (2.9): <£.„ D.GG~ly 1
= ui, <£., D . G G - ^ O , l
<£_«„ G" D + G>= - v „ <£_., C- D+G + v}=0,
(3.4) (3.5)
with CL,eA+ and <xeIl+\A+. Recalling that n, and v, are constant quantities, these constraints are obviously the supersymmetric analogues of the ones of [1].
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In order to recognize in the Lagrangian, as well as in the equations of motion, the N = i super-Toda theory, let us restrict ourselves to supergroup valued superfields G admitting a local Gauss decomposition G = ABC
(3.6)
with A=exp(
X X°E\B=exp(
i
£ Y'E_t),
(3.7)
where E± „ is the bosonic or fermionic generator associated to the root ± a e II + . The d>*(x + ' + ,x~'",n +,rj~) — denoted for simplicity by d> - are bosonic superfields, while the X* and Y" are bosonic (respectively fermionic) local superfields following the corresponding generator E±a is commuting (respectively anticommuting). From the constraints (3.4) and (3.5) we deduce the equations AlD+A=
I v^.exp (I
D.CC-^
£ n,E-.texp(
K./PA, I Ktfll),
(3.8) (3.9)
which, together with the Polyakov-Wiegmann relation (2.7), lead to the action S(G) = $d2xd2r, | - KtJD _
(3.10)
where r is the rank of the supergroup (S. The exphcit form of the equations of motion can be calculated from (3.10): one gets the r=rank(9) equations of the N = 1 #-super Toda theory D_/)+
r).
(3.11)
Now it is a simple exercise to verify that the invanance group of the constraints (3.4) (respectively (3.5)) is exactly generated by the elements Q(x~~,n~)e'3+ (respectively
1
1
J^d- J<j+&- (D+o)=Ad*(
(3.12) (3.13)
3.2. The Algebra OSp(l|2) and Super-Toda Theories It is known [11] that the superalgebra OSp(l|2) must play in Super-Toda theories a role analogous to the one played by Sl(2) in Toda theories [2]. This will be seen explicitly in the following. Let us concentrate on the supercurrent J = J(x~~,n~). The constraints (3.4) impose J to be of the form J(x--,r,-)
= J-i+l a*6d+
£ Xa(x~~ ,n~)Ea,
(3.14)
86/7 +
where we now call for convenience J_ 4 the quantity n defined in (2.9) •/_♦=/!= ! * £ - „ , . 1=1
(3.15)
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Then, defining
'♦*-E^(lK y W
(316)
H=^{J.i,J^} = ^i^HJ,
(3.17)
and
it is straightforward to verify that lH,J±i]=±y±i.
(3.18)
Defining also *±-i{J±*.-'±*}. we can check that these last quantities are not zero since
(3-19)
V±,J*t]=-2[.H,J±i]=+J±i
(3.20)
by using the Jacobi identity. Finally the C.R. ll*i,X*1=0,[H,X±-]=±X± (3.21) complete the proof that generators {J±i,X±,H} form a basis of an OSp(l|2) algebra. We note that this superalgebra constructed from (3.15) and (3.16) as a subalgebra of the si superalgebra, appears as the superprincipal embedding of OSp(l |2) in si: we denote it OSp(l |2)piJ-1 (as already mentioned in [1 ] for the case of algebras, the values of the \i{ parameters can be chosen equal to unity by reseating the step operators E±a{). Let us emphasize that, following (3.18) and (3.21), J±i and X± are eigenstates of H with the respective eigenvalues h = + \ and h = ± 1. Remembering the C.R. (2.2) any E±ai with *teA + satisfies [H,£±.(] = ± 1 i Kk%tE±ai = ±\E ±M .
(3.22)
From the decomposition of any root from simple roots and the Jacobi identity, we deduce that H provides a grading of the si superalgebra [H, EJ=hEh with h e \X. (k)
Each fermionic root belongs to an H-eigenspace si
(3.23) with h half-integer, while r
each bosonic root corresponds to an integer value of h. Denoting by
L,4i«..
(3-24)
and we have =0
if \hl+h2\>haMX.
(3.25)
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33. Determination of the Super-W Generators We are now in position to generalize to superalgebras the Drinfeld-Sokolov techniques for the characterization of W-generators. The power of this approach for Lie algebras has been made explicit in [1]. Let us rewrite (3.14) as "max
J= I Jh,
(3.26)
J0 being associated with the Cartan part and ./*(/» >0) to the roots of nlk) = {aen+/Eaes/ih)}. Now, consider a ^-element of the form: gho=exp(
Y G"E.U0£i.
(3.27)
One easily notes that (Ad*(gJ(J)-J)e
0
J/W
(3.28)
and the restriction of this quantity to s/
I
0-[£.,/-4].
(3.29)
Then it is natural to look for an element g^ annihilating the largest number of terms in •/»„-$. Repeating the process for the different values of h 0 ^ i , we will be left with elements belonging to the s/ subspaces ^<*o) = ^(»o)\j_ i (^(» 0 +i))
(3.30)
with As it will be explicitly shown in the next section, if n»0=dim^"(*o)=dimj/(*o>-dimJ_i(j/<*0+*)),
(3.31)
one has £ nM = r=rank(^),
(3.32)
8=8^.8*^-♦-** will allow to gauge transform J into
(3-33)
thus a suitable group element
J'=Ad*(g)(J)=J_ i + i WhlP™
(3.34)
with P<*',e^"<*<,> {^h^h^. Due to the complete reducibility of the s/ superalgebra into OSp(l|2)pp,i supermultiplets (see Sect. 4), the r elements i**'* we have to select in the Jr{kt) can be chosen such that J+i(P<*'')=0)/.(^i;« = l , - , r .
(3.35)
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Following [1] we will call such particular Drinfeld-Sokolov gauge the highest weight gauge. The Whi quantities are differential polynomials in the components of the currents J(x~ ~,n~). Their construction ensures that they form a complete set of gauge invariant polynomials, so that they will close under the Poisson Brackets (PB) of the theory and constitute a super- Walgebra. To determine the spin content of this algebra (Sect. 5), we have first to reduce the adjoint representation of each fermionic superalgebra with respect to its OSp(l |2)pp,, (Sect. 4). 4. OSp(l|2)ppa, Multiplets in Fermionic Simple Superalgebras In this section we study the decomposition of a fermionic simple superalgebra s/ into irreducible representations of its OSp(l |2)ppaJ subalgebra. Before presenting the results, let us recall some general properties of OSp(l |2) superalgebra. 4.1. Some Properties of the OSp(l|2) Superalgebra The following features about OSp(l |2) will be useful for the rest of the section. Proposition 1 [12]. Allfinitedimensional representations of OSp(l |2) are completely reducible. This ensures that the adjoint representation of a superalgebra s/ reduces to a direct sum of irreducible representations of its OSp(l|2)PIM,. Proposition 2 [12,13]. Any irreducible representation o/OSp(l|2) is characterized by a quantum number q = 0, ^, 1, \, ■ • ■ and decomposes under its bosonic part Sl(2, R) into two multiplets (q,q—i) for q 4=0 - the case q=0 reducing to the trivial (one dimensional) representation. We note that the dimension of irreducible OSp(l|2) representation R(q) is
(4fl + l)=(2q + l)+(2ta-i)+l). Proposition 3 [12,13]. The product of two irreducible OSp(l|2) representations decomposes as follows: R(qi)xR(q2)=
"'© 2 R(q),
(4.1)
« = l«l-«2l
q taking integer and half-integer values. As an aside comment, we remark that these properties confirm OSp(l|2) as the supersymmetric analogue of SI (2). We recall that OSp(l|2)ppa| in s/ is generated from the fermionic root: F _ i = i £ - I | , r = rank^
(4.2)
i= 1
(we repeat that the fit coefficients in previous sections are irrelevant since they can be absorbed by reseating of the £a/s). Then the negative bosonic root appears as the sum of negative roots which are simple for the bosonic part of s/, r
X_ = {F_ i ) F_ i }=>:£_ I /t(
(4.3)
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413
with r=r for si = OSp(2n ± 1 |2n), OSp(2n|2n) and OSp(2n+2|2n), and r = r - 1 for •af = Sl(n+l|n). 4.2. Reduction of a Superalgebra into OSpOPJpp,, Multiplets Let us consider separately each family of superalgebras admitting a fermionic S.R.S. 4.2.1. Sl(n + l|n) case (n^l). This is the simplest case. Indeed the Sl(n + l|n) fundamental representation (n +1)© n reduces with respect to OSp(l |2)ppal into the representation J?l - 1 = (D
where the sum goes over integer and half-integer q's. Therefore Sl(n + l|n)/OSp(l|2)pp.1 = R(n)©/?(n-i)©R(n-l)©...©R(i).
(4.5)
Let us add that the Dynkin diagram of Sl(n + l|n) relative to the S.R.S. is [9]
(g)—<8> V«2
«J-*!
.-l-£»
£
.-5n
5
»- £ ».l
The OSp(l|2)PIMll is built from F+i = Etl.ii + Eii.tl+-
+ Ein^i,
(4.6)
while the bosonic root is X + = { £ + i , £ + i } = £ei_.2 + - + £ £ n _^ 1 + £,1_),2 + - + £,„_1_a„.
(4.7)
Moreover, >W=4(2n)=n, that is the highest q value in the above R(q) decomposition.
(4.8)
4.2.2. OSp(2n—1 \2n) case (n ^ 1). The superalgebra OSp(2n—1 |2n) contains as its bosonic part the algebra 6(2n—l)©Sp(2n), and its fundamental representation reduces with respect to its bosonic part to (2n—l,l)©(l,2n). The (2n—1) fundamental of 0(2n—1) is irreducible with respect to the OSp(l|2)ppi, bosonic part, i.e. Sl( 1,1 )„„,, part, that is (2n — 1 )=D„-1, as well as the (2n) representation of Sp(2n):(2n)=/>._,. The adjoint of 0(2n — 1) can be obtained by taking the antisymmetric part in the product (2n—1) x (2n—1). In terms of Sl(2) representations, one can use the table of 0(2n-l) exponents [10] to get: 0»- 1 xD B _ 1 | / < = D 2 , _ 3 © D 2 l I _ s © - © D 1 .
(4.9)
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In the same way, the adjoint of Sp(2n) can be constructed from the symmetric product of (2n) x (2/i), and again the list of Sp(2n) exponents provides the result: B.-iXD..i|,=:Dto.1©D2,.je-eD1. (4.10) Fermionic generators in the adjoint of OSp(2n—l|2n) will be contained in the product (2n-l)®(2n), that is Dm_1xDB-i = D2a-i®D2a-i®:.®Di.
(4.11)
Using Proposition 1 and Proposition 2, one can gather the Sl(2) representations of (4.9), (4.10) and (4.11) into OSp(l|2) ones in an unique way to obtain OSp(2n - 1 |2n)/OSp(l |2)ppal = R(2n - 1 )© R(2n -f)®R(2n - 3)©... ...©J?(2(n-p)-l)©R(2(n-p)-|)©R(2(n-(p + l))-l)©... ...®K(f)©K(l). (4.12) The Dynkin diagram associated to the fermionic S.R.S. is
<8>—®—<8>
0->-i ,
where there are 2(n—1) grey dots (®) and the black dot (#) corresponds to an OSp(l|2) fermionic root. One notes that hmMT=U2+-+2)=2n-l (4.13) indeed corresponds to the highest g-value in the above R(q) decomposition. 4.2.3. OSp(2n +1 \2n) case (n ^ 1). We can follow the same method as the one used just above, replacing (2n—1) by (2n + l). The result is OSp(2n+1 |2n)/OSp(l |2)ppmI = R(2n -i)©R(2n - 1)©R(2« -f)© • • • •••©R(2(«-p)-i)©/?(2(w-p)-l)©/?(2(n-(p+l))-i)©•••©/?(§)© R(\).
(4.14)
The OSp(2n+ l|2n) fermionic Dynkin diagram is
<8>—<8>—®
0->-#
,
where there are (2n—1) grey dots. The value *.».,=4(2(2n-l)+l)=2n-i does correspond to the highest R(q) representation.
(4.15)
4.2.4. OSp(2n|2n) (n> 1) case. We recall the isomorphism OSp(2|2)sSl(2|l). The reduction of the adjoint of 0(2n) and of Sp(2n) with respect to Sl(2)ppm, is given by the table of exponents [10] for these algebras 0(2n)^D 2 „_3©Z) 2(1 _ 5 ©-©D 1 ©Z)„. 1 ,
(4.16)
Sp(2n)^Z) 2 ._ 1 ©D 2lI _3©-©D 1 .
(4.17)
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The (2n) fundamental representation of Sp(2w) is irreducible under Sl(2)ppal: an indirect proof stands in the property of the Sp(2n) adjoint representation to contain Dln _, (see the exponent table [10] for example). Such a representation can only come from the product DH-i x D ll _ i . However, the (2n) of 0(2n) cannot be irreducible with respect to Sl(2)ppal: in such a case the OSp(2n|2«) fermionic generators coming from (2n) x (2n)=DH_i x D , ^ would belong to Dj representations with; integer, and it would be impossible to reduce the OSp(2n|2n) superalgebra into OSp(l|2) representations. But one needs the 0(2n) fundamental representation to contain D„~i in order to get D. by the product D„^i xD,..-»Di: this Di is necessary to reconstruct OSp(l|2) corre sponding to (Di.Dj in OSp(2n|2n). Therefore for 0(2n) we have the Sl(2)ppil decomposition (2n)=Z)„_ ,©/)<,.
(4.18)
It follows that the fermions in OSp(2n|2n) will belong to (D,,_1©D0)xD1,_i = D 2 l l _ } ©D 2 l l _|©-eD i eD 1 ,_ i ,
(4.19)
and we finally get OSp(2n|2/i)/OSp(l |2)ppil = R(2n -1) © R(2n - f) © R(2n - 3) © • ...®K(2(n-p)-l)©K(2(n-p)-|)©K(2(n-p-l)-l)©-. •••©K(i)©K(l)©J?(n-2-). (4.20) The OSp(2n|2n) fermionic Dynkin diagram is
®
with 2n grey dots and '»m„=i[2(2n-2) + 2] = 2 n - l indeed corresponding to the highest R(q) representation.
(4.21)
4.2.5. OSp(2n 4- 2|2n) case (n ^ 1). The reasoning is the same as for the OSp(2n|2n) case, and the result is OSp(2n + 2|2n)/OSp(l|2)pp.1 = R(2n-i)ffiR(2n-l)©R(2n-i)©•••©R(2(n-p)-i)©/?(2(n-p)-l)©K(2(n-p-l)-l)©-" •••©/*(§)© R(l)®R(n). (4.22) We find again that ^m„=K3 + 2(2n-2)] = 2 n - i (4.23) in accordance with the value of q in the above decomposition. The OSp(2n+2|2n) fermionic Dynkin diagram is
®
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4.2.6. D{2,1; a) case (a 4= 0, — 1). We get the same decomposition as for OSp(4|2), that is D(2, 1; a)/OSp(l |2)pp., = 2R(1) 0 R®.
(4.24)
The Dynking diagram is now
1+a
with *-.=!
(4-25)
as expected. It would be of some interest to study the consequence of the a parameter on the corresponding super- W algebra. 5. The Spin Content of Super-If Algebras We start by constructing the stress energy tensor of a super-Toda theory. Then, it is straightforward to deduce the conformal spin of a If generator from the results of Sect. 4. It appears that the orthosympletic algebras are well-adapted to produce a generalization of the N = \ super-Virasoro algebra, while the N = 2 superconformal algebra always shows up in the Sl(n + l|n) theories. In this last case, we introduce the Sl(2|l) ppil superalgebra, containing OSp(l |2)pp„„ and better adapted to describe the group theoretical situation. 5.1. Stress Energy Tensor for Super-WZW and Toda Theories In order to determine the superconformal spin of the W-generators, we have to construct the stress energy tensor of the theory. Let us first define1: J%Y)= <J(X), T"> with X=(x; n),
(5.1)
T* being any generator of the Lie superalgebra s4 under consideration. We also note r\ab=
(5.2)
the scalar product already defined in (2.2, 2.3) with ***».=#
(5-3)
and the grading [ a ] = 0 (respectively [a] = l) if V is a commuting (respectively anticommuting) generator. Then J(X)=J.r={-\pJ°Ta 1
, where Jb=J'r,ab
From now on, we drop the Lorentz indices and write (x, tf) instead of (x
(5.4) , IJ )
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417
and, for example <J(X),J{X)) = Jar,'*Jb.
(5.5)
Do not forget at this point that J{X) is a fermionic superfield, which implies Ja(X) to have the grading fl>] +1). Then we can set {J'{X), J»(y)}p.B. = « ( - l ) l a > < 1 + ' k " ( / c " 6 ^ - Y)J%Y) + Kr,abDxd(X- Y)), (5.6) the //* being the structure constants and K the parameter of the central extension of the Kac-Moody superalgebra s/. We point out that in the T"s basis, the constants fahc=ffbtjic are completely graded-antisymmetric, i.e. fcbc_
_t_\lai[b]fbac=
_ t _ \[Jr] [c] facb
(5 7)
The super Dirac distribution is defined as S(X-Y) = d(x-y)-(ri-d)
if X = (x,ri) and
Y=(y,6)
(5.8)
which implies in particular S{X-Y)=-d(Y-X)and {J'(X), J»(y)}p.B. = - ( - D(1 + M m +m{AY),
J"(X)}r_B,.
(5.9)
After these preliminary measures, we can construct the super stress energy tensor. As in the non-supersymmetric case, it will be obtained by adding to the WZW part a correction term such that the current components constrained to be constant, have a vanishing superconformal spin. The WZW stress energy tensor reads ±-2V(X)J(X)J(X)>-J *-wzwW = - TZz < W J(X)J(X)> - ^ <J(X), DJ(X)} K
(5.10)
with {LwZW(X), r ( y ) } P B . = WAX
- Y)J°(Y)
-5(X-Y)dyJ'(Y)-^DxS{X-
Y)DJ°(Y)),
(5.11)
and finally we get Z™.(X) = Lwzy/(X) - iD\H, J(X)>,
(5.12)
2
remembering D = id and H given by (3.18). Owing to the CR {H(X),E„(Y)}P.B=ihS(Xwhere he\Z\{0}
Y)Eh(Y),
(5.13)
(cf. (3.17)), we get:
{Lr^iX), £,(y)} P . B . = i((i+htfJiX - Y)EJ[Y) -S{X-Y)dyEh(Y)-^Dxd{X-
Y)E„(Y))).
(5.14)
One may remark that the Cartan components of the current are not primary fields in a Toda theory, while the other generators are. Since there is no Cartan generator showing up in J' given by (3.34), one concludes that the Whi are primary super fields with superconformal spin (/zf + \), that is Whi contains one component with conformal spin (/zf+^), and one component with spin (/»,• + !).
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5.2. Orthosymplectic Superalgebras and the N=\ Case: We recall that to each R(q) representation of OSp(l|2) appearing in the above decomposition is associated a W generator with superconformal spin (q+$), the two component fields being therefore of spin (q+$\ {q +1). Let us first consider the spin content of the orthosymplectic algebras. We have: OSp(2M-l|2n):(i2)+(2,|)+(i3)+...+(2n-2,2n-f)+(2«-i2n) OSp(2n|2n):(i 2)+... +(2n-2,2n-\)+{2n-{, 2n)+(n, n+i) OSp(2n+l|2n):(i 2)+...+(2n-2,2n-f)+(2n-i 2n)+(2n, 2n+i) OSp(2n+2|2«):(i2)+...+(2n-i2M)+(2n,2n+|)+(n+in + l) D(2,l;a) a *0,-l:2(£2)+(2j). (5.15) One remarks that the conformal spin content of OSp(2n +1 |2n) is obtained by adding the spin multiplet (2n,2n+^) to the spin content of OSp(2n-l|2n). Similarly one goes from OSp(2n + l|2n) to OSp(2(n+ l)-l|2(n+1)) by adjunction of the conformal spin multiplet (2n+§, 2n + 2). These features of course reflect the embeddings OSp(2n-l|2n)cOSp(2n+l|2n)cOSp(2n + l|2n + 2). In the same way, one has to add the spin multiplet (n,n+\) to the OSp(2n —l|2n) spin multiplets to get the set of OSp(2n|2n) spin multiplets, and the multiplet (n+i, n+1) to those of OSp(2n +1 |2n) to obtain the OSp(2n+2|2n) spin decompo sition. In these cases, the associated embeddings are OSp(2n— l|2«)cOSp(2n|2n) and OSp(2n+1 |2n) C OSp(2n+2|2n). As is well known the OSp(l |2) algebra has the correct spin content to build the JV = 1 Super Virasoro algebra [5,14]. Thus, all these orthosymplectic algebras which are permitted for Super-Toda theories furnish simple generalizations of the N = \ Super Virasoro algebra that is JV = 1 Super- Walgebras. We note in particular that there is, in any such a series, neither spin 1 nor spin ^ element. 5.3. Sl(n+l|n) Superalgebras and the N = 2 Case 5.3.1. Introducing the Sl(2| 1 )ppi, Superalgebra. For the Sl(«+11«) superalgebras, we have the following spin decomposition: Sl(n + l|n):(l,f)+(|,2) + ...+(n,n+i)+(n+in + l),
(5.16)
and one remarks that two spin multiplets, namely (n +1, n+%)+(n+\, n+2) have to be joined to the spin content of Sl(n +1 \ri) to obtain the Sl(n + 2\n +1) one. Indeed, considering the embedding Sl(n + l|n)cSl(n + 2|n+1), one has to add the two OSp(l|2) representations R(n+\)+R(n + \) to the adjoint representation of Sl(n -I-1 \n) to get that of Sl(n + 2\n +1). Actually, these two OSp(l |2) representations constitute an irreducible one under a special Sl(2|l) subalgebra of Sl(n + 2|n +1) which we will call Sl(2|1)ppa,. Let us define more precisely this algebra. Starting from the fermionic Dynkin diagram of Sl(n +1 \n) - see Sect. 4.2.1 - we set
F_.= I
F + . = ( I £,,_„.,, F t , = I £ I r M
(5.17)
i K^E.tJ^l+tj,
(5.18)
F_,= I
i K^-^E.tj+tj
211
W Algebras and Superspace WZW Models
with Kl'=(K-\
419
and:
I" ' 1 0- 1- 1 0 1 1 0
K=
(5.19) 0 1 1 0,
It is now a simple exercise to verify that the algebra generated from F±at, F±f constitutes an Sl(2|l) algebra. Indeed {F±a,F±a} =
{F±„F±ll}=0,
(5.20)
{F±„F±,}=E±,
(5.21)
{F+n>F-<,} = H++H->
(5.22)
mthH±J- I I (K™H2)±K™-»H1}_X), £i=ij=i
{F + ,,F_,} = H + - t f _ , \.E±,F?J=+F±ll,\_E±,FTI,-]
(5.23)
(5.24) = TF±a,
[ £ ± ) F ± J = [£ ±> F ±/ ,] = 0 )
(5.25) (5.26)
and [tf ± ,FJ=+iF. ) [H ± > F / ,]=±F„ [ H ± , F . J = +iF_.,[H ± ,F_ / ,]= - i F _ # > [H + ) £ ± ] = ± £ ± > [ H _ , E ± ] = 0 .
(5.27)
We call the subalgebra just defined Sl(2|l)ppal in Sl(n + l|n). One immediately notes that: Sl(2|l)ppil contains OSp(l|2)pp,, as a maximal subalgebra, with fermionic generators F±t = F±t + F±p
(5.28)
and bosonic generators E±, H+. More generally with respect to its Sl(2|l ),,„,,, the adjoint representation of Sl(n +1 \n) reduces to SKn + l l n V S p i ) , , , , . ^ ^ ) © ^ - ! ) © . . . © ^ ! ) ,
(5.29)
where we denote by A(m) - with m integer - the 8m-dimensional typical representation of Sl(2|l), the decomposition of which with respect to OSp(2|l) being: fi{m)=R{m)®R(m-±).
(5.30)
212
420
F. Delduc et al.
The superalgebra Sl(2|l) corresponds to the N = 2 Super-Virasoro case - or AT = 2 Ademollo et al. algebra - with spin (1, f, f, 2). As discussed in [15] the superalgebra Sl(3|2) does correspond to the super- W3 algebra with spins (1, \, f, 2,2,f,3) and it is reasonable from the study of their spin content, to consider, following [16], the superalgebras Sl(n +1 |n) as corresponding to a direct generalization of the N=2 superconformal algebra. The just above defined Sl(2|l)pp,i algebra with its particular position in S1(M + 1|H) appears, the N = 2 case, as the analogous of OSp(l|2)pp,, for the N = l case. In this context, one can wonder whether the second Cartan generator H_ in Sl(2| 1) could be associated to some grading, in the same way the generator H+, also in OSpfl^pp,,, defines the grading (see (3.23)) related to the conformal spin. Actually, by a direct calculation, one can prove that: [H_,£ ± ( < S ( _ e i 4 l ) ]=+i£ ± ( a ( _ I ( , l ) ,ie{l,2,...,«}, [f/_,£ ± ( t ( _ a i ) ]=±i£ ± ( J f _, l ) ,
(5.31) (5.32)
while for any bosonic root £ a in Sl(n + l|n): [tf_,£J=0.
(5.33)
It follows that for any fermionic generator Ey in Sl(n + l|l), [tf_,£,] = *(}>)£, with a(y)G{-U}.
(5.34)
To some extent, the H_ generator is related to the t/(l) Kac-Moody generator or spin 1 generator - appearing in the N=2 Super-Virasoro algebra. Let us mention that our results for the spin content of Walgebras associated to super-Toda theories, agree with the tableaux given in [4] and guessed from spin values of low dimensional super- W algebras. Finally, let us remark that the existence of only one spin one in the Sl(n +1 \n) decomposition - and no spin one in the orthosytnplectic cases - forbids the possibility to obtain super-Virasoro algebras with TV > 2 in this approach. For the super-Toda model based on Sl(n +1\n), the N — 1 superconformal tensor given in (5.14) is improved with the superspin 1 operator Wt that contains the second supersymmetry generator together with the 1/(1) Kac-Moody generator. The construction of the W, operator goes as follows: 5.3.2. The Super-Wl Generator. Since the W, operator is the lowest spin generator, it is easy to obtain it from the general method of Sect. 3.3. We first execute on J a gauge transformation (3.12) based on negative simple roots g-i = exp/ I WE_X
(5.35)
so that the coefficients of all the Cartan generators in Ad*(g_4) (J) are set to zero. Then, a second gauge transformation g_,=exp(
V Q*E\
(5.36)
is used to cancel all the coefficients of the (negative) simple roots generators, except the one associated to a lowest weight of OSp(l |2)ppill, and which is exactly Wi. In order to give a compact form for W,, we first define a linear transformation T which
213
W Algebras and Superspace WZW Models
421
acts on a general element of Sl(« +1 \ri), 4>2 +
M=
(5.37)
as
0.
-X
T(M)=
(5.38)
~9n
(5.39)
Str(T(M)r(W)) = - Str(MN), [T(M), X(N)} - T([T(M), N}) - t([Af, T(N)}) + [Af, N} = 0.
(5.40) (5.41)
T makes explicit the role played by Sl(2|l)pp,i in the N = 2 case: actually, the smallest Lie algebra containing T(OSD(1 |2)ppil) is just Sl(2|l)ppill, the action oft on the generator of this superalgebra being given by (the notations are the same as in Sect. 5.3.1) WJ=-Fm,
t(F_J=F_ a , x{H + ) = H_,
z(Ff) = Ffi,
T(F_,)=-F_„
z(H_) = H+.
(5.42) (5.43)
In fact, the transformation ix is a complex structure [17] on the compact supergroup generated by Sl(n + l|n), and it is not surprising that it appears in the expression of Wu Wl={ Str(Jt(J)) - i Str(H _ DJ).
(5.44)
6. Examples Let us apply the general properties discussed above on the two simplest and basic examples. We recall that for the Sl(n +1 \n) series, the super-trace operator is proportional to < , >
214
422
F. Delduc et al.
6.1. Study of OSp(l\2) OSp(l 12) is generated by two fermions F ± and a bosonic SI(2) (H, £+,£_). Its commutation relation reads3 IH,E±]=±E±,
[JJ,F ± ] = + ± F ± )
[E + ,F_] = F + , [£ + ,£_] = 2H, {F + ,F + } = i £ + )
[£_,F + ] = F_, {F + ,F_}=-±H,
(6.1)
{F_,F_}=-±F_.
Using the 3-dimensional representation
li
0
\
A) I A
i / = 0 - i 0 , £+= 0 0 0 , \0 0 0/ \0 0 0/
£_=|1
0 0|,
(6.2)
1° ° *\ F+= 0 \0 One gets for the constraints One gets for the constraints
0 0 , F_= | J 0/ current J, current J,
0 0 i|.
l
(6.3)
(6.4)
W /* o *, y being fermionic and U a bosonic superfield and a constraint (J,F-} = 2 / i = C . An element of the residual gauge group then takes the form
r " °\
G=exp(AE_+2QF.)=
\ A 1 Q\ \-fi 0 1/ A (respectively Q) being bosonic (respectively fermionic) G acts on J as: A (respectively ft) being bosonic (respectively fermionic) G acts on J as:
(6.5)
Ad{A, Q) (J) = GJG -l+(DG)G~l
(6.7)
A0=-(L/+-DA ^ V
V
)
Be careful of the change of normalisation J± = ±2F±, X± = ±E±
215
W Algebras and Supcrspace WZW Models
423
we get the invariant supercurrent
/o J' = Ad(A0,Q0)(J) = lw3l2 \0
o M 0
0
(6.8)
v. 0/
with ^ 3 / 2 = r+-^(<M>
+ A2-QlQ2,Q1
+ Q2),
(6.9)
Ad(A,Q)A0 = A0-A-QQ0,
(6.10)
Ad(A,Q)Q0=Q0-Q.
(6.11)
Finally, W3/2 can be identified with the super-Virasoro generator via the formula: W3/2= ^
Str \^JJJ+ i JDJ-HD2A
(6.12)
with the supertrace operator (Str) proportional to the scalar product <, >.
6.2. Case of Sl(2\ I) The fundamental representation of Sl(2|l) is 3-dimensional: (6.13)
(6.14)
(6.15)
(6.16) The constraints <J,F__>= -fix, <J,F_ + >=/x2, and <J,£_> = 0 lead to
216
424
F. Delduc et al.
The residual gauge elements G=exp(/4£_+flF_
+
/ I + r F _ . ) = U+±270 \
0 0\ 1 Z\
fl
0
(6.18)
1/
act on J as k&(A,Q,Z)(J) = Ir-EUi-QUi+U\
^ZQ)((Pl-H2Q)-(A
+
iZQ)(^2-^i^)
C/1 + 0 ( « 2 - | i 1 2 ) - | i 1 ( i 4 + i 2 : 0 ) 0 * 2 -Ai,2:
ft U a - ^ ^ - ^ O J + ^A-iZfl))
I
0
0
(5.19)
0
+ UM-±((Dr)fl + 27£>fi) 0 DZ \
Z>fi
0
0
with i4 (respectively G, Z) bosonic (respectively fermionic). 1 Again, for the special transformation A0 = UiiUi-HtUi 2niii2 Q0 = — # , amd Z0 = — $ 2
we
+
DQt-DQz),
obtain the invariant current
A*2
o , w
3!2
J0=Ad(A0,Q0,Z0)J=\
- ^ i
o
n2
o
U
0,
A«i
W\ »'
(6.20)
0
\A*2
with (2nlfi2Y-2ix2
^3,2 =
-2AI,#,1/2
2/^1^2
- ^ M a - ^ M j + ^DI/.-^Dl/j + D^*,-*,)) Wl=2^2
t /
l+^
t /
(6.21)
2 + *l*2 + ^ l + ^ 2 )
that is also
W3/2 = — - Str (J JJJ+ J
JDJ-H^J) (6.22)
217
425
W Algebras and Superspace WZW Models
where T is defined as (see Sect. 5.3.2): /#, t y
0 *2
\u1
i*i
fi2 \ / # , u2 = r *i+*2/
\i/,
0 -*2 MI
-n2 \ -i/2 .
(6.23)
*,-*2/
7. Conclusion Using an N = 1 superfield formalism we have shown that Super-Toda theories are constrained super-WZW models associated with superalgebras admitting a completely fermionic simple root system. Carrying a constrained super-WZW model leads to reduce the corresponding superalgebra with respect to its OSp(l 12) principal embedding. To each OSp(l 12)ppal representation showing up in this decomposition is attached a super- W generator belonging to the symmetry algebra of this super Toda theory, or super- W algebra. The Sl(n + 1 \n) series provides a family of N = 2 super- W algebras, whereas the other series lead to N = 1 super- W algebras. We remark that if the classification is governed by the OSp(l |2)ppil algebra in the orthosymplectic series, it better stands on a bigger subalgebra, that we have denoted Sl(21 l) pptl and which contains OSp(l 12)pp.„ in the Sl(n -t-11 n) case. As examples, we explicitly construct the N = 1 super-Virasoro algebra from the OSp(l 12) theory and the N = 2 Ademollo et al. algebra from the Sl(211) theory. Among the developments we can think of, let us first mention the N = 2 supersymmetric case, in which the algebra Sl(2|l)ppill has a role to play. New types of super- W algebras will also be provided by constructing non-Abelian [18] - or generalized [19] - super-Toda theories, then limiting the constraints to a subset of the original ones. Technically, the different OSp(l 12) embeddings in the superalgebra of the theory will have to be studied, each of them giving rise to a different super-W algebra: these OSp(l |2) embeddings replace the Sl(2) ones for a non-Abelian non-supersymmetric Toda theory [18, 19]. Finally, from a simple group theoretical point of view, our study deeply shows that the OSp(l 12) , embedding in a simple superalgebra plays a role analogous to the one of the Sl(2)ppa, in an algebra. Our results suggest that a general relation exists between the OSp(l 12)ppil subalgebra and the Casimir degrees of a superalgebra. Such a property would generalize the result of [20] for algebras. References 1. Balog, J., Feher, L., Forgacs, P., O'Raifeartaigh, L., Wipf, A.: Phys. Lett. B227, 214 (1989); Phys. Lett B244, 435 (1990); Ann. Phys. 203, 76 (1990) 2. Leites, D.A., Saveliev, M.V., Serganova, V.V.: In: Group theoretical methods in physics. Amsterdam: North-Holland 1985; preprint IHEP 85-81, Serpukhov 1985 3. Nohara, H., Mohri, K.: Nucl. Phys. B349, 253 (1991) 4. Komata, S., Mohri, K., Nohara, H.: Nucl. Phys. B359, 168 (1991) 5. Evans, J., Hollowood, T.: Nucl. Phys. B352, 723 (1991) 6. Inami, T., Izawa, K.I.: Phys. Lett. B255, 521 (1991) 7. Kac, V.: Adv. Math. 26, 8 (1977) 8. Van der Leur, J.W.: Contragredient Lie superalgebras of finite growth. Utrecht thesis (1985) 9. Frappat, L., Sciarrino, A., Sorba, P.: Commun. Math. Phys. 121, 457 (1989)
218
426 10. 11. 11 13. 14.
15. 16. 17. 18. 19. 20.
F. Delduc et al.
Drinfeld, V.G„ Sokolov, V.V.: J. Sov. Math. 30,1975 (1985) Leznov, A.N„ Savelie, M.V.: Sov. J. Theor. Math. Phys. 61,150 (1984) Scheunert, M„ Nahm, W., Rittenberg, V.: J. Math. Phys. 18,155 (1977) and references therein Berezin, F.A., Tolstoy, V.N.: Commun. Math. Phys. 78, 409 (1981) Arvis, J.F.: Nucl. Phys. B212, 151 (1983); B218, 309 (1983) Babelon, O.: Nucl. Phys. B2S8, 680 (1985) Babelon, O, Langouche, F.: Nucl. Phys. B290, 603 (1987) Leznov, A.N., Savelier, M.V., Leites, D.A.: Phys. Lett. B96, 97 (1980) Chaichian, M., Kulish, P.P.: Phys. Lett B78, 413 (1978) Liao, H.C., Mansfield, P.: NucL Phys. B344, 696 (1990) Romans, LJ.: Preprint USC-91/HEP 06 Lu, H„ Pope, C.N, Romans, LJ., Shen, X., Wang, X-J.: Phys. Lett B264, 91 (1991) Nemeschansky, D., Yankielowicz, S.: Preprint TAUP 1860-91, USC-91/005A Spindel, PIL, Sevrin, A., Troost, W., Van Proeyen, A.: Phys. Lett. B206, 71 (1988) Leznov, A.N., Saveliev, M.V.: Commun. Math. Phys. 89, 59 (1983) Saveliev, M.V.: Mod. Phys. Let 5A, 2223 (1990) and references therein O'Raifeartaigh, L„ Ruelle, P., Tsutsui, I., Wipf, A.: Preprint ETH-TH/9M, DIAS-STP-91-02 Kostant, B.: Adv. Math. 34,195 (1959)
Communicated by J. Frohlich
221
Reprinted with permission from Theor. Math. Phys. Vol. 65, pp. 1205-1213, December 1985 © 1986 Plenum Publishing Corporation
^ F I N I T E A D D I T I O N A L S Y M M E T R I E S IN T W O - D I M E N S I O N A L CONFORMAL QUANTUM F I E L D THEORY A.B.
Z aroolodchikov
Additional symmetries In two-dimensional conformal field theory generated by spin s = i , 1 3 currents are investigated. For spins s = 5/2 and 8 = 3. the generators of the symmetry form associative algebras with quadratic determining relations. "Minimal models" of conformal field theory with such additional symmetries are considered. 1.
Introduction
The group of conformal transformations of two-dimensional space (or space—time) is infinite dimensional. It consists of arbitrary analytic transformations t-W,
F-S(i)
(1.1)
af the complex coordinates 2—£'"HS\ z—fc'-fV. where l \ V are the coordinates of the two-dimensional space. The general properties of two-dimensional quantum field theory Invariant with respect to this group are described in (1): the present paper is written under the assumption that the reader is familiar with the quoted paper. We give here only some of the basic formulas. The independent components r-7\,-r„+2ir„; of the traceless energy—momentum tensor T makes it possible to write
T-T„-TU-2IT„
(1.2)
satisfy the Cauchy—Riemann equations !hT—d,T—0, and this T-T(z); T-T{z).
(1.3)
It can be seen from (1.1) that the conformal group can be regarded as the direct product l"(i)xriZ) of the groups of analytic substitutions of the variables z and z , respectively, the fields T ( z ) andT(z~) being associated with the generators of the subgroups r ( z ) and r ( z ) , respectively. In what follows, we shall frequently concentrate our attention only on the subgroup r ( z ) , understanding that the same applies to r
ft.4>
<Mi(«.z)X>-$
(1-5)
tre determined by ■
There the integral is around a small contour surrounding the point z. and X denotes any product of local fields of the form X-Ak{x„l,)...A„(t.,U). tt-8> ^>us. the transformation properties of any field A. are determined by the singular terms of the operator expansion of the product 7(C)^I(I, z). In quantum field theory, there exists a certain set of "primary" fields *i(z, 2), which are characterized by the operator expansions r(C)w1(«.i)--jr^w,(f,2) + r^-£w,(i.*) + 0(l),
r « ) « . ( i , Z ) - - j j r ^ w , ( z , ? ) + - ^ i w 1 ( « , z ) + 0 ( l ) . tt.T)
L. D. Landau Institute of Theoretical Physics. USSR Academy of Sciences. Translated from Teoretlcheskaya I Matematlcheskaya Flzlka. Vol.65. No.3, pp.347-359, December. 1985. Original article •ubmitted November 19. 1984.
1205
222
where A, and 2 , are numerical parameters that characterize the given primary field *, and are called dimensions. In reality, the combinations «,-A,-A, and <4—Ai+i, are the spin and scale dimension of the field ♦,, respectively. For local flelds *,, the spin s , can take only integer Sor Bose flelds) or halfinteger (for Fermi fields) values. The operator expansion for the fields T ( z ) themselves has the general form e
2TW)
T'(t')
where the prime on T denotes the derivative, and c Is a numerical constant, regarded as a parameter of the theory (11. The field T ( z ) also satisfies a condition of regularity at infinity: T(i)~l/i'
as
«"►«.
(1.9)
In accordance with (1.5), it Is helpful to introduce the operators L a ( z ) , which act on the local fields A . ( z . z ) and are defined by L.(z)A,(i,i)-f iUt-i)-"T(t)A,(i,z). It follows directly from (1.8) that these operators form the V i r a s o r o
(1.10)
algebra
IU, Z. ] - ( n - m ) t . . . + •^•(n'-iOe......
Q.ll)
Here and in what follows, we omit the argument z of the operators L g . By analogy with (1.10), one can define operators t , . the operators t > and L m commuting. The primary fields ♦, satisfy the equations L.€,-L.Q,-0
for n>0, £.4>,-A,»„
£,Vi-&,w<.
All local fields occurring in the theory can be obtained by applying the operators L a with n < 0 to the primary fields *, (in particular, L_,
a^."'(i)-0,
where w(z) is an arbitrary analytic function; these currents can be regarded as the generators of the additional symmetry. An example of such a situation — conformally invariant field theory symmetric with respect to the current algebra — Is considered in [S] as a conformally invariant solution of the two-dimen sional Wess-Zumlno model. In this example, s - 1 and the (matrix) field Q, Is related to the generators of the Kats-Moody algebra. Another example i s provided by superconformal symmetry 14-6] with s = 3 / 2 . when the field Q y is a ■supereurrent." It is of interest to Investigate the possibility of additional Infinite symmetries in field theory that correspond to different spins s of the generators Q t . The main requirement imposed on the field theory is associativity of the operator algebra [1]. The complexity of the analysis of the associativity condition Increases rapidly with increasing spin s, so that in this paper we restrict ourselves to cases s £ 3. Section 2 gives a general formulation of the model. Specific examples of theories possessing con served currents with spins s = J. 1 3 are considered in Sec.3, where it i s shown that the cases of spins s s 2 do not lead to essentially new algebras: s ■ J corresponds to free fermlons, 6 = 1 leads in the general case to the Kats-Moody algebra, s = 3/2 corresponds to supersymmetry, and s « 2 reduces to direct products of Virasoro algebras. We also investigate here currents of spins 5/2 and 3 and show that the generators Q t do not form Lie algebras but more general algebras with quadratic deter mining relations. In Sec.4, we discuss the connection between infinite additional symmetries and "minimal
1208
223
conforms! theories." 2.
F o r m u l a t i o n of the
Model
We consider two-dimensional conforms! field theory in which there exists a conserved current Qs(z> of spin s . In the general case, the field Q, can have several components; In this case, we shall write Q.\ n - l , 2 0. The current Qs is a primary field (see the Introduction), i . e . ,
nt).u)-—iL-7.(2)-i--5-.'w+0(i).
o.i)
(C-z)C-z This relation in conjunction with (1.8) enables us, of course, the express any correlation function of the form mt,)...T&,)Q.lz,)...Q.[i„)> (2.2) in terms of the correlation function «?.(.-,) ....(:„)>.
(2.3)
Indeed, on the complete complex plane the function (2.2) is a single-valued analytic function of, say, the variable t, having poles at the points J: ?.< and z , ;.„. The residues at these poles are completely specified by formulas (1.8) and (2.1). Therefore. taking into account (1.9). we can write down the relation
r, W 0 .(,,...(,.(,.,> + {£[^ + ^ A ] ^ f - ^ + ^
(2.4)
which expresses the (N + M(-point function (2.2) In terms of the (N - 2 + M ) - and (N - 1 + M)point functions. Applying (2.4) recursively, we can express (2.2) in terms of (2.3). We can show that the result does not depend on the order in which (2.4) is applied (In the sense of the choice of £ or another variable Ct), i . e . . the expansions (1.8) and (2.1) are consistent with the condition of associativity of the operator algebra. To have the possibility of completely calculating the correlation functions (2.2), It Is necessary to specify the singular terms in the operator expansion
g.UXMO-H °:1':.yl. + 0(l).
(2.5)
Here, R a (z) are certain local fields of dimension and spin a, and aa are numerical coefficients. The field Rg has zero dimension; we shall always assume that R Is the Identity operator I. In addition, we must bear in mind the condition of regularity of the field Q s (z) at infinity: Q.{z)~z---,
: - » .
(2.6)
The expansion (2.5) makes it possible to write, by analogy with (2.4),
...(z„)> - Y \ i - ^
+
-rzirr4rVT^''>-T^--^-^)x
9.U-,)fl.(z,),(«w,)...?.(z«)>.
(2.7)
The sign factor (-1)"' In the second term on the right-hand side Is introduced because Q, is a Fermi field for half-integer spins. Equation (2.7) will be a nontrivlal recursion relation that makes It possible, like (2.4), to lower the order of the correlation functions if all the fields R in (2.5) are representatives of conforms! families
1207
224
of the Identity operator [IJ and, perhaps, the field [Q # l Itself. Using the symbolic notation of [11, we can write Q.Q.-all)+b[Q.]+0(l). (2.8) Here, a and b are numerical coefficients (structure constants) In the expansion (2.6) In front of the primary fields I and Q t themselves; the coefficients In front of the corresponding secondary fields are completely determined by the requirement of conformal lnvariance [11. We emphasize that the regular terms omitted In (2.8) can, generally speaking, contain representatives of other conformal families. It Is obvious that the coefficient b Is equal to zero If Q ( Is a Fermi field. The value of the coefficient a is a question of the normalization of the field Q f ; In what follows, we shall always choose a ' c / s . Toe anaatz (2.8) determines the model of additional symmetry considered In this paper. This model is not the most general; for example, one can consider cases when there are several conserved currents of different spins. In addition, we shall, as a rule, restrict ourselves to the case of a single-componeot field Qs. As we pointed out. if (2.8) is valid the relations (2.4) and (2.7) make it possible to lower the order and. thus, calculate explicitly the correlation functions (2.2). Moreover, the result must not depend on the order in which these relations are applied. This fundamental condition, which Is tantamount to the require ment of associativity of the operator algebra a . 8 ) . (2.1). (2.5), Imposes, if it can be satisfied at all, restrictions on the parameters a. b. and c in (1.8) and (2.8). In (2.8). the square brackets denote the contribution of all representatives of the corresponding conformal families: [ / ] - i - - ( 1 + ^ " L - , + Z , ^ " L . , + x>ti','l.-,,+z%'"L-. + . . . ) / , 'L-.+x1?.., /.-,■+*■?, L-> + .. .)(>..
lQ.)-x-'{i+xl!
where x * z — »', and the quantities j9 are the standard coefficients of the conformal chain; the corre sponding definition and method of calculation can be found In [ll (see also 17]). Essentially, these coefficients can be determined In different ways by applying the relations (2.4) and (2.7) to calculate the correlation functions (2.2) with M = 2 and M > 3. We give the result for the first few coefficients:
where t-(5i+l)/(22+5c), (2.11) 3 and the field A(z) Is determined by the relation T ( z ) T U ' ) * singular terms of (1.8)+ — *""(»') + A(i') + O(i-z). Now, to guarantee associativity of the complete operator algebra d. 8). <2.1). (2.10). it is necessary, choosing the parameters c and b appropriately, to obtain crossing symmetry of the four-point function (2.3) with M = 4 (this assertion is essentially proved in [ID. In the following section, we consider several examples of associative operator algebras of the indicated form. 3.
C o n s e r v e d C u r r e n t s of Spin
s £ 3
We here consider possible additional symmetries generated by the currents Qs with s-7:, 1 7„ 3. A. Spin j . We denote Q.:.(i)~\2e^(z).
Then the operator expansion (2.10) has the form
♦ ( ! ) ♦ ( » ' ) - ^ 7 + 0(1).
G- 1 '
Calculating the correlation functions <$(>,)...$(2*)) by means of (3.1), we can readily verify that *(z) Is a free Fermi field. Obviously, the introduction of a multicomponent field ♦*('), o - l , 2 , . . . , D , does not change the situation. B. Spin 1. We consider Immediately the case of a multicomponent field Q denoting Q:('-)~ (c/*r)V(i), a—1 D, where k Is a new constant. Obviously, the expansion (2,10) has in this case the 1208
225
general form /*W/(0-;
+'•
\
+0(1)
(3_2)
there /." are numerical coefficients. Since J" are Bose fields, the condition of symmetry of (3.2) under die substitution : ~ t ' . a — b means that /.•*—/V*. Considering the three-point function
(3.3)
i.e.. if t" are the structure constants of a D-dlmensional Lie algebra. Thus, the operator algebra with H.8). (2.1). and (3.2) with 3 - 1 is related in the general case to a semldlrect product of the Kats-Moody ilgebra and the Vlrasoro algebra (see [3D. C. Spin 3/2. We denote Q,,{z)—S(z). The general form of the expansion (2.10) In this case is 2C .„ + - j f ^ - + 0(l). (3.4) 3(z-z )• (z-z ) It can be shown that the condttioti"oT crossing symmetry of the four-point function (S(z ) . . .S(z )> does not impose any restrictions on the value of the parameter c . It is easy to show that the fields T ( z ) and S(z) in this model generate the superconformal group [4-6], the field S(z) being a supercurrent. By analogy with (1.10). we introduce the operators
S(z)S(z')-
S«-4,(i.f)-.$dt(C-«)'* , *S(SM.(i.i),
(S.5)
where * - ± 7 . , ±'l It follows from (1.8). (2.1). and (3.4) that these operators form, together with Lm, the Neveu—Schwarz algebra
[L.,S,l-(7,/i-*)S«„
{5.,S,}-2i,., + i - ( * , - 4 - ) « . . 1 . . 3
x
(3.6)
4 '
where the curly brackets denote the anticommutator. Thus, for s * 3/2 our model reduces to supercon formal field theory. It is interesting to study the case of a multicomponent spin 3/2 field: S'(z), 1 - 1,2 N. It ii also natural to Introduce currents J"(z) of spin 1 generating linear transformations of the fields S':
$<%<> ( 5 ) / - O S ' ( i ) - » ( « ) ««•«'(«).
0.1)
«nd forming the Kats—Moody algebra (3.2). Here, t" are matrices of a representation of a certain Lie ilgebra: [f, !')-/,•*(•. For N < 4, this model evidently leads to extended supersymmetrles. If N > 4. u algebra with quadratic determining relations Is obtained. The investigation of this model, which in our view Is very Interesting, goes beyond the scope of the present paper. P. Spin 2. Considering directly the case of a multicomponent field Q,, we Introduce the notation Qj'(z) » T'(z). I =■ 1 , 2 N; we shall also denote T(z) - T°(z). Then the operator expansions a . 8 ) , '2.1). and (2.10) will have the general form _ _ ! l ^ + ^ m + * L 3 ! ^ + 0(1)f ,3.8) 2(z-z')' (z-z)' z-z' •here 1, J. k » 0 . 1 N, and c*> and i]i are numerical coefficients, symmetric functions of 1 and i by virtue of the requirement of symmetry of the left-hand side of (3.8). If the matrix cM is assumed to k nondegenerate, we can without loss of generality write cl> « c«'>. The requirement of crossing •ymmetry of the three -point,
d." -dm-d„k-d,„;
d.u*d?-d,,u
0.9)
*hich mean that d'{ are the structure functions of a (N + 1 )-dlmensk>aal associative commutative algebra *Uh generators A and with determining relations A^A,-d^A.. It is easy to show that If (3.9) Is satisfied ">e tensor &ijt can be reduced by an afflne transformation of the fields T' to the form 1209
226
*•-««*..
<8.10)
Thus, the algebra (3.8) reduces to the direct product of N ♦ 1 copies of the algebra Q.8), i . e . , of the Vlrasoro algebra. It is interesting to consider the case when in addition to the fields T< there are cooserved currents J« of spin 1, but this would also go beyond the scope of the present paper. We see that for cases s s 2 the ansatz (2.8) does not lead to essentially new algebras. situation is changed If we consider higher spin values.
The
E. Spin 5/2. We now turn to the case of a conserved current 0v,(i) — U(t) of spin 5/2. The operator expansion (2.10) (In which the coefficient b is equal to zero because U ( z ) is a Fermi field) makes It possible In this case to write down the following relation for the correlation functions: - X | - ^ Z ^ r < t / ( j , ) . . . U ( j , - , ) £ / ( ! , . , ) . . . £ / ( ! , ) > + ~
O(J,-I,)'
jr
X l ( - » ' [l (»>-*<) . 2 „+T^7-7T " (»,-»<)
+
di,
i TZZ'. 1 10 I , - I , it,'
m Y,-^^-W(t,)...U(t,-,)Mt,)U(i,.,).. ,_■
-tf (i„)>.
(S.ll)
*•-*•
Since the correlation functions of the right-hand side of (3.11) can be expressed In terms of the (N - 2 ) point correlation function by means of (2.4) and (2.11), this relation makes it possible to calculate recursively all correlation functions of the fields V(t). For the four-point function, the result has the form
(3.12)
where
x denotes the anharmonic ratio
(».-«.) («.-«.) («,-!.) (!,-»,) '
(3.14)
and S r
81
101 + -2(22+5c)rl*—rJl
(3.15)
The requirement of crossing symmetry of the four-point function (3.12) is expressed by the equations C.(i)-C.(l-i),
(3.16a)
G.(l/x)-i"G.(*).
(3.16b)
It is readily seen that (3.13) satisfies (3.16b) only If X - 3, whence c
"/...
(3.17)
Thus for s • 5/2 the condition of associativity of the operator algebra (1.8), (2.1), and (2.10) uniquely fixes the values of all the parameters. As in the case of (1.10) and (3.5). we Introduce the operators U* *—±7„ ±'/i,... in accordance with t W , ( « . i ) - # « < ; - ! ) ' ♦ » i/ttM.U.i).
(3.18)
It follows from the operator expansions (2.1) and (2.10) that these operators in conjunction with L a form an algebra with the determining relations (1.11) and lL.,Ui]-('Un-k)U..,; is 19)
^,1,-^A..,+[^+2)(^+3,-(*4)(-4)]^-^(*-f)(*'-4)« 1210
'
227
where the operators A, are quadratic in L: A.-
£
:i»i.-.:.
(3.20)
Here, the symbol : : denotes normal ordering (the operators L with higher index are placed to the right), and d,.-'l,(l-nf),
d,..,-7.(l+m)(2-m).
(3.21)
F. Spin 3. We consider the case s » 3; Qj(») = V(x). In this case, the coefficient b In (2.8) is also equal to zero, since the term (i-z')-'V(z') In 12.10) would contradict symmetry of the left-hand side of (2.10) under the substitution t *+ i'. Therefore, the expansion (2.10) can be written In the form
! ^ r " ( ' ' , + 2^ A ' (l '>] + 0(1)-
(8 22)
-
As in the case of (3.11). taking into account (3.22), we can write down a recursion relation that enables us, by lowering their order, to calculate the correlation functions (2.3). Such calculations lead to the following result for the four-point function: ( V f j . j i ' w v e . ) >'('.)>-<».-*.)-•<«.-«.)-'<;.(*). (3.23)
2
2
2 1
where x is the anharmonlc ratio (3.14), and n - -
f 1 . 9
1
. , 2 , 2
1
32 16 5 (22+5c) '
It can be directly verified mat the expression (3.23) satisfies the crossing symmetry conditions (3.16) for all values of \i. i . e . . the condition of associativity of the operator algebra (1.8), (2.1), and (3.22) does not impose any restrictions on the values of the parameter c. Introducing the operators Va (n - 0, ±1. . . . ) In accordance with V.A,(,,i)-
fdt(Z-l)"'V(i)A,(t.i),
we can obtain the following commutation relations between V and L: [L., Vm)-{2n-m)V.,.,
(V., V . ) - - j ^ ( » - m ) A . , . + ( n - m ) [-L(n+>n+2) (n+m+3)- i ( » + 2 ) («+2) ] t . . . + ^ - ( - i , - 4 ) ( « ' - l ) n o . „ . ^ 0
(3.24)
Mil
where the operators A, are determined by (3.20) and (3.21). Equations Q..11) and (3.24) are the determining relations for the algebra of the additional symmetry generated by the spin 3 current. Thus, In the cases of spins 5/2 and 3 the generators of the additional symmetries form, together with the confbrmal generators, associative operator algebras with the quadratic determining relations (3.19) and (3.24). We note that algebras with quadratic determining relations (containing, in contrast to the ones described here, a spectral parameter) play a fundamental part in the qnantum inverse Mattering method (see, for example, (81). An Interesting example of a finitely generated quadratic algebra has been studied by Sklyanln [9]. 4.
Discussion
The space of local fields occurring In a conformal field theory with additional symmetry corresponds to a certain (In general, reducible) representation of the corresponding algebra of the symmetry. If, as 1211
228
usual, one requires that the spectrum of dimension* be bounded below, men simple dimensional analysis (see [1. 3J) shows mat every irreducible representation is a representation of highest weight. For example, for the case of a "symmetry of spin 5/2" 8 . e . , for the algebra (3.19)) this means that the field theory contains "invariant fields* \ satisfying the equations L.9A-0,
C/«a>.-0 for
n,*>0,
Z-.O.-AiK,
(4.1)
where the operators U, are determined by (3.18), and A is the dimension of the field * a . All the remaining local fields of the theory are obtained by applying the operators U.,, £_. with k, n > 0 to the Invariant fields *A (we recall that here we ignore the dependence of the fields on the variable z and do not consider the operators E . , Vk). The subspace of fields of the form L...L
L-„U.k,...
£/-„,«>.,
(4.2)
where all the n and k are positive, correspond to the representation of highest weight of the algebra (3.19). For the case of the "spin 3 symmetry" with the algebra (3.24), the Invariant fields 4V* are characterized not only by the dimension A but also by the parameter v and satisfy the equations L.4>i..-V.9t,,-0
for
n>0,
£,®»..-A®» ,;
V,®»,,—»©4.,.
The space of the representation of highest weight oonsists in this case of fields of the form £V-„w.. r
(4.3) i-.,V_.,..
In quantum field theory, the set of invariant fields and values of the parameters (A for symmetry of the spin 5/2 and A and v for spin 3) must be chosen in such a way as to satisfy the requirements of local fields and associativity of the complete operator algebra. We intend to discuss in detail the properties of conformal field theory possessing the additional symmetries s - 5/2 and s = 3 In a further paper. Here, we merely mention that there exist cases of strong degeneracy of the representations (4.2) and (4.3), when these representations decay Into a f i n i t e number of conformal families (I.e., a finite number of Irreducible representations of the Virasoro algebra). At the same time, the corresponding conformal field theories are related to certain "minimal models' Introduced In [1]. We consider first the algebra (3.19) of spin 5/2. We note first of all that the negative value (3.17) of the parameter o, dictated by the requirement of associativity, to a large degree renders this model of additional symmetry useless as a model of quantum field theory; It Is readily seen that when c < 0 the requirement of posltlvlty In field theory cannot be satisfied [10). At the same time. Interest attaches to solutions of the conformal bootstrap equations that do not satisfy the posltlvlty oondltlon; such solutions can describe phase transitions in two-dimensional statistical systems with non-Glbbs averaging (for example, random walk without self-Intersection, systems with random Interaction). For c = - 1 3 / 1 4 there exists the "minimal model" p/q = 4/7 (see [1]). The spectrum of the dimensions of the primary fields In this model is described by A,.,.,-
(7W
~^'"9.
-1.2:
—1.2.....6.
Note that the field *,,,., has the dimension A,,..,-'/>. The fusion rule for this field, calculated in accordance with the standard rules [1], has the form * , , . , * , , . , - [ / ] . Therefore, this field can be identified with the .generator of an additional symmetry of spin Vi:
(U-i-'/,L-,V-h)Q.„-0.
«.«M
The primary fields 4 (1 .., and t>,,.., (which have dimensions A,,..,—7i.—V.+'/i and A(1,i,—Vn+*/«) can be identified with the states ♦,!..,—U-%9;„ fn..,-"-<.*-'/- (we have taken into account (4.4a)). Thus, In the considered minimal model there exists a subalgebra containing the primary fields if,,. „„ m-1.2. ..G, which possess the additional symmetry (3.19).* "With regard to the fields *,, . , in this minimal model, they cannot be local with respect to the field U(z). The corresponding representations of the additional symmetry are evidently analogous to the representations of the Ramond algebra in superconformal theories 15]. Here, we consider only "local" realizations of the symmetry. 1212
229
For the algebra (3.24) corresponding to the spin 3, the value of the parameter c la not fixed. We consider however the special case c = 4/5. For this value of c, there exists a minimal model p/q = 5/6 *ith spectrum of dimensions A,.,.,-
(5
"-6"»'-t, 120
„_!.;!, 3 .
m_lt2,3.4.
As follows from the analysis made in [10], this model satisfies the positlvlty condition. It apparently des cribes the critical theory of the three-position Potts model [11]. The Held ifci.« has dimension A,,,i>—3 and can be Identified with a conserved current Viz) of spin 3. The primary fields *,,.., with n - 1 , 2 , 3 , 4 and ♦(■ .i with n = 1.2 in this model generate a subalgebra In which the symmetry (3.24) Is realized locally. We believe It would be Interesting to study the cases of degeneracy of the representations of the algebra (3.24) and the corresponding conformal field theories for arbitrary values of c, especially In the very Interesting region c > 1. LITERATURE 1. 2. 3. 4. 5. 6. 7. 8. 9. 10. 11.
CITED
A. A. Belavtn. A. M. Polyakov. and A. B. Zamolodchlkov, Nucl. Phys. B, 241, 333 0964). B. L. Feigin and D. B. Fuke. Funktslonal. Anallz I Ego Prllozhen.. IS, 47 (1982). V. G. Knlzhnlk and A. B. Zamolodchlkov, Nucl. Phys. B, 247, 83 (1984). M. Bershatskl. V. Knlznlk, and M. Teitelman. Phys. Lett. B, 147. 217 (1985). O. Fiiedan. Z. Qlu. and S. Shenker. Phys. Lett. B. 151, 37 (1985). H. Etcheaherr. Phys. Lett. B. 147. 212 (1985). Al. B. Zamolodchlkov. Commun. Math. Phys.. 96, 419 (1984). L. D. Faddeevand L. A. Takhtadzhyan, Usp. Mat. Nauk, 34, 141 (1979). E. K. Sklyaniu. Funktslonal. Anallz 1 Ego Prllozhen., IS. 98 0982). D. Friedan. Z. Qlu. and S. Shenker. Phys. Rev. Lett.. 52, 1575 (1984). V. S. Dotsenko. Nucl. Phys. B. 241 (FS11). 57 (1984).
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Reprinted with permission from Physics Letters B Vol. 207, No. 3, pp. 295-299,23 June 1988 © 1988 Elsevier Science Publishers B. V. (North-Holland) EXTENDED CONFORMAL ALGEBRAS Peter BOUWKNEGT Institute for Theoretical Physics, University of Amsterdam. Valckemerslraat 65. 1018 XE Amsterdam. The Netherlands Received 30 March 1988
We investigate extensions of the Virasoro algebra by a single primary field of integer or halfinteger conformal dimension A. We argue that for vanishing structure constant C j j , the extended conformal algebra can only be associative for a generic c-value if J = 1 / 2 . I. 3 / 2 . 2 or 3. For the other J < 5 we compute the finite set of allowed c-values and identify the rational solutions. The case Cjj * 0 is also briefly discussed.
Recently much progress has been made in our un derstanding of two-dimensional conformal field the ories (CFTs). An important subclass of all CFTs are those for which the partition function is composed of finitely many analytic building blocks. These are called rational CFTs [ 1 ]. It is hard to imagine how thisflnitenesscomes about for central charges 01, unless there is some larger symmetry algebra in the game. The analytic building blocks would then be the characters of this extended algebra. So it is argued that one can classify all RCFTs by finding all possible ex tensions of the Virasoro algebra. There is an ambiguity in what one would call the symmetry algebra of a RCFT. We adopt the conven tion that the symmetry algebra is a minimal set of primary fields, forming a closed operator product al gebra (OPA), that have to be added to the Virasoro algebra such that the torus partition function is a fi nite sesquilinear sum of irreducible characters of this extended conformal algebra. With this definition it is very likely that, at least for RCFTs with periodic boundary conditions, only integer dimension pri mary fields have to be added [2]. However for fermionic theories, allowing for anti-periodic fields, it might prove to be convenient to introduce also halfinteger dimensions. Motivated by the apparent relation between RCFTs and coset pairs of Kac-Mcody algebras, many ex tended conformal algebras have been constructed (3,4]. Their representation theory has been investi gated by generalizing the Feign-Fuchs construction
[3,5]. Recently, a step towards classification of RCFTs of central charge C3> 1 has been taken by de riving very restrictive conditions on the central charge and conformal dimensions of the primary fields pres ent in a closed associative OPA [6,7]. The results, however, do not put any restrictions on the possible symmetry algebras, as defined above. In this paper we will make an attempt towards clas sification of the symmetry algebras by considering extensions of the conformal algebra by a single chiral primary field #j, of conformal dimension A. We nor malize 0j such that
*V*j = (cAm/]+C J j[* J ],
(1)
where [/] and [0j] respectively stand for the confor mal family of the identity operator and the primary field M 8 ] . Motivated by the discussion above we will restrict ourselves to integer or halfinteger J". Algebras of this type for J ^ 3 werefirstsystematically analyzed in ref. [9]. The outcome was that for J = 1/2, 1,3/2, 2 and 3 the OPE (1) gives rise to an associative OPA for a generic value of the central charge c. We will argue that for vanishing structure constant Cjj these are in fact the only possible conformal dimensions. For Cjj # 0 it is also possible to take A=4 and possibly alsoJ=6. The object of our analysis in the four-point corre" In fact the condition 2 J e Z , 0 is not too restrictive as it has been shown that algebras of type ( I ) require 4 J E Z > 0 [ 6 ] .
295
231 lation function of the primary field 4>A which because of projective in variance has the form
= (Z,-z4)-^(2,-r2)-"»""U),
(2)
(3)
Associativity of the extended conformal algebra (1) is equivalent to requiring crossing symmetry of the four-point functions [ 8 ]. If only one primary field
yu,{x)
=
(c/A)2P(A,0,x)
+ (c/A)(C£)2?(A,A,x)
+ ...
(4)
The... stand for the conformal blocks of the primary fields entering in the regular part of the OPE( 1), which are secondary with respect to the extended symmetry algebra. The conformal block can be computed perturbatively [8] ": ,
f{A,A ,x)=x"'
2A
£ x"?„(A,A).
(5)
On the other hand, if 2JeZ > 0 one can use (1) to write down Ward identities expressing the four-point func tions in lower correlation functions [ 8,9 ]. The Ward identities allow one to compute Sf1"" (x), after which crossing symmetry can explicitly be verified. This method was employed in ref. [9] for A43, but be comes rather cumbersome for larger A because the OPE coefficients of the secondary fields have to be computed explicitly. However, as we will show in the following, using some ingredients of finite group the ory, the possibility of crossing symmetry can be in vestigated by means of simple counting arguments. From the Ward identities one can easily see that the four-point function &" (x) is a linear combina tion of functions from the set 11
For the purpose of this paper we computed £(J.O) upton=9. and .SM,4')uptoii«:3 [10).
296
I / J t " - ' , . . . , 1/X, 1 ,
1/(1-*)
1/(1-*)"}.
(6)
Let us now define the following transformations on meromorphic functions/(jr): (Sf)(x)=x-2Jf(l/x),
where x is the anharmonic ratio x=(z1-22)(zJ-z4)/(z1-r4)(zj-z2).
S={l/x2J,
(Tf)(x)=Al-x).
(7)
For integer A, S and T generate the dihedral group 3>3, defined by the relations S2 = T2 = (S7")3 = 1. For halfinteger A, S and 7" generate the double covering S> 6 s«3®£ 3 , defined by S2 = T2=(ST)i=l [11]. The requirement of crossing symmetry is the require ment that *"> (x) should be a singlet under 9, for integer A, i.e. transform according to the identity rep resentation p(S) = 1, p( 7") = 1. For halfinteger A it should transform according to the one-dimensional representation p(S) = - 1 , />( 7") = 1. The set 5 forms a basis for a reducible representation of 3, respec tively S)t, which we also denote by S. To count the number of independent crossing symmetric func tions in 5, we have to count the number of represen tations p, say Nr that are present in S. This is most easily done by computing the character x*(g) = IxS(g) of the representation £, for every group ele ment g. The number of representations/) can then be computed by taking inner products
Nm
' ikZbx'l')Xxls)' for G = &, respectively S 6 .
(8)
The result is N, = \(A+\)
+ \t,
(9)
where {=-1
ifJ=lmod3/2,
=0
ifJ=l/2mod3/2,
=1
ifJ=0mod3/2.
(10)
A basis {/>,u>,i=l N„} for these crossing sym metric functions can easily be constructed by taking />-orbits of functions / e ; . P(x)=
£ p(g)(gf)W
.
(11)
For instance the orbit off(x) = 1 Ix24 is given by P{x)=[l/x2A+\/(l-x)2J+(-l)2J). We can express the four-point function (2) as
(12)
232
(13)
By comparing the first few terms in the perturbative expansion (5) with the explicit form of the functions />,'•" the expansion coefficients a, can be computed. In general this is an overdetermined system of equa tions allowing only solutions for specially chosen val ues of c. It is this observation that we will analyze in more detail. First consider the case Cjj = 0. In fact Cjj can only be nonzero for Ae 2Z >0) because of spin statistics and symmetries of (1). In case C J = 0 only the conformal block ?(A, 0, x) is present. The analytic properties of the conformal block functions ?(A, A', x) were studied in ref. [12]. It turns out that ?(A, A', x) is a meromorphic function of c with poles only in the finite c-plane, their posi tion being determined by the Ka£ formula [13]. From the pole structures in c of the conformal block coef ficients JF(J, 0) (5) it follows that the coefficients *AA, 0) are linearly independent. Also one can ar gue that the coefficients !$„+ i (A 0) can be expressed as a linear combination of the ^», k^n [10]. Ob viously, the four-point function (2) can only be crossing symmetric for a generic c-value, if the num ber of invariants N„ is greater than or equal to the number of different pole structures %, for ne {0, 1,2, .... 1A-1} [i.e. in the singular terms of the OPE (1) ]. This only happens for A= 1/2,1, 3/2,2 and 3. Summarizing, we conclude that only for A = 1 / 2 , 1 , 3/2, 2 and 3 are there enough invariants to build the conformal block &(A, 0, x) for a generic value of c. Realizations of these symmetry algebras for A < 2 are well known. Recently it has been shown that the J = 3 algebra [ 9,14 ] can be realized as the Casimir algebra ofSU(3) [3]. For the other As there appear consistency condi tions on the a, which can only be solved for a finite set of c-values. We list the cases A ^ 5:
It is remarkable that all the solutions for c (except for c = - 3 5 ) are members of the minimal series [8] c(r,s) = l-6-^y-L-
(15)
obtained from the level 1 A \'> vertex operator reali zation, by the Feign-Fuchs construction ". The po sitive rational solutions are members of the unitary discrete series [15]. We remark that the rational A=5 solutions c = 6 / 7, — 7 and —350/11 are also members of the minimal series of the E (6) Casimir algebra [ 3 ] c(r,s) = 6 n - 1 2 1 3
(r
~5) j .
(16)
Apparently, for the c-values 6/7, - 7 and -350/11 the higher order Casimirs of E (6) are null fields, and the symmetry algebra is effectively reduced to the al gebra of the second and fifth order Casimir only. We believe that in general consistent rational c-values signify the presence of a minimal series of some ex tended algebra containing #> We have no explana tion nor interpretation for the occurrence of nonrational consistent c-values. We should stress, however, that (14) only lists the consistent c-values, obtained by comparing (13) with the singular terms in the perturbative expansion (5). It may still be pos sible that some c-values turn out to be inconsistent at a deeper level in the perturbation expansion. In any case the nonrational solutions would not correspond to RCFTs, because it has been shown that having a finite set of primary fields in the operator content of a CFT implies rationality of c [6]. The mechanism which makes associativity of the OPE hold only for special values of c can be made more explicit. Suppose we have an operator product expansion between two fields A and B of integer or halfinteger conformal dimension,
A(z)B(w)= I {**}'lWJ +{AB}0(w) + ...,
(17)
J=5/7-c=-13/14, J=7/2-c=21/22, -19/6, -161/8 ,
and normal ordering of A and B is defined by ■AB:(z)m{AB}0(z). Then the normal ordered "graded" commutator of A and B is given by [ 3 ]
J=4-»c=86±60y2, 4=9/2-c = 25/26, - 7 / 2 0 , -125/22, -279/10, - 3 5 , J = 5 - c = 6 / 7 , -350/11, - 7 , 1 3 4 1 6 0 ^ 5 .
(14)
" From the known fusion rules of the minimal models [8] one can of course also obtain a set of comment c-values for larger
297
233
:[A,B]:(z)=
£ ^d'{AB)r(z)
.
(18)
Associativity of the OPA implies the Jacobi identity :[:M,5]:,C]:(z)+cycl. = 0.
(19)
Consider for instance the case A=5/2. Using the ex plicit OPE [9] it is straightforward to verify that ** :[:[05/2,05/2]:,05/2]:(-) = 3 ! * ( r ) ,
(20)
I would like to thank Kareljan Schoutens for dis cussions and Sander Bais for a careful reading of the manuscript. This work is financially supported by the Stichting voor Fundamenteel Onderzoek der Materie(FOM).
where
+ ^j-c(l:Tdi>in:-^S:T0in:).
(21)
So in general the associator does not vanish. How ever, precisely for
"'
34(c+24)(c'-172c+196) (5c+22)(7c+68)(2c-l) '
This J = 4 algebra is supposedly realized by the Casimir algebra of Sp(4). Similarly the J = 6 algebra is supposed to correspond to the Casimir algebra of G(2) [3,16]. For A>% the naive counting would suggest that it is impossible to build a crossing sym metric four-point function for generic c-values. How ever, we cannot completely exclude the possibility of cancellation between various terms in the two con tributing conformal block functions. ** In general it is not sufficient for associativity of the OPA to check (19) for the primary fields only.
298
So far we have discussed extensions of the confor mal algebra by a single primary field. If more pri mary fields are included then of course there are more four-point functions that have to be analyzed (see e.g. ref. [ 17 ]). It is not inconceivable that similar count ing arguments can be used to extend the analysis of this paper to more complicated symmetry algebras [16].
References [ I ] D. Friedan and S. Shenker. unpublished. [2) MR. Douglas, preprint CALT-68-l 453 (September 1987): P. Bouwkncgt. preprint ITFA-87-23 (December 1987). Proc. 1987 Brasov Intern. Summer School on Conformal invariance and strings. [3] F.A. Bais. P. Bouwkncgt. K. Schoutens and M. Surridge. preprint 1TFA-87.I2/THU-87-J8 (August 1987); preprint ITFA-87-I8/THU-87-2I (September 1987). Nucl. Phys. B. to be published, preprint 1TFA-87-22/THU-87.29 (De cember 1987), in: Proc. Copenhagen meeting on Perspec tives in string theory (September 1987). to be published. |4) V.A. Falcev and S.L Lykyanov, Intern. J. Mod. Phys A 3 (1988)507: T. Hayashi. thesis Nagoya University: R. Goodman and N.R. Wallach. Rutgers preprint (1987); 1. Thierry-Mieg. preprint DAMTP-87-29 (November 1987), in: Proc. 1987 Cargese school on Nonperturbative quantum field theory, to be published: P Goddard and A Schwimmer. preprint DAMTP-88-02 (January 1988); A. BilalandJ.L. Gervais. Phys. Leu. B 206 (1988)412. [ 5 ] D Kastor. E Mamnec and Z Qiu. Phys. Lett. B 200 (1988) 434; J. Bagger, D. Nemeschansky and S. Yankielowic2, Phys. Rev. Lett 60(1988)389: V. Pasquier. preprint SPhT-87-125 (September 1987); F. Ravanini. preprint NORDITA-87-56 (October 1987); J. Soda and H. Yoshn. preprint RRK-88-5 (February 1988). 16 J C Vafa, Phys. Lett. B 206 (1988) 421. [7]E. Verlinde. preprint THL'88-17 (February 1988). [8JA.A. Belavin. A.M. Polyakov and A.B. Zamolodchikov. Nucl. Phys. B 241 (1984) 333. [9) A B. Zamolodchikov. Theor Math. Phys. 65 (1986) 1205. [ 10] P. Bouwkncgt. to be published elsewhere.
234
( I I ] H.S.M. Coxeter and W.O.J. Moser, Generators and rela tions for discrete groups (Sprinter, Berlin, 1980). [12] A.B. Zamolodchikov, Commun. Math. Phys. 96 (1984) 419. [ 13 ] V.G. Kac, Lecture Notes in Physics, Vol. 94 (Springer, Ber lin, 1979) p. 441; B.L. Feign and D.B. Fuchs, Funct. Anal. Appl. 16 (1982) 114. [ 14] V.A. Fatecv and A.B. Zamolodchikov, Nucl. Phys. B 280 [FS18] (1987)644.
[ I 5 ] D . Fnedan. Z. Qiu and S. Shenker, Phys. Rev. Lett. 52 (1984) 1573; Commun. Math. Phys. 107 (1986) 535; P. Goddard, A. Kent and D.I. Olive, Commun. Math. Phys. 103(1986) 105. [16] Work in progress. [17] V.G. Knizhnik. Theor. Math. Phys. 66 (1986) 68; S.A. Apikyan, Mod. Phys. Lett. A 2 (1987) 317.
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Reprinted with permission from Nuclear Physics B Vol. 361, pp. 255-289,1991 © 1991 Hsevier Science Publishers B. V. (Noith-HoUand)
3T-ALGEBRAS WITH TWO AND THREE GENERATORS R. BLUMENHAGEN, M. FLOHR, A. KL1EM, W. NAHM, A. RECKNAGEL and R. VARNHAGEN Physikalisches Institut der Universital Bonn, Nussallee 12, 5300 Bonn I, Germany Received 30 July 1990
We construct all '^algebras of chiral fields which in addition to the energy-momentum density have a single generator of conformal dimension up to 8. Some of them were unexpected, which indicates that present conjectures concerning the classification of conformally invariant quantum field theories in two dimensions are rather incomplete. We also explicitly construct the ^Aj-algebra with generators of dimensions 2,3,4.
1. Introduction Since 3T-algebras were discovered by Zamolodchikov in 1985 [1], they have become more and more important in theoretical physics. They not only serve as a useful tool in the investigation of integrable systems [2], but also provide a promising approach to the problem of classifying all rational conformal field theories (RCFT). As is well known the latter is one of the outstanding questions in statistical physics as well as in string theory. Furthermore, this problem is of mathematical interest, too, because of the connection of RCFT with certain invariants of 3-manifolds via topological quantum field theory [3]. As far as the classification problem is concerned, the study of '^-algebras in some sense provides a concept complementary to that of fusion algebras. These deal with abstract properties of representations of conformally invariant operator algebras, leaving the latter more or less unspecified. In contrast, when investigating 2T-algebras one tries at first to construct an algebra of local fields explicitly and then to get insight into RCFT from its irreducible representations. 2T-aIgebras, also called extended conformal algebras, describe the operator product expansion (OPE) of conformally invariant chiral fields. The singular part of such an OPE yields a Lie bracket structure, the regular part an operation of forming normal ordered products. In constructing these algebras one usually proceeds in such a way that the more restrictive conditions of conformal invariance are satisfied a priori, whereas the requirements which have to be insured "by hand" are the simpler ones arising from either Jacobi identities or associativity of
236
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R. Blumenhagen el at. / ^-algebras
the OPE together with crossing symmetry of the 4-point-functions. If one chooses the OPE point of view, the explicit calculations that have to be performed include - following the lines of Belavin et al. [4] - the determination of the structure constants of the primary fields as well as the coefficients of the descen dants, which can be done using the conformal bootstrap method. For exploitation of the associativity condition for four identical fields one has to investigate the restrictions from D3-invariance of the 4-point-function. This task has been carried out more or less completely for the spin 4 extended algebra [6,7], the spin 6 case [8], and some other lower spin algebras in ref. [5]. In this paper we use the Lie bracket approach. On the one hand in this method there are more structure constants to be calculated and the notion of normal ordered products needed is slightly more involved, but on the other hand we do not have to deal with coefficients of derivative fields, as these are incorporated in some universal polynomials depending only on the conformal dimensions of the fields. The consistency conditions arising from the Jacobi identities in the cases we investigate reduce to just one equation by means of some general theorems. It turns out that this treatment is systematic enough to be easily put into an algorithm feasible for computers. The paper is organized as follows: In sect. 2 we briefly outline the basic features of our approach to the construction of 3T-algebras, including some definitions, a theorem that fixes the commutator of two local fields up to structure constants, and some lemmata important from both the purely theoretical and the calculational point of view. In sect. 3 these general results are applied to a few simple cases of 9T-algebras, namely extensions of the Virasoro algebra by a single local field of spin \ to 8. By the same methods we construct the 2T-algebra containing a spin 3 and a spin 4 primary field. To keep the presentation concise, some of the calculational details are collected separately in appendix A. Sect. 4, besides from a short summary, gives a few proposals concerning higher spin cases.
2. General results. An algorithm for the construction of 3T-algebras Let 9~ be the algebra of local chiral fields of a conformal field theory defined on 2-dimensional space-time (with compactified space). Because of SU(1, l)-invariance 9~ carries a natural grading by the conformal dimension and is spanned by the non-derivative (i.e. quasi-primary) fields together with their derivatives. Local ity and invariance under rational conformal transformations impose severe restric tions upon the commutator of two chiral fields so that it is almost completely determined by their dimensions, up to some "structure constants". Theorem. Let {<j>t\i e 1} be a set of non-derivative fields of integer or halfinteger conformal dimensions rf(<£,) = h(i), which together with their deri vatives span &. Define the Fourier decomposition of left chiral fields by
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R. Blumenhagen el al. / W-algebras
257
(z) = L„^zz"~'"-4')<(>n, and denote the vacuum of the theory by |v>. Furthermore, put <*y=
ijk =
(2-la)
■
Then the Lie algebra of the Fourier components of the left fields has the form
[*,.«.*>.-] ± = Zc!iPiik{m,n)4>k.m+n + du8n,_J\"+^~^Y
(2.1b)
where C'ijdlk = Cijk. Using the notation h(ijk) = h(i) + h(j) - h(k) the universal polynomials pjjk are given by Pilk{m,n)=
£
cnklm+h(i)-\\ln+hU)-\\
f,jeZt r + s = hVjk)- 1
\
f
l\
{2Ac)
S
J
with c«* Cr J
-
-(-l)' V
}
(2Mfe)
"1)!5!r! (h(i)+h(j)+h(k)-2)\\
(2A(0-2-rU2A(;)-2-5\ s )[ r )' (2.1d)
The C,;/t are invariant under even permutations of their indices and change under odd permutations by a sign factor ( - l)h<-'ik\ Let & in addition carry an involution (f>^-*4>+. If one chooses the fields to satisfy >(+ = (-1) [ '' (01 #_ / , then the structure constants dtj and Cjjk are real. For a proof of this and the following statements as well as for more details cf. ref. [9]. In addition to their Lie bracket structure 3T-algebras admit another important operation, namely forming normal ordered products (NOPs) from chiral fields. Usually the NOP of two chiral fields (f>, x is defined in terms of Fourier compo nents as follows N{4>,X)n-=
E k«Hx)
4>„-kXk+ E
XAn-k\
(2-2)
k>d(x)
in this form it occurs in the OPE of 4> and x (see below), but is not a non-derivative field, so that e.g. eq. (2.1) cannot be used to gain any information about its commutator with other fields. For the NOP to be "well-behaved" under
238
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R. Blumenhagen el al. / TV-algebras
SU(1, ^transformations we have to add some corrections to N(
£(_1)^)(A(yA:)+a(^) + 2«-lj"1/2/1(/)+n-lj
{ * : « « * ) > 1} x(h(ijk)
I
+a(ijk)+2n n
'a(ijk)-l\~l h(ijk)-lj
^
"
'
- 1 )"'[2hU) +« ~ 1 \ / \ h(ijk)+n j d"^+"
where
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R. Blumenhagen el al. / JP-algebras
259
The division of non-derivative fields into NOPs and simple fields proves to be very useful because of the following Lemma. The commutators of normal ordered products are completely deter mined by the commutators of the simple fields involved. This means that the whole Lie algebra structure of the 3T-algebra is already fixed by the commutation relations of the simple fields it contains. For instance, we can derive recurrence formulae like the following which is useful for the calculations of sect. 3: Denote two primary fields by their conformal dimensions 5 and 5', let Y be an arbitrary non-derivative field and X-=Jr(Y,d"L). With D = h(X) = h(Y) + n + 2 we have
X(8'(n
(
l)
+ 2-r
+ k) - (8 - D + n + 2 - r + k))Caii.Y
2(2D-n~3)
\
n
)
{
n + 2
j
C
^
{2A)
The general setting outlined above is sufficient to formulate an algorithm for the explicit construction of chiral ^algebras with finitely many simple fields. The steps of the scheme are as follows: (a) As an input, the content of Virasoro-primary simple fields has to be fixed; for simple fields of dimensions h(i) we denote the resulting J^-algebra by 7fX2, Ml), h(2),...). (Here 2 of course symbolizes the Virasoro field, whereas the occurrence of the unit operator is not explicitly noted.) (b) Form all linearly independent NOPs which may occur in the commutators of the simple fields. In particular, one only needs those NOPs with dimension up to 2 5 - 2 , where 6 is the maximum dimension of the simple fields (25 - 1, if 5 is half-integer). (c) Calculate the structure constants showing up in the commutators of two simple primary fields using the theorem. Some of the structure constants, namely those connecting three simple primary fields, will remain free parameters at this stage. (d) Whereas SU(1, l)-invariance of the 2T-algebra is already guaranteed by the form of the universal polynomials in eq. (2.1), the validity of the Jacobi identities still has to be checked. This yields a certain number of conditions on the free parameters of the theory (also cf. ref. [5]). At first sight the last step seems far from being manageable. Because of the preceding lemma, however, one only has to require the vanishing of [[•^A'L'/'l + cycl. for three simple fields <{>, \ , and t/», in order to ensure that the
240
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R. Blumenhagen el al. / ^-algebras
Jacobi identity holds for all other non-derivative fields, too. Moreover, it is sufficient to consider the primary fields on the r.h.s. of this expression (cf. refs. [9] and [10]). As, in addition, all Jacobi identities involving the energy momentum tensor on the l.h.s. are trivially fulfilled (this is essentially due to the fact that the structure constants containing descendant fields are already fixed by invariance under arbitrary conformal transformations), for the W(2,5)-algebras step (d) actually reduces to checking a single Jacobi identity. Validity of the Jacobi identity imposes the only restrictions upon the structure constants and the central charge of the theory. When these are fulfilled, our construction guarantees the existence of the 3^-algebra under consideration, or equivalently, associativity of the field algebra with respect to OPE. For complete ness we note that the OPE of two non-derivative fields can easily be obtained by using the structure constants of eq. (2.1):
*,-(*)4y(H')= L(z-w)-Miik)CJ'Ji^-(z-WyyM^)
(2.5a)
with , r 1 flfy4_|2A(*)+r-l)" |A(*w)+ " )-
(2.5b)
3. Explicit construction of some /^-algebras In the following the algorithm explained in sect. 2 is applied to a few cases of /^-algebras. To be specific, we study the 2T-algebras 3T(2,8) generated by the Virasoro field and one additional (local) primary of dimension (spin) 8 for 8 = f to 8, as well as the algebras 2T(2,3,4) and 2T(2,4,4). For the simplest of these examples, there already exist some results in the literature, which, however, are incomplete or rely on rather unsystematic methods in some cases. In contrast to this, our approach not only is more conceptual, but also provides a straightforward way of testing the existence of any finitely gener ated a^-algebra, the only restrictions coming from practical limits of computer calculations. The algebras W(2,8) with bosonic extra primary, that is 8 = 4,5,6,7,8, will be discussed in more detail, whereas in the fermionic cases we Just list the essential results. 3.1. THE ALGEBRA 2r(2,4)
This 2T-aIgebra provides the opportunity to discuss the essential steps of our algorithm in a well known example [5-7]. The simple fields here are the unit
241
R. Blumenhagen el al. / "^-algebras
261
operator, the energy momentum tensor satisfying the Virasoro algebra [Lm,Ln]
+ -t-2c(n3-n)8n+m0,
= (n-m)Lm+n
(3.1)
with central charge c, and an additional primary field W of conformal dimension 4: [Lm,W„] = (n-3m)Wn+m.
(3.2)
The expression we have to investigate is the commutator of W with itself. From locality and SU(1, l)-invariance this can only contain non-derivative fields of even dimension h up to h = 28 - 2 = 6, namely \,L,W itself and NOPs of these dimensions. The latter are given by h =4
A-=jV(L,L)=N{L,L)-±d2L,
2 1 h = 6 r~jV( L,d2L) = N( L, d2L) - dN( L, dL) + - d2N( L, L) - — d*L, d2A ,
A -=jr( A, L) =N(A,L)-6
n-=Jr(<W,L)=N(W,L)--d2W. 6
(3.3)
(Note that there are precisely p(6)- 2 p ( 5 ) + p ( 4 ) = 2 linearly independent NOPs of dimension 6, which can be built from L and its derivatives alone, as was stated in sect. 2.) In terms of these fields, the commutator of W with itself takes the form [Wm,Wn] = -\n1J3}8n+m,o
+ CkiVP442(m,n)Lm+n
+
+ C%wp^{m,n)Wm+n
+
+ C^iVpA4b(m,n)Am+n
+ C^iVpAA6(m,n)nm+n.
C*lvP444(m,n)Am+n
ClvwpA46(m,n)rm+n (3.4)
Throughout this paper we normalize W in such a way that dww = c/8.
(3.5)
Using the general formula in the theorem we can calculate the structure constants Cww from t n e relation C$lvdXY= CWWY. For h(X) = 6 the matrix D6 = (dij) with d(
242
262
R. Blumenhagen et at. / M-algebras
r and A) being orthogonal to those involving one W-field (here: fi), its determi nant det D6 = det D^det
Dp> =
[ c2 \ I c(c + 24) \ — (7c + 68)(5c + 22)(2c - 1) ^ , (3.6)
splits up into two factors, the first coming from A and T, the second simply being equal to dnn. We arrive at 42 5c + 22 3(19c-524)
r
Cww=
10(7c
A
+ 68)(2c-l) '
Cww=
24(72c + 13) (5c + 22)(7c + 6 8 ) ( 2 c - l ) '
28 C
^
H/=
3 ( c + 24)C^H/-
(3 7)
'
Note that the denominator zeros of the structure constants correspond to certain null states coming from the Kac-determinant which will make the algebra inconsis tent. For example for c = - ^ we have 354 - \ir= 0. Apart from the central charge c the structure constant C^,w up to now remains as a free parameter. The requirement that the Jacobi identity holds for three Jf-fields sets up a relation between these two constants. Insert (3.7) into [[Wm, Wn\, Wq] + cycl. = 0 and use eq. (2.1). This yields [[Wm,Wn],Wq]+Cycl.
= P2(m,n,q)Lm+n+Q+P4(m,n,q)Wm+n+q
+
Rm+n+lj±0. (3.8)
Here by Pk(m,n,q) we denote linear combinations of products of the universal polynomials, also containing the central charge c and the structure constant C^w The non-simple part of the r.h.s. is summed up into Rm+n+q. As was explained in sect. 2, for the whole r.h.s. to vanish it is sufficient that P^{m,n,q) = 0. Inserting the explicit form of this polynomial and taking advantage of some linear dependen cies of products of the universal polynomials occurring in this expression leads to the following condition on the structure constant C^w c2 - 172c + 196
5c + 22 , ,„ , 2 C
54
772J-< -> ° (7c + 6 8 ) ( 2 c - i ) '
<39a)
243
R. Blumenhagen el al. / M'-algebras
263
which for c # - 2 4 fixes the c-dependence of C%w to be w Cww)
^
2 =
54(c + 24)(c 2 -172c+ 196) (5c + 22)(7c + 6 8 ) ( 2 c - l )
;
( 3 % )
at the value c = — 24 of the central charge eq. (3.8) cannot be fulfilled. Condition (3.9) already ensures that the Jacobi identity is valid for all chiral fields occurring in W{2,4), so this 3T-algebra W(2,4) exists for generic value of the central charge c with exception of the single values c = - 2 4 , - T> ~ T> 5 a n c ^ t n e domains 86 - 60v/2 < c < 86 + 60\/2, as well as - f < c < ^ and - 24 < c < - f, where C%w would not be real (which, according to the theorem of the last section, is impossible if the field algebra :T carries an involution $->(£ + ). Furthermore, note that the structure constant C%w vanishes for c = 86 ± 60/2 , whereas at the 'zero' c = - 24 the algebra actually is inconsistent. This analysis confirms and completes the results of refs. [5-7]. (In ref. [6] the numerical factor showing up in the relation between c and C^w is wrong.) 3.2. THE ALGEBRA 3^(2,5)
The initial data are as above, but W now has dimension 5 = 5: [Lm,W„] = {n-4m)W„+m.
(3.10)
Because 5 is odd, W cannot show up in its commutator with itself, i.e. C^w = 0 from locality. The NOPs relevant for [W, W] are A,T, A as before and three additional fields of conformal dimension 8: El--=sT(A,L),
E2-=,r(r,L),
E3-=yr(L,d4L).
(3.11)
In principle the NOP X = ./P'{W,dL) could also occur in the commutator [W, W\, however, it is easy to see that the structure constant C$,w ' s proportional to C^w, so that this field does not contribute. For this and the next examples the determinants of the ^—matrices and the structure constants for the NOPs occurring in [W, W] are listed in the appendix. Using these, we exploit the Jacobi condition as before. In contrast to the algebra 2^(2,4), where two free parameters existed, in the case W(2,5) this leads to a condition that leaves only 5 possibilities for the central charge: 6
350
r~ c=-,-7,-—,134±60i/5.
(3.12)
Only for these values of c the W(2,5)-algebra is consistent (see also ref. [5]).
244
264
R. Blumenhagen el al. / ^-algebras
3.3. THE ALGEBRA 2r(2,6)
Here W denotes a primary field of dimension 6: [Lm,Wn] = (n-5m)Wn+m.
(3.13)
Just as in the first example, C^,w here is a free parameter not restricted to be zero. The NOPs relevant for the commutator [W, W] are those already listed for W{2,5) in subsect 3.2 plus one non-derivative field of dimension 8 il-=jr(W,L),
(3.14)
and the following NOPs of dimension 10: T\=jr(E\,L), P=jT(n,L),
T2-=JT(E2,L),
X:=JV(W,d2L).
T3 ==^(£3, L) , T4-=J^(L,d6L) , (3.15)
Calculation of the structure constants C^,w yields very complicated expressions in c and C%w, which have to be inserted into [[Wm, Wn], Wq] + cycl. = 0. From the l^m+n+1?-term of this Jacobi identity one then obtains in complete analogy to 3^(2,4) the c-dependence of C^w-
w Cww
(
2
>
=
400(c 2 -388c + 4)(c + 2)(c + 47)2(13c + 516)2 3(5c + 22)(7c + 68)(2c - l)(5c + 3)(3c + 46)(3c + 286)(llc + 232) ' (3.16)
For similar reasons as in the example W(2,4) the c-value c = - 2 has to be excluded here, W(2,6) is inconsistent for this central charge. Re-inserting (3.16) into Cfrw leads to the relatively simple structure constants listed in appendix A. In conclusion 3^(2,6) exists for all values of the central charge with the exception of c = - 2, the denominator zeroes and of the following intervals, where CZw w o u l d not be real: 194 - 1 1 2 ^ < c < 194 + 112^2, - f < c < | , - f < c < - 2 , - y < c < - y , and, with the double zeroes - 4 7 and - ^y excluded, - ™
245
R. Blumenhagen et al. / W-algebras
265
3.4. THE ALGEBRA 2T(2,7)
W now has conformal dimension 5 = 7 [Lm,Wn}
= {n-bm)Wn+m,
(3.17)
the structure constant C^w has to vanish as in the case 5^(2,5). The relevant NOPs are those built up only from L and derivatives thereof; the other ones like yV(W,dL) do not contribute to [W, W] for the same reason as in the example W{2,5). So we have to take into consideration all the NOPs of W(2,6), except for O, P, and 1 of course, as well as seven new fields of dimension 12: D\-=Jf(T\,L),
D3-=J^(T3,L)y
D2-=JV{T2,L),
D5-=yy(L,dsL),
D6-=sr(E3,d2L),
D4-=yV{T4,L),
Dl-=Jf(Jf{&,dL),dL).
(3.18)
The polynomials involved in the Jacobi condition (cf. the more detailed discussion of 3F(2,4)) in this case span a two-dimensional space; therefore, one might expect that W{2,1) cannot exist for any c-value at all. One finds, however, that this 3T-algebra is consistent for 25 c = - y .
(3.19)
In particular, our result shows that there is no unitary representation of W{2,1).
3.5. THE ALGEBRA 2T(2,8)
The calculation proceeds in analogy to the previous cases, with [Lm,Wn]
= {n-lm)Wn+m;
(3.20)
here C^w again is a second parameter. The non-derivative fields which have to be taken into consideration are those occurring in W{2,7) and the following NOPs of dimension 14: F\-=Jf(D\,L),
F2-=yT(D2,L),
F3-=yK(D3,
L),
F4=J^(D4,L),
F5 =yT(D5,L),
F6-=^(D6,L),
Fl -=jr{Dl,
L),
F8-=yr(T4,d2L),
F9-=yT(J'(E3,dL),dL),
FlO-=J^(L,di0L).
(3.21)
In addition, there are some NOPs containing the primary field W, namely n-=Jf(W,L),
(3.22)
246
266
R. Blumenhagen el al. / 7P-algebras
having conformal dimension 10, P=yT(fl,L),
2-=yr(W,d2L),
(3.23)
with dimension 12 and four more fields of dimension 14: ri-=yT(P,L),
T2:=JT(2,L),
T3—jr(jr(lV,dL),dL),
T4-=yr(W,d4L).
(3.24)
Their determinants and structure constants are listed in appendix A. For W(2,8), the polynomials in the Jacobi identity span a two-dimensional space as in the example before, so this algebra should exist at least for some isolated values of the central charge. Indeed one finds that W{2,8) is consistent for the rational values 21
224
22
65
944 1015 17
2
(3.24a)
with the corresponding structure constants (in the same ordering) . ,„
x2
W
2731943701550627281872
)=
(Q v
86005968234265625
ww
'
124088261649132 ' 32463659123020775 ' 83237962743648511799 0, (3.25b) v 155898446715324359100 ' (surprisingly, the huge numerators and denominators of these expressions decom pose into very small prime factors), and for the irrational c-values c = 350 ± 2 5 2 ^
(3.26a)
with positive structure constants {Cwwf
= 23814(687101988298954903007869659141427107^ ±971708950585901684115820941603319346)/ (73150235(49583364744608221528766050177884819\/2 +70121466889916921151822857852723281)).
(3.26b)
For the values c = - 2 3 , - ^ , and - ^ of the central charge the Jacobi identity is fulfilled, but with negative (Cj^w)2. In principle, the algebras W{2,8) for S > 8 can be investigated by the same method, but the calculational effort grows very fast with 8 (roughly with 5!, which
247
R. Blumenhagen et al. / jt'-algebras
267
is the number of commutations necessary in order to compute the structure constants du). However, just by taking a closer look at the polynomials occurring in the Jacobi conditions, one may immediately conclude that these algebras can only exist for isolated values of the central charge, because the number of linearly independent conditions hidden in the Jacobi identity for three H^-fields is at least two (and increases even more for higher 8 [5,9]: approximately with 5/3), whereas there are at most the free parameters c and C^w. On the other hand, our conjectures in sect. 4 suggest that for arbitrarily high 8 there is indeed at least one c-value for which W(2,8) is a consistent ^-algebra with vanishing structure constant C L .
3.6. FERMIONIC CASES
Here we briefly discuss the algebras W{2,8) with an additional generator of half-integer dimension 8 = 1 to -y. In these cases no new fields have to be considered. Actually, the anticommutator {Wm, Wn), which is the object to be studied here, can only contain NOPs of even spin formed entirely out of the energy momentum tensor and its derivatives, up to dimension 28 - 1. In particular, the structure constant C^,w does not appear, so we expect these algebras to exist only for some isolated values of c. Because the analysis is completely analogous to the examples studied before, we refrain from giving any details (cf. appendix A for the structure constants). We merely list the values the central charge has to take on in order to ensure the existence of the respective ^"-algebras in table 1 (cf. also ref. [5]). In sect. 4 we will give a few proposals how these values may be interpreted as members of certain series. In particular, the argument dealing with higher spin algebras mentioned in the last paragraph applies to the fermionic case just as well.
3.7. #(2,3,4) AND OTHER ^-ALGEBRAS WITH THREE GENERATORS
The remainder of this section is concerned with ^-algebras of slightly different type, namely examples generated by the energy momentum tensor L and two additional primary fields. We will discuss the example iF'(2,3,4) in some detail, TABLE 1
The c-values for which the existence of fermionic 2C(2, S)-algebras is proven ar(2,|): 3^(2,1):
c c
5T(2,JJ):
c
ar(2, ^ ) :
c
Sr(2,Ji):
c
-35;
-
217. 26 • 9 611 34 <' 14
25
II
473
_ 825
_ CQ
248
268
R. Blumenhagen et al. / ^-algebras
which contains two fields U and V of dimension 3 and 4, respectively,
[Lm,Un] = (n-2m)Un+m,
(3.27)
[Lm,Vn] = (n-3m)Vn+m.
(3.28)
This algebra can be thought of as the Casimir algebra of SU(4) [11], and we will show that it exists for arbitrary values of the central charge up to some exceptions. The treatment differs from that of the examples 3T(2,8) in that here we have to consider three basic commutators, namely [U, U], [V, V], and [U, V], which apart from the central charge include two more free parameters C\jV and Cyy. With the following notations for the relevant NOPs
/, = 4
3 , A-=^(L,L)=N(L,L)-—d2L,
h=5
3 , A-=jr(U,L)=N(U,L)---d2U,
h = 6 r-=sr(L,d2L)
=N(L,d2L)
A ==./r(/l,L) = N(A,L)
-6N(L,dL)
2 + -d2N(L,L)
1 -
jz&L,
-.-d2A,
a-=jr(V,L)=N(V,L)--d2V,
6 P-*{U,U)-N{U,U)-±*L--t(^*A-^C?lu*V,
2 T»*jr(U,dL)
-N(U,dL)
- -dN(U,L)
1 , + " ^ ^>
( 3 - 29 )
249
R. Blumenhagen el aL / If-algebras
269
these commutators have the general form [^.£41 = ^ ( " 5
)5 n+m ,o + C^P33 2 (m,n)L m + n + C^/7 3 3 4 (m,n)A m+n
+ CuuP3M(m^n)Vm+n, [Kn.K] = \[n
(3.30a)
7 3 )5 n + m ,o + C ^ / ^ m . / O L ^ , , + C^p 4 4 4 (m,«)A m + n
+ C^p 4 4 4 (m,«)K m + n +p 4 4 6 (m,/i)[C^ 1 / r m + n + C ^ 4 m + n + C ? A + n + CyyPm+n + CTyyTm+n\, (3.30b) [Um>K] = CbvP}42(m>n)Lm+n + C^ypw(m,n)Um+n
+
+ C^pM5(m,n)Am+n+piA6(m,n)[c[yrm+n
C^ypw(m,n)Am+n + CflyAm+n
+ C0yiim+n + CZyPm+n + C ^ r m + I I ] . (3.30c) The field V cannot occur in the last commutator, because CyV~ Cyy, which of course vanishes. Furthermore, note that in this example even one of the normal ordered products in (3.29) formed according to the definition given in sect. 2 depends on the structure constant C\jU at this stage. Calculation of the structure constants as before leads to CL
—7
CA —
L —r^ _n % C uv~ ~uv~ u>
cr
=c&
L
Cl/K=2,
=cn
32
5c + 22 ' 3
r"U — ~rv
^uv~
=cp
A
Cyy= —
I'-UU'
=0
cA
*~uv~
cT =
39
—
7,. 4.114
3
4(c +
cv
uu '
cv 2)~uu'
42
, Cyy = 0,
(3.31)
whereas the other Cyy with h(X) = 6 are rather complicated rational functions in C\jV and C£ k , which simplify drastically when the latter are expressed in terms of the central charge c, much as was the case for 3T(2,6). We therefore list these structure constants at the end of the calculations, as well as the determinant of the dimension 6 fields.
250
270
R. Blumenhagen el al. / W-algebras
For consistency of the W-algebra it is necessary and sufficient that all Jacobi identities involving three simple primaries are fulfilled. From general arguments and explicit calculations, however, one can infer that all the restrictions on the parameters of the model are already included in the condition
[[K-.K,m,]+cycUo.
(3.32)
Inserting the commutators (3.30) and the structure constants (3.31) into this equation, after some tedious calculations involving the linear dependencies of the universal polynomials one arrives at the result 16(7c+114)(c + 2) 3(5c + 22)(c + 7) '
2
*
uu
' 2
(C^
=
27(c2 + c + 218)2 (7c + 114)(5c + 22)(c + 7)(c + 2) '
(333a)
with the additional conditions v y CuuCyy
_
~
12(c2 + c + 218) ~ (5c + 22)(c + 7) '
(333b)
(so that there are only two choices of sign in eq. (3.33a)) and C£y*0.
(3.33c)
With these results the missing structure constants read _ ■VV~
rp = Cvy
3(19c-582) iiA\t i\ ' 20(7c +i 114)(c +, 2) '
-,rl/^_
45(5c + 22)
-
.
_ vv *"VV
„
96(9c - 2) (7c + 114)(5c + 22)(c + 2) ' 36(c2 + c + 218)
rn = ——-
,
,_,
rv )
c\ 34^
2(7c + 114)(c + 2 ) ' Lyy (5c + 22)(c + 7)(c + 2){Cyy) '(3J4) and the determinant of (all) the dimension 6 fields introduced in (3.29) again factorizes: c5 det D6 = - —— -(7c + 114)(5c + 22) 6 n 2835(c + 7) ' X(3c + 116)(c + 13)(c + 2 ) 2 ( c - 1).
(3.35)
251 R. Blumenhagen et al. / '^-algebras
271
In conclusion the "Casimir algebra" 2F(2,3,4) exists for all values of c except for the isolated points c = - 2 , - y , - 7 , - -^ and the intervals - ^
(3.36)
of the central charge. On the other hand all the ^"-algebras W(2,5,, 82) with both the dimensions 8, > 2 odd are inconsistent for any value for c. In order to show the non-existence of these examples, one at first easily proves that the two fields U and V of dimensions 5, and 82, respectively, must commute with each other (using formulae like eq. (2.4) one can express all structure constants as multiples of duv and Cyy,Cyy; the latter constants vanish by locality, the former by orthogonality of U and V). This result in turn implies that e.g. the Jacobi identity involving the {/-field twice and the K-field cannot be satisfied (here one has to show essentially that the polynomials ps s 2k(m,n)p2kS s(m + n,q) are linearly independent for 1 < k < 81 - 1), which concludes the proof. 4. Summary and speculations Using a modified systematic framework we were able to set up a general algorithm for the explicit construction of chiral algebras with local fields. Applying this to some simple cases containing two or three generators, we could give a detailed analysis of the algebras W{2,8) for 8 = | to 8. As far as ^-algebras with three generators of integer spin are concerned, we explicitly examined the cases #(2,3,4), which is consistent for generic c, and #(2,4,4), where the parameter c is fixed to take on some special values. As a general result we obtained, that all the iT-algebras with two additional generators of odd dimension are not consistent for any central charge at all. In the following we once more summarize our results concerning the algebras W(2,8). Of course, one would like to discover some systematic pattern underlying the collection of data gained by our calculations. Indeed we will give a few conjectures how to fit the W(2,5)-algebras we found to exist into a general scheme. While there are good reasons for some of our propositions, the other ones are rather heuristic; nevertheless, we shortly present these observations, too, at the end of this section.
252
272
R. Blumenhagen et al. / W-algebras TABLE 2
The c-values for which the algebras W(2,8) exist with vanishing structure constant G w
5T(2, |): ar(2,4): y(2,|): ar(2,5): ar(2,^): ar(2,6): y(2, f ) : ar(2,7):
22'
6 >
8 '
c = 86 ± 60 v/2; 27V! 7 125 c = 25 10 , - 3 5 ; 22 ' ' 26', - 20> 6 c —7 ' - 7 , - ■fF.134±i «h/5;
c - c ■»
217 26 516
;
47,194 ± 112v/2; 9 n 611 in. c —34i 14 ' 10 > 25. c= - ? ' 39 473 825 11 25 C c = 28' 38' 28! 38' 10' 10 > 3344 '■ 16' 16 '
» wT''
-"•
ar(2,8):
At first we list in table 2 the values of the central charge c for which the algebras W{2,8) exist with vanishing structure constant C%w = 0. We also found that 3T(2,8) exists for c = § , - ^ , - - ^ and 350 ± 252v£ with non-vanishing C^w I n addition the algebras ar(2,4), 2T(2,6), and 2T(2,3,4) are consistent for generic central charge, i.e. except for some isolated points and some intervals. The singular points are due to denominator zeroes of the expression for ( C j ^ ) 2 in c, the intervals are forbidden because (C%w)2 would become negative for these c-values. Furthermore, our algorithm shows that as far as W(2,8) is concerned, 5 = 4 and 8 = 6 are the only cases with these properties, besides Zamolodchikov's 2T(2,3) algebra, of course. For higher dimensions 8 the number of conditions encoded in the Jacobi identity is too large for the central charge to remain a free parameter. As the number of linearly independent conditions grows with 5, it may at first sight appear as though 2T(2,8) could not exist at all for 8 large enough. There are, however, some convincing arguments that suggest the following Proposition. If 8 e Z + / 2 admits a decomposition 8 = ( p — 2X<7 - 2)/4, p, q e Z + coprime, the algebra 3T(2,8) exists for c = 1 -6(p-q)2/pq with vanishing structure constant C%w. This conjecture is based on simple fusion algebra considerations: Given a representation of the Virasoro algebra with central charge c contained in the minimal series, the dimensions of the primary fields take on the values (pr-qs)
~(p-q)
h{p,q\r,s)-
,
l-
1<S>-1.
(4.1)
Apq In particular, h{p,q;q1,1) = h{p,q\l,p - 1) = 8, if 8 satisfies the relation of the proposition. As a consequence, according to the fusion rules given by Belavin
253
R. Blumenhngen et aL / IT-algebras
273
et al. [4] one has [ * ] x [ S ] = [l]-
(4.2)
If the representation is unitary, this implies - by general arguments due to Doplicher et al. [12] and Fredenhagen et al. [13] - that the corresponding parafield V of dimension 8 yields an automorphism of the fusion algebra (according to some recently proposed terminology it is "anyonic" [14] or a "simple current" [15]). The operator describing the relation of V(x)V(y) to ViyWix) commutes with all of the operator algebra and hence is a scalar. Thus IP can be added to the algebra of local fields, if S e Z + / 2 . The arguments found in ref. [15] strongly indicate that the theorems in refs. [12,13] can be extended to non-unitary situa tions, which would imply the proposition given above. We list the c-values which can be explained by this proposition plus two apparently related ones in table 3. Here the columns are labeled by the pair (r,s) = (l,p - 1) occurring in eq. (4.1); for the c-values in the table we use the notation (p,q) = c. This means that for c given by the (p, q)th element of the minimal series and for 8 = h(p,q;l,p - 1) the algebra W{2,8) exists with vanish ing structure constant C^,w. The entries marked by * on table 3 are c-values which fulfill all the conditions of the proposition except for p and q being coprime. In general, however, this restriction cannot be omitted (e.g. 3T(2,8) does not exist for c = (4,18)=-f). A considerable number of the c-values showing up in table 2 (and additionally c = - -}f from 3T(2, f), see ref. [1]) can be explained by the proposition. There are
TABLE 3
The c-values which would be explained by the proposition in this section plus two apparently related ones. For notation and labelling see the text. (1.2) ar(2,?): ar(2,3): 5T(2,?): ar(2,4): ar(2,|): 2T(2,5):
ar(2,V): ar(2,6): ar(2, -£): 5T(2,7): 2r(2,-£): ST(2,8):
(1,3) (4,7)= - H if1
(4,9)= - £
((3,20) 3 , 2 0=) = - ^10 ( 3 , 2 2 )== - f350 (3,22) i?i
(4,11)= - f (4,12)= -T
(3,16)
(1,4)
(1,5)
(1,6)
(5,8)(6,7) =
(4,13)=-£ (3,26) = 516 13 611 (3,28) = - <$■ 14
(4,15) = - -ft
((3,32) 3 , 3 2=) = -825 ^ 16
(4,17)- - f
2
(3,34) =
<M4 17
(5,12)=-$
(7,8) = §
254
274
R. Blumenhagen et al. / If-algebras TABLE 4
The c-values not explained by the proposition in this section ar(2,i): ar(2,l): ar(2,^): ar(2,^):
(12,11)= % (12,13)=| (12,17)=£ (12,19) -^
four more cases of ST-algebras with the central charge contained in the minimal series, but with S # h(p, q; 1, p - 1), as shown in table 4. Remarkably, in all these cases the dimension of the additional generator of the 3T-algebra is given by S = h(p,q;l,5). Both this pattern and the one arising from the proposition can be revealed in the ADE-classification of modular invariant partition functions by conformal characters due to Cappelli et al. [16]. In table 5 non-trivial examples are shown that may be related to the ADE series (we use the notation hip, q; r, s) introduced in eq. (4.1); the central charge of course is contained in the minimal series and given by c = (p,q) with p, q coprime. The labelling of the rows by pairs of Lie algebras is as in ref. [16]. To be more specific, let us assume that the characters mentioned above arise in RCFT. Then their chiral field content can be read off due to the isomorphism between the vector space of fields and the Hilbert space. Let the CappelliItzykson-Zuber character be written as L
^.r-.sXr.iX*,,-,
(4-3a)
with non-negative integers ■^"r,J,,-iJ- Then the generating function of the vector space of chiral fields is given by Z-L-^r.s.l.lXr.,-
TABLE 5
The patterns, which may be related to the ADE-classification (A,_„D2„): (A,_„E6):
h(4n - 2,q; l,4n - 3) = (q - 2Xn - 1) «12 > < ? ;l,7) = <7-3
h(U,q-\,5)={(q-4) (A,_„E8):
M30,<7;l,ll) = <7-5 /i(30,;l,19) = 3(-3) /i(30,
(4-3b)
255
R. Btumenhagen el al. / H'-algebras
275
Since simple fields have to be primary apart from the Virasoro field, the number of simple fields is at most E r s.^r s ,,,. J^-algebras with 2 generators in the most obvious way are given by the series (Ax s are listed in the first two rows of table 5. The (A.q_],D2n) series exactly reproduces the c-values and dimensions 8 that can be derived from our proposition. For the choice q = \l the exceptional series (Aq_ |, E6) yields the value c = \\ with h = 8: indeed W(2,8) exists for this central charge with non-vanishing structure constant C^w. There are other W(2,5)-algebras hidden in the ADE-classification of conformal partition functions: Consider the (A,_,,E 8 ) series which partition functions con tain the term [y,, + X\,u +*i,!9 + X\,2<>\2- At first sight, this seems to correspond to a ^-algebra with four generators with conformal dimensions as in table 5. However, consider the primary <£, n of dimension q - 5; the commutator of <£, ,, with itself cannot contain the fields <£, 19 and >, 2q as the latter have too high dimensions. Therefore, '#'(2,8) with 8 = M30, q; 1,11) already is a closed subalgebra. These considerations e.g. allow us to fit the example of W(2, 8) with central charge c = - ™ = (30,13) into the ADE-classification. The other fields
*<2):=*1.4+*|.8>
*<3>:=*1.5+*l.ll>
(4-4)
may be regarded as characters of irreducible representations of the 3T(2,5 ^-alge bra. The corresponding dimensions of the primary fields are the lower ones appearing on the r.h.s. [15]. The three representations yield a fusion algebra of Ising type [21], which means that [<£li5] X [<£, 5] = [$, ,] = [1]. As has been argued in the context of the proposition, this property ensures that 2T(2,8X) can be extended by the field <£, 5 having conformal dimension 82 = (q - 4)/2. Because of dimensional arguments like those in the last paragraph [4>U5, <£, 5 ] does not contain the field with dimension 8U so <j>5 , generates a closed sub-2T-algebra. An example is provided by the algebras W(2,\) and W(2,8), which both share the central charge c - (12,11)= § , with | = A(12,11;1,5) and 8 = M12,11; 1,7). Pre sumably, the field <£, 7 is composite, such that
256
276
R. Blumenhagen et al. / IT-algebras
These considerations enable us to give some interpretation of all the values of the central charge found in sect. 3 except for the two cases in table 3 where p and q are not coprime. Of course they cannot explain the examples of 3T-aIgebras with c not contained in the minimal series, namely the negative integers (which "obviously" satisfy c = 1 - 85 for 8 = 3k/2) and the irrational c-values, as well as c= - ^ f o r ar(2,8). Other observations worth noting concern the connection of 2T-algebras with semisimple compact Lie algebras. Considerable effort has been made in construct ing 2T-aIgebras from Casimir operators of Lie algebras; e.g. Zamolodchikov's 3T(2,3) could be interpreted as the Casimir algebra of A(]> [11,17], and 3T(2,3,4) constructed in sect. 3 is likely to correspond to A(j} in an analogous way. Besides that, most of the values of the central charge collected in table 2 prove to be elements of the discrete series derivable from Kac-Moody algebras by the coset construction [18] or by means of BRST cohomology [20]. To be specific, the values c = — ^ j and -47, for which 3T(2,6) exists with vanishing C^w> appear in the series of the exceptional Lie algebra G2 [20] (3p2 + q2\ c c / p , * ) = 194-56 — — .
(4.5)
for (p,q) = (13,4) and (8,7), respectively, thereby confirming the connection of W(2,6) with this Lie algebra, which was already assumed in ref. [5]. The c-values - ^ , - 7 , and § of 3T(2,5) show up in the E 6 series (cf. e.g. ref. [20]) c E 6 ( P . g ) = 6 1-156 V ^
,
(4.6)
for (p,q) = (11,9), (8,9), and (13,14). Finally, c = - ^ belonging to 3T(2,8) is a member of the Eg-series [20] cE8(p,g)=8 l - 9 3 0 ( f 7 ^ g )
.
(4.7)
Furthermore, the values of the central charge listed in the first two columns of table 3 are given by a simple pattern when connected with the discrete series of the Lie algebras Dn and B„ /
(P-Q)2\
\
PQ J
cD„( P, 9) = n 1 - (2n - l)(2n - 2)
,
(4.8)
2n + l / (p-qf\ cBa(p,q) = —j—\\-2n(2n-l)KypJJ ,
(4.9)
257
R. Blumenhagen el al. / &-algebras both of which can be derived using the coset construction. The first of them reproduces all the c-values of the bosonic 3T-algebras listed in table 3 by the formula c = cD(28 + 1,28 - 2) for the 0 , s ) = (1,2) column and by the formula c = cD(28 + 2,28) for the (/-, s) = (1,3) column, with the constraint that p and q are coprime. The fermionic 2T-algebras are connected with the B„-series (4.9) (corresponding to the so called WB„ models containing a fermionic generator [19]) by the same equations only with D g replaced by B 5 . (Note that this scheme cannot be extended to the other columns of table 3. In fact, one observes that naive continuations like c = cB(28 + 3,28 + 2) for the (r,5) = (1,4) column would lead t o o 1.) Also both c-values 1 and - 7 7 , for which W(2,4,4) appears to exist, can be found in the cD< series for (p, q) = (8,7) and (11,6). Note, however, that the latter does not belong to the minimal series. This concludes our attempts to reveal some general patterns hidden in the variety of consistent ^-algebras constructed in this paper. Our results indicate that still some new underlying structures remain to be discovered, before a complete classification of conformally invariant quantum field theories in two dimensions can be achieved. Appendix A Here we present the structure constants C^,w appearing in the commutator of the simple primary field with itself that were left out in sect. 3. The determinants of the (d, ; )-matrices are listed, too. At first we consider the structure constants of those NOPs X built up from the energy momentum tensor only. For the simpler cases (up to d(X) = 12) we give general formulae valid for any integer or half-integer spin 8 of the local primary field W (the notations of the NOPs are as in sect. 3): 2
2(55 + 1) 5c+ 22 ' 4(70c52 + 42c5 + 8c + 2952 - 57S - 2) 3(7c + 68)(5c + 22)(2c- 1) ' c(145+ 1) + 4 ( - 2 8 5 2 + 1 4 5 - 1) 10(7c + 6 8 ) ( 2 c - l )
'
rE[ = 2(1050c253 + 1260c252 + 606c2S + 108c2 + 3305cS3 - 498c52 - 701cS + 78c '"WW
-2515 3 + 9185 2 - 8295 - 6)/(3(7c + 68)(5c + 22)(5c + 3)(3c + 46)(2c - 1)),
277
258
278
R. Blumenhagen el al. / 7-algebras
C*?w= (9450c352 + 3915c35 + 495c3 - 84000c253 + 108090c252 + 35688c25 +2214c2 - 699640c53 + 315636c52 + 83332c5 - 11136c +13895253 - 32313652 + 921685 - 3408)/ (65(7c + 68)(5c + 22)(5c + 3)(3c + 46)(2c - 1)), Cffw=
(351c25 + 13c2 - 10824c52 + 2616c5 - 304c + 64944S3 - 64944S2 + 81005 + 300)/(2184(5c + 22)(5c + 3)(3c + 46)),
Cww= 4(H550c25" + 23100c253 + 20130c252 + 8580c2S + 1440c2 + 76675c54 + 30590c53 - 25615c52 - 10898c5 + 1608c + 37675" - 1841053 + 29929S2 - 163425 - 24)/ (15(llc + 232)(7c + 68)(5c + 22)(5c + 3)(3c + 46)(2c - 1)), CTww = (6756750c353 + 6467175c352 + 2477475c35 + 356850c3 - 63848400c25" + 86945550c253 + 79785285c252 + 24855285c25 + 2903130c2 -830808800c5" + 268022180c53 + 193729070c52 + 21080734c5 - 7908564c - 1068283365" + 40639168053 - 41980083252 + 692411365 - 1159008)/ (5525(llc + 232)(7c + 68)(5c + 22)(5c + 3)(3c + 46)(2c - 1)), C$w = 11( 1327326c"52 + 442442c"5 + 40222c" - 39543504c353 + 21742409c352 + 5245695c35 - 285350c3 + 242361504c25" - 815400232c253 + 86867386c252 + 10459358c25 - 10811636c2 + 3567648432c5" - 4094600240c53 + 377225760c52 + 212182112c5 + 1419456c + 10706037125" - 290591846453 +155561760052 - 486597125 - 7462656)/ (315588(llc + 232)(7c + 68)(5c + 22)(5c + 3)(3c + 46)(2c - 1)),
259
R. Blumenhagen el al. / M-algebras
279
CJ-V = (12716c35 + 289c3 - 753610c252 + 189618c2S - 12818c2 + 12944360c53 -9486620c52 + 1609652c5 + 115168c - 6213292854 + 10355488053 -32768736S2 - 21482565 + 147840)/ (624240(llc + 232)(7c + 68)(5c + 22)(2c - 1)) , Cww = 4(10510500c455 + 31531500c454 + 42942900c4S3 + 31891860c462 + 12478440c45 + 1990080c4 + 151698400c355 + 231672000c354 + 126000160c353 + 34839360c352 + 20447680c3S + 8687040c3 + 424911495c255 + 157754085c254 - 92863605c253 - 168268389c252 - 103609386c25 + 3352680c2 -265783494c55 - 450378930c54 - 26055378cS3 + 294358674c52 - 40873272c5 -7518960c + 1944543555 - 10629577554 + 21901515553 - 20603206552 + 752322505 + 21000)/(45(13c + 350)(llc + 232)(10c - 7)(7c + 68) X(7c + 25)(5c + 22)(5c + 3)(3c + 46)(2c - 1)), C%2W = 2(34842307500c554 + 59231922750c553 + 44000856900c552 + 16136060850c55 + 2372479200c5 - 342726384000c455 + 565265268750c454 + 1075329070725cV + 717389089170 c 4 5 2 + 239285155005c4S + 34685264610c4 -7538849105200c355 + 1952706509100c354 + 4984892219645c353 + 2292930169620c352 + 441103497785c35 + 32812050630c3 - 26815279119960c25 + 15264944069070c254 + 3795745213740c253 - 3048884405958c252 -463196226492c28 - 173333391840c2 + 12692405604432c55 + 7067903625540c54 - 7097975933316c53 - 6660045737172c52 + 666606742716c + 102598373880c - 254422045268055 + 1208588226420054 - 1942629242084053 +1137516486732052 - 10282469780005 + 7112112000)/ (116025(13c + 350)(llc + 232)(10c - 7) X (7c + 68)(7c + 25)(5c + 22)(5c + 3)(3c + 46)(2c - 1)),
260
280
C{fw=
R. Blumenhagen et al. / V-algebras
ll(62525217654900c653 + 51621805315080c652 + 16788193610370c65 + 2014387947390c6 - 1810748216877600c5 5" + 973148326053540c553 + 970487535774120c552 + 218172425597490c55 + 5400924162270 c 5 + 11202949599441600o"55 - 52858561112113120c"5" - 2306331794316095c"53 + 4120421887189192c"52 - 648415024519327c"5 - 622922099143350c4 + 275681687174434240c3S5 - 461362577268547480c35" -21728772639878161c353 + 39397687697427376 c 3 5 2 + 8368360374287475c3 5 -2456055610188870c3 + 1139142210190016400c255 - 1592265068539111560c25" + 141716930635877316c253 + 151587930775927560c252 + 50652798065961684c25 - 1679464598020440c2 - 407023631420243280c55 + 314758976762479840c5" + 337243620862323956c53 - 237346013672695168c52 + 19207659638712052c5 + 412932494931960 c + 19628593971616544055 -7850622845401136005" + 93307210382408272053 - 29312153262986656052 -64660184659080005 + 687818583144000)/ (16999147620(13c + 350)(llc + 232)(10c - 7)(7c + 68) X(7c + 25)(5c + 22)(5c + 3)(3c + 46)(2c - 1)),
C%w= 13(937124O628750c752 + 2619934419375c75 + 184479616125c7 - 568895280203250c653 + 241268992097175c652 + 45113983872825c65 - 4346343142050c6 + 9713029013688000c55" - 20664219824596950c553 + 2254250549614665c552 + 289347319625910c55 - 129347583717975c5 - 47051751963216000c"55 + 334320857983277200c"5" - 259025979565647490c"53 + 18061888249155854c452 + 7098251137660936c45 + 821588705249700c" - 1241717541570150400c3S5 + 3405451004673718480c35" - 1570458816193888262c353 - 28610596065407308c3 - 11827044806522310c35 + 8505184708273080c3 - 5786039707661010240c255 + 11351962731680349600c25" - 4243137120727296648c253 - 1675105657303560c2 - 213692380098872352c25 + 17037206423628720c2 + 983406641873444160c55 - 1273624839893033920c5" - 2534357186202133448c53 + 2591835090375552544c. - 307941078997862536c5 - 8318174966831280c - 158922489371552192055 + 52424289470414048005" - 460413877185688096053 + 91814300557321408052 + 681637071353040005 +544184525808000)/ (235372813200(13c + 350)(lie + 232)(10c - 7)(7c + 68) X(7c + 25)(5c + 22)(5c + 3)(3c + 46)(2c - 1)) ,
261
R. Blumenhagen et at. / V-algebras
281
C*jfw= 1573(36117900c652 + 11816350c65 + 737450c6 - 1273490400c553 + 855356250c552 + 291291525o55 - 1951425c5 + 15801676800c"5" -28494930800c"53 + 6870682630c"52 + 3696868245c"5 - 32703125c" - 632067072O0c355 + 249542048000c35" - 191668287720c353 -4267268304c352 + 16906072224c35 + 112397800c3 - 366101120000c255 + 734705825920c25" - 207180847288c253 - 126388015064c2S2 + 17894983732c25 + 814320420c2 + 722187896320c55 - 1781248255040c5" + 989104O21024c53 - 12148512672c52 - 22068918032c5 - 1602673360c - 9688594304055 + 2422148576005" - 6732419152053 - 6551847104052 + 125969880005 + 38589600 (1291483200(13c + 350)(10c - 7)(7c + 68)(7c + 25)(5c + 22) X(5c + 3)(3c + 46)(2c-l)), Cwbw = (3177037500c75 + 48877500c7 - 252785169000c652 + 117226791500c65 -2085513500c6 + 7673916705000c553 - 7492652622000c552 + 2046880938375c55 + 34279154175c5 - 93664439232000c4S" + 183825617912300c"53 - 89096209659730c"S2 + 11164732258680c"5 + 188149250450c" + 374657756928000c355 - 1581056007003200c3S" + 1471363718271720c353 - 376908839503326c352 + 27253417307181c35 - 1302922369225c3 + 2577646458732800c255 - 6416356418761120c25" + 3913093480685428c253 - 605501321890816c252 + 75635627033408c25 -7007418064620c2 - 111038912283520c55 + 2811389054240c5" + 1323491550801056c53 - 1224608924054568cS2 + 161985946905692c5 + 2348323852660c + 109914356661824055 - 274785891654560054 + 184557573397912053 - 270616671513760S2 - 157413107280005 - 1376886126000)/(15484392000(13c + 350)(10c - 7)(7c + 68) X (7c + 25)(5c + 22)(5c + 3)(3c + 46)(2c - 1)),
262
282
R. Blumenhagen el al. / IT-algebras 5 3
C{FW= - ll(20065500c S + 13185900c5S2 + 3774225c5S + 569625c5 -290472000c4S4 + 504871500c4S3 + 299373060c4S2 + 52668315c4S + 8714475c4 + 1161888000c3S5 - 6373572800c354 + 3155756660c3S3 + 2111923292c3S2 - 85869152c35 - 459600c3 + 138754112O0c2S5 -25403817760c2S4 - 3046054476c253 + 8505215872c282 - 711181736c25 - 104314260c2 - 37138840960c55 + 92727669920c54 - 54466694352c53 + 4093479856c52 + 192858736cS + 83207280c + 47772992055 - 119432480054 - 137222504053 + 413907392052 - 8872740005 + 17892000)/ (86184(13c + 350) (10c - 7) (7c + 68) X(7c + 25)(5c + 22)(5c + 3)(3c + 46)(2c - 1)) . For the fields Fl to F10 the general expression would be very involved, so we merely list the structure constants for the specific cases 5 = -y C£'„,= 39(2359943586000c5 + 51173171404868c4 + 340912309262668c3 + 640887368914519c2 - 313556935313290c - 42224581678125)/ (56(13c + 350)(llc + 232)(10c - 7)(7c + 68)(7c + 25)(5c + 164) X(5c + 22)(5c + 3)(4c + 21)(3c + 46)(2c - 1)), Cww = 9(3133997040643560c6 - 97484045298492762c5 - 553901864734350121 lc4 -51723474943503509770c3 - 124400417420454072277c2 + 26288195794834712500c + 16861409939530695000)/ (166600(13c + 350)(llc + 232)(10c - 7)(7c + 68)(7c + 25) X(5c + 164)(5c + 22)(5c + 3)(4c + 21)(3c + 46)(2c - 1)), C £ V = 11(227187548329116466000c7 - 35896929829553560325740c6 + 184749240288090677370808c5 + 47654857491521959127517959c4 + 559996103353161517469981515c3 + 1583347939869890158138436198c2 + 29292999188811471380012700c - 391379250817682248905630000)/ (1231157340000( 13c + 350)(llc + 232)(10c - 7)(7c + 68)(7c + 25)(5c + 164) X(5c + 22)(5c + 3)(4c + 21)(3c + 46)(2c - 1)) ,
263
R. Blumenhagen et at / jr-algebras 8
283 7
C £ V = 169(7336408998043125000c - 3006969965871552889250c
+255887754408918814512995c6 + 2118829903377813533573071c5 -304345071877948707161317492c4 - 4321855266729027400863538070c3 - 14025378160071730007080085374c2 - 4042501493258563662114635100c + 5656830001031651892967440000)/ (277010401500000(13c + 350)(llc + 232)(10c - 7)(7c + 68)(7c + 25)(5c + 164) X (5c + 22)(5c + 3)(4c + 21)(3c + 46)(2c - 1)), Ctfw = 221(63567810556250000" - 3334793702151931250c8 + 623187741463767445875c7 -32501817341822722663035c6 - 729265566934696236048828c5 + 37043279866419767653935081c4 + 650813212550699015551363135c3 + 2387286051119854483786974182c2 + 1235081330296370937897811800c -1581443358512676279348420000)/ (273353850000000)(13c + 350)(llc + 232)(10c - 7)(7c + 68)(7c + 25) X(5c + 164)(5c + 22)(5c + 3)(4c + 21)(3c + 46)(2c - 1)), Cww=
(1859(1325943512075000c8 - 259791002321110750c7 + 12419633794980565405c6 + 297871147951201653899c5 - 14223897085672936659698c4 -245135327077531487561830c3 - 659854202731194444477556c2 + 352633144071551625915600c + 293547680582716458360000)/ (268226O000O0(13c + 350)(llc + 232)(10c - 7)(7c + 68)(7c + 25)(5c + 164) X(5c + 22)(5c + 3)(4c + 21)(3c + 46)(2c - 1)),
ChwW=
- 143(419087890312000c7 - 17759806193312680c6 - 604800943776287594c5 + 20077307331023874713c4 + 478361292238382405605c3 + 1046778016065289168886c2 -2511117369495575073600c -102686703366638160000)/ X(20286000( 13c + 350)(llc + 232)( 10c - 7)(7c + 68) X(7c + 25)(5c + 164)(5c + 22)(5c + 3)(4c + 21)(3c + 46)(2c - 1)) ,
264
284
ft
Blumenhagen et at. / V-algebras 6
C£V= 37349( 13346375000c - 6160525738750c5 + 903704483593275c4 -48015817324111616c3 + 395309483740127902c2 + 17647757568618354540c + 16576716950134867944)/ (40470570000000(llc + 232)(7c + 68)(5c + 164) X (5c + 22)(5c + 3)(4c + 21)(3c + 46)(2c - 1)) , Cww= ~ 2197(2550692500c5 - 624082821775c4 + 29161355582681c3 + 2611338018418c2 - 15730757515970640c - 2753618390987904)/ X(1352400000(llc + 232)(7c + 68)(5c + 164)(5c + 22)(5c + 3) X(4c + 21)(3c + 4 6 ) ( 2 c - l ) ) , C£'£ = (2158406250000c7 - 1569406489000000c6 + 452693030892665000c5 -61199911253845544775c4 + 3344419441862024469076 c 3 -29553220803125349665522c2 - 1203808534230505935011940c - 2551279778385831780706584)/ (1004157000000000(llc + 232)(7c + 68)(5c + 164) (5c + 22)(5c + 3)(4c + 21)(3c + 46)(2c - 1)) , and 8 = 8: C £ V = 128(91445760000c5 + 2005172427780 c 4 + 13477701650146 c 3 + 25580576270581c2- 12168172573312c - 1776514109755)/ (5(13c + 350)(llc + 232)(10c - 7)(7c + 68)(7c + 25)(5c + 164) X(5c + 22)(5c + 3)(4c + 21)(3c + 46)(2c - 1)) , C(?w= 24(368789367623040c6 - 13272918610341138c5 - 714431962645911483c4 -6655284624931140182c3 - 16056938689641266927c2 + 3229184503942094138c + 2267161773925952120)/(38675( 13c + 350)(llc + 232)(10c - 7)(7c + 68) X(7c + 25)(5c + 164)(5c + 22)(5c + 3)(4c + 21)(3c + 46)(2c - 1)) ,
R. Blumenhagen el al. / "T-algebras
C£V=
22
7
285 6
( 8429886221486548000c - 1450117540255367555845c
+ 12450935334999994852264c5 + 2100745527675011644894139c4 + 24366042991472498065865834c3 + 68778896274167258910142824c2 + 1714341256447406389451600c - 17508171981846090427960000)/ (71451095625(13c + 350)(llc + 232)(10c - 7)(7c + 68)(7c + 25) X (5c + 164)(5c + 22)(5c + 3)(4c + 21)(3c + 46)(2c - 1)), C £ V = 13(4109012749616906250c8 - 1810928778108565080875c7 + 169813103113358840285885c6 + 829714935130333038130813c5 -219531868554928579737941437c4 - 3040581883464172115485301872c3 -9816121805901929768336507292c2 - 2858100134658922374777950800c + 4039492842904990518536720000)/ (9893228625000(13c + 350)(llc + 232)(10c - 7) X(7c + 68)(7c + 25)(5c + 164)(5c + 22) X (5c + 3)(4c + 21)(3c + 46)(2c - 1)) , C ^ = 17(20107552657500000c9 - 11350214945322356250c8 + 2292388265328643521375c7 - 134319514507859476517330c6 -2440727893123252094878579c5 + 165007101270210393321243796c4 + 2778187386828663546213881276c3 + 10100432541489252097163445136c2 + 5212094677083496462594006400c - 6752737954563351469340160000)/ (58575825000000(13c + 350)(llc + 232)(10c - 7)(7c + 68)(7c + 25) X (5c + 164)(5c + 22)(5c + 3)(4c + 21)(3c + 46)(2c - 1)) , C £ V = (l43(2227778806706250c8 - 476695567460119875c7 + 25862058192620658820c6 + 503388209486376675041c5 - 31755904984269362232584c4 -523037921426780745492004c3 - 1397187195528289891518944c2 + 732172673178464427694400c + 627503309112307266240000)/ (28738500000(13c + 350)(llc + 232)(10c - 7)(7c + 68)(7c + 25) X (5c + 164)(5c + 22)(5c + 3)(4c + 21)(3c + 46)(2c - 1)) ,
266
286
Cww=
R. Blumenhagen el al. / 3> -algebras
- H ( 124567589888000c7 - 6227646229664195c6 - 176215043804331091c5 + 7659990866651865034c4 + 169595574466767553204c3 + 367189243038948207144c2 - 871498053300802306400c -36760007924067680000)/(362250(13c + 350)(llc + 232)(10c - 7)(7c + 68) X (7c + 25)(5c + 164)(5c + 22)(5c + 3)(4c + 21)(3c + 46)(2c - 1)) ,
Ctfw = 2873(3516515625c6 - 1743411558125c5 + 276276982996100c4 - 16058544419599884c3 + 164640240348191616c2 + 6291381812392465696c + 5880201255012475776)/(722688750000(llc + 232)(7c + 68)(5c + 164)(5c + 22) x(5c + 3)(4c + 21)(3c + 46)(2c - 1)), C$?w=
- 169( 1430836875c5 - 377805233325c4 + 19722667013888c3 - 46410795951612c2 - 11213587570166672c - 1963323873071232)/ (48300000(llc + 232)(7c + 68)(5c + 164)(5c + 22) x(5c + 3)(4c + 21)(3c + 46)(2c - 1)),
C&ft = (2137652343750c7 - 1666948023453125c6 + 516054344820024375c5 -75080948526515245900c4 + 4468473911116490862196 c 3 -48396438460468019226304c2 - 1720931142127477307541824c - 3614806316012588147641344)/ (932431500000000(llc + 232)(7c + 68)5c + 164) (5c + 22) X(5c + 3)(4c + 21)(3c + 46)(2c - 1)) .
267
R. Blumenhagen et at. /
^-algebras
287
The structure constants Cfcw where A" is a NOP containing the primary field W are as follows: For 5 = 6 we have
ww
~
p Cww=
186 13C+156 ""*" 12(572c + 2089)
w
5(13C + 516)(C + 47)(C + 2 ) C H ' H "
9( 13c -694) 260(c + 47) (c + 2)
Wlt
whereas for S = 8 these structure constants are given by Cn
=
328 17c + 944 ll(83c-5886)
CH,H/
17(95C + 434)(C + 6 3 )
ww
'
24(12821c +81283) C w
"
=
(95C + 434)(17C + 944)(C + 6 3 )
w CM
'H"
32(4534920c3 + 127199201c2 + 754656049c - 359112082) 7(2c2 + 179c + 2702)(95c + 434)(17c + 944)(5c - 4)(c + 63) Cl2w= (3(356435345c4 + 3868519779c3 - 1559203697776c2 -29729418486796c - 10503032893136)/ X (5950(2c2 + 179c + 2702)(95c + 434)(17c + 944)(5c - 4)(c + 63))C%„ , /-T3
13(27053c2 - 1099746c + 20978776) 1 ' rw 770(2c2 + 179c + 2702)(17c + 944)(5c - 4)
T4 Cww=
13(11400c3-3373333c2 + 97401306c+ 3386315464) 119700(2c2 + 179c + 2702)(17c + 944)(5c - 4)
w ww
'
Finally, we list the determinants of the (rf,y)-matrices, which occur in the examples considered in sect. 3. As fields of different conformal dimension are of course orthogonal, these matrices are block-diagonal. Furthermore, all NOPs built
268
288
R. Blumenhagen et ai / Tf-algebras
up from the energy momentum tensor only have vanishing dtj with those contain ing the primary field W once. Therefore the determinant det Dd splits into the two corresponding factors det Dd = det DdL) det DdW), in obvious extension of the notation used in the example 3^(2,4) in sect. 3. The values of the first factors are det D
det Dft> =
211507200 3 2 2 2 9 2 4 2 Q 7 c'(5c + 22) (2c - l) (7c + 68) (5c + 3)(3c + 46)(llc + 232) , 14051203676022767616000
det D\? = 12
det D( ' =
,
.
,
,
c o^^^„ (5c + 22)5(2c - l) 4 (7c + 68)3(5c + 3) 2 v 111162825525037 ' v ' K ' v ' 2 X(3c + 46) (llc + 232)(13c + 350)(10c - 7)(7c + 25) ,
12921366003008049614690713058807277158400000000000
14
17901007737389769326194282279
„ c (5c + 221 V
'
X(2c - l) 6 (7c + 68)5(5c + 3)4(3c + 46) 3 (llc + 232)2(13c + 350) X(10c - 7)(7c + 25)(5c + 164)(4c + 21) . (The numerical factors in these expressions are built up from surprisingly small primes; cf. the analogous phenomenon in the case of 2T(2,8).) The second factors of course depend on 5. For 3^(2,4) they are given by c(c +24) detD*14" g , in the case 3T(2,6) by del D^> = ^-(13c 156
+ 516),
5c2 det DW = ^ ( W e + 516)(c + 47)(c + 2),
269
R. Blumenhagen el a I. / A'-algebras
289
and for >T (2,8) they read c
d e t D ^ — (17c+ 944), det D
W = T ^ 7 7 ( 1 7 c + 944)(95c + 434)(c + 63), 17556
12c4 det D ' f = ^ ^ ( 17c + 944)2(95c + 434)(c + 63)(5c - 4) X(3c + 46)(2c 2 + 179c+ 2702).
References [1] A.B. Zamolodchikov, Theor. Math. Phys. 65 (1986) 1205 [2] J. Balog, L. Feher, P. Forgacs, L. O'Raifeartaigh and A. Wipf, preprint DIAS-STP-89-31; A. Bilal and J.-L. Gervais, Nucl. Phys. B318 (1989) 579 [3] E. Witten, Commun. Math. Phys. 122 (1989) 351; M. Kontsevich, preprint CPT-88/P.2189 [4] A.A. Belavin, A.M. Polyakov and A.B. Zamolodchikov, Nucl. Phys. B241 (1984) 333 [5] P. Bouwknegt, Phys. Lett. B207 (1988) 295 [6] K. Hamada and M. Takao, Phys. Lett. B209 (1988) 247; [Erratum: B213 (1988) 564] [7] D.-H. Zhang, Phys. Lett. B232 (1989) 323 [8] J.M. Figueroa-O'Farrill and S. Schrans, preprint KUL-TF-90/11 [9] W. Nahm, Proc. Trieste Conf. on Recent developments in conformal field theories, Trieste, October 1989; Proc. 3rd Regional Conf. on Math. Phys., Islamabad, 1989; W. Nahm, Conformal quantum field theories in two dimensions (World Scientific, Singapore), to be published [10] P. Bouwknegt, preprint CTP-1665 (1988) [11] F.A. Bais, P. Bouwknegt, M. Surridge and K. Schoutens, Nucl. Phys. B304 (1988) 348, 371 [12] S. Doplicher, R. Haag and J.E. Roberts, Commun. Math. Phys. 23 (1971) 199; 35 (1974) 49 [13] K. Fredenhagen, K.H. Rehren and B. Schroer, Commun. Math. Phys. 125 (1989) 201 [14] F. Wilczek, Phys. Rev. Lett. 49 (1982) 957 [15] A.N. Schellekens and S. Yankielowicz, Nucl. Phys. B327 (1989) 673 [16] A. Cappelli, C. Itzykson and J.-B. Zuber, Commun. Math. Phys. 113 (1987) 1 [17] A. H. Diaz and J.M. Figueroa-O'Farrill, preprint KUL-TF-90/10 [18] P. Goddard, A. Kent and D.I. Olive, Phys. Lett. B512 (1985) 88; Commun. Math. Phys. 103 (1986) 105 [19] G M T . Watts, preprint DAMPT 89-39 [20] J.M. Figueroa-O'Farrill, preprint KUL-TF-90/12 [21] M. Caselle and G. Ponzano, preprint DFTT 8 / 9 0
270
Reprinted with permission from Nuclear Physics B, December 1993 (38 pages) © 1993 Elsevier Science Publishers B. V. (North-Holland)
ITP-SB-93-84 BONN-HE-93-49 December 1993 hep-th/9312049
A class of W-algebras with infinitely generated classical limit J. de Boer 1 , L. Feher 2 '* and A. Honecker2 1
Institute for Theoretical Physics State University of New York at Stony Brook Stony Brook, NY 11794-3840, USA 2
Physikalisches Institut der Universitdt Bonn Nussallee IS, 53115 Bonn, Germany
Abstract There is a relatively well understood class of deformable W-algebras, resulting from Drinfeld-Sokolov (DS) type reductions of Kac-Moody algebras, which are Poisson bracket algebras based on finitely, freely generated rings of difFerential polynomials in the classical limit. The purpose of this paper is to point out the existence of a second class of deformable W-algebras, which in the classical limit are Poisson bracket algebras carried by infinitely, nonfreely generated rings of difFerential polynomials. We present illustrative examples of coset constructions, orbifold projections, as well as first class Hamiltonian reductions of DS type W-algebras leading to reduced algebras with such infinitely generated classical limit. We also show in examples that the reduced quantum algebras are finitely generated due to quantum corrections arising upon normal ordering the relations obeyed by the classical generators. We apply invariant theory to describe the relations and to argue that classical cosets are infinitely, nonfreely generated in general. As a by-product, we also explain the origin of the previously constructed and so far unexplained deformable quantum W(2,4,6) and W(2,3,4,5) algebras.
* An Alexander von Humboldt Fellow. On leave from Bolyai Institute of Szeged Univer sity, H-6720 Szeged, Hungary.
271
0. Introduction The classification of extended conformal algebras (also called W-algebras, or local chiral algebras) is a key ingredient to the classification of two-dimensional rational conformal field theories, which apart from being interesting in its own right is also interesting since it is related to problems in statistical physics, string theory and integrable systems. The experience accumulated so far (see [1] for a review) shows that W-algebras come in two varieties. Firstly, there exist 'deformable' (or 'generic') W-algebras for which the structure constants are continuous functions — with isolated singularities — of the Virasoro centre c for a fixed field content, i.e., for a fixed conformal weight spectrum of generating fields. Secondly, there exist also 'nondeformable' (or 'exceptional') W-algebras that appear only at particular, isolated c values. It is generally believed that, with notable exceptions, the nondeformable W-algebras can be understood in terms of the deformable ones, for instance they could occur in particular minimal models of deformable W-algebras. Most deformable W-algebras considered so far result from Drinfeld-Sokolov (DS) type Hamiltonian reductions of affine Kac-Moody algebras, and thus have a classical limit which is a Poisson bracket algebra carried by a differential polynomial ring generated by a finite number of independent generating fields. To put it differently, a class of deformable quantum W-algebras exists to which those algebras belong which admit a finitely, freely generated classical limit. It appears that this class of W-algebras is by now reasonably well understood (see, e.g., [2-5] and references therein), though a lot of work remains to be done before we will have it completely catalogued. However, there are a number of reasons for believing that the above mentioned class does not exhaust the deformable quantum W-algebras. We have such indications in the context of each three methods usually used for obtaining W-algebras; the direct construc tions, coset constructions and the first class Hamiltonian reduction method. Indeed, the direct constructions provided two so far unexplained deformable W-algebras, with confor mal weights 2,4,6 [6,7] and 2,3,4,5 [8], respectively, for which the procedure used in [2] for extracting the classical limit fails. In this paper we shall explain these algebras in terms of certain coset constructions, and shall see that their classical analogues are in fact infinitely, nonfreely generated (and therefore these algebras would appear to have no classical limit if one tries to force the procedure of [2] which is geared towards a finitely generated classical limit). Examples of classically infinitely generated coset algebras have recently been dis cussed in [9]. More generally, there is a large class of coset algebras, including for instance the diagonal cosets {Qk © Gm)/Gk+m at generic levels k and m, for which a simple group theoretic argument given in this paper shows that generically they have infinitely gener ated classical limits. Finally, it is clear that the DS reductions, which underlie all known deformable W-algebras with a finitely, freely generated classical limit, are a very special
272
subclass of the reductions of Kac-Moody algebras defined by conformally invariant first class constraints. In some examples of first class reductions to which the DS mechanism does not apply it has already been shown in [4] that the ring of gauge invariant differential polynomials is not freely generated. In this paper we further develop an illustrative example of this sort and demonstrate that the invariant ring carrying the reduced Poisson bracket algebra is infinitely, nonfreely generated. We wish to emphasize that although reductions of finitely generated DS type Walgebras and Kac-Moody algebras seem to lead generically to infinitely, nonfreely gener ated algebras at the classical level, the corresponding reduced quantum algebras are finitely generated in all cases studied so far 1 . We shall see that the underlying mechanism respon sible for this is that the infinitely many classical generators are not independent but obey infinitely many relations and upon normal ordering (a subset of) the relations quantum corrections arise which allow for eliminating the infinitely many 'would-be-generators' in favour of a finite subset. The paper is organized as follows. We shall first analyze a very simple example, a reduction of a 0-y system, in detail to illustrate the ideas. In particular, we shall see why the quantum version of the classically infinitely generated reduced algebra is finitely generated. Then we shall explain how this construction is related to a coset construction underlying the so far unexplained W(2,4,6)-algebra. This will lead us to discussing general coset constructions as well as bosonic projections of fermionic W-algebras and orbifolds of W-algebras that also possess infinitely, nonfreely generated classical analogues in general. Finally, to show that infinitely, nonfreely generated classical algebras arise in all reduction procedures, we treat an example of Hamiltonian reduction by first class constraints that leads to such a reduced classical system. We give our conclusions and comment on open problems at the end of the main text, and there are also two appendices containing technical material. 1. A reduction of a 0-y s y s t e m Below, we work out our simplest example, first at the classical then at the quantum level. We start by considering two independent generating fields £±(z) defined on the circle, subject to the Poisson brackets (PBs):
tt-(*U+(y)} = «(*-y),
tt-(*U-(v)}
= tt+(*U+(v)} = o.
(i.i)
Then we have the chiral algebra carried by the differential ring V consisting of the poly nomials in £± := d'£±. The fields £± are primary fields of weight \ with respect to the A claim to the contrary made in ref. [10] is not correct, see also section 3.
273
confonnal structure defined by
T:=-i(e+ac_-f_ae+).
(1.2)
This system is the classical version of a linear '/3-y system' (/3 := £_, 7 := £ + ) often used in conformal field theory. We introduce the sl(2) subalgebra of V generated by the currents
J* :=*-*+,
JE~-\H,
(1.3)
JF:=\H,
satisfying the PB relations { J « (*), Mv)}
= 2JE(y)S,
{ J « ( * U ± ( v ) } = ±{±(y)*,
{JH(x), JF(y)} = -2JF(y)6, { J s ( * U - ( v ) } = t+(y)S,
{ J B (x), J F ( y ) } = J H (y)«, {JF(x),i+(y)}
=
Uy)&,
(1.4) where 6 = 6(x—y). We wish to describe the reduced chiral algebra carried by the commutant (centralizer) V,i(2) of the s/(2) defined by the zero modes of the currents (1.3) in V. In other words, we are interested in the 'classical coset' of the #-7 algebra with respect to the 'horizontal' subalgebra sl(2) C s/(2) C V, i.e., V,t(2) = V/sl(2). To find the commutant notice from (1.4) that V is a ring of polynomials in infinitely many variables that form doublets, ( £ + , £ _ ) for any i = 0 , 1 , . . . , under the global s/(2) transformations generated by the zero modes of the currents. Therefore the pairwise symplectic scalar products of the doublets, given by
Wij^gW-gk?,
(1-5)
are obviously sl(2) invariants, i.e., belong to the invariant subring V,i(2) C V. The fact that the Wij are actually a generating set of V,i(2) is much less obvious, but it follows from invariant theory. In the terminology of Weyl [11], this is just the 'first main theorem' of invariant theory for the (defining representation of the) classical group SL(2). It is perhaps worth recalling here that invariant theory (see, e.g., [11,12]) deals with the following class of problems (among others). Take a group G and a set Va, ...,VU of finite dimensional representations of G. Consider the space M of polynomials p depending on (a fixed or arbitrary number of) variables that belong to these representations, p = p ( v " , . . . , u " a , . . . , u ° , . . . , v™"), where t>£" G Va for ia = 0 , . . . , m a etc. The linear space M. carries a natural representation of G induced by transforming the arguments of p. The problem then is to describe the G-singlets, i.e., the invariant polynomials. An important point is that since M is a polynomial ring so is the subring of invariants. The two major questions are: i) Describe a generating set of the invariant ring, ii) Find the relations obeyed by the (in general not algebraically independent) generators. The answer to i) is called the
274
'first main theorem' and the answer to ii) the 'second main theorem' of invariant theory for a given problem. In particular, in [11] these problems are solved for G a classical group and M. the space of polynomials depending on an arbitrary number of variables in the vector (defining) representation of G. Returning to our problem, it is easy to check that in addition to antisymmetry, Wij + Wj,i = 0,
(1.6)
the generators Wtj satisfy the following relation: WijWk,i
- Wi,kWj,, + WijWj,k
= 0,
(1.7)
for any i,j,k,l. The relation (1.7) is known as the 'syzygy' in invariant theory, and the 'second main theorem' of invariant theory states that all polynomial relations between the sl(2) invariant polynomials are consequences of (1.6) and (1.7) (see Chapter VI.1 in [11] and also Corollary 3.2 in [13]). Of course, this statement holds if we consider the variables £j! independent, i.e., if we forget about the action of the derivation d of the differential ring V, given by d£± = C± ■ Taking the derivation into account we also have the relation dWitj = Wi+1j + WiJ+1.
(1.8)
The generating set {Wij} is overcomplete (redundant) on account of (1.8) and to describe the reduced PB algebra in the most economical way we should select a subset of the gen erators forming a minimal generating set of V,i(2)- For this consider the linear span of the redundant set of generators at scale dimension d: Vd := linear span{Wi,;-1 i + j + 1 = d}.
(1.9)
The derivation d maps Vd into Vd+\ according to (1.8) and it is easy to see that by using this we can express the generators { Wij | V t , j } in terms of a subset of the generators spanning one dimensional subspaces of V*2r for r = 1,2,... any natural number. In this way we obtain a nonredundant (minimal) generating set of V,i(i), for instance {Wi,2,} with s running over the nonnegative integers. In terms of the redundant generating set the reduced chiral algebra is given by
{Wijix), Wk,,{y)} =(-l)'+1 £ > ! ) ' 0 „ 0 Wk,i+j+l-a(y)6^(x - y) o=0
j+l
+(-i)> E(- 1 ) 6 f J t V M + W - I - I G ^ C * - v) 6=0
+(-i)
i+1
V °
/
(1.10)
c ;
(c)
E ( - i ) ( t *W<+;-M-e(y)S (* - y) ^
c=0
'
+(-i)' B - i ) ' (' \ k) ww*-.(y)*(rf)(* - »)• A—n
^
'
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In the present example the r.h.s. is linear in the generators and we observe that this feature is also valid for the PB's of the generators {Wi ,2*}, as the elements of the redundant generating set are given by linear expressions in terms of the nonredundant generating set {Wi^,}. The elements in the nonredundant generating set {Wi,2»} are of course not independent, since the number of degrees of freedom should not increase in a reduction and we started with just two generating fields £±. Indeed, they satisfy the infinitely many differential-algebraic relations that can be obtained from (1.6), (1.7) and (1.8) by expressing all Wij in terms of W.J.}The main result of the above analysis is that infinitely many generators obeying in finitely many differential-algebraic relations are needed to describe the reduced classical chiral algebra carried by V,i(2). We next analyze this reduction at the quantum level. For this we take two bosonic chiral quantum fields (+(z), £-(•*), where the argument now varies on the punctured complex plane, for which the only nonregular OPE is
e_(x)C + (y):=-5-+«g.
(1.11)
x—y Here we introduced the Planck constant % explicitly in order to make clear the correspon dence to the PB (1.1), but one could of course set h to unity by a rescaling of the fields. The fields £± are primary fields of weight | with respect to the conformal structure defined by
f:=-i(f + a|_-|_ae+).
(i-i2)
We adopted the notation of Bais et al [14], thus (AB) denotes the usual normal ordered product of the fields A and B. We also define the quantum sl(2) currents by normal ordering the expressions in (1.3), JH:=(U+),
i B :=-i(| + e+),
JF~\{i-(-),
(1.13)
and find the (only nonregular) OPE's of the quantum currents to be 2ftJ E (y) , JH{x)JE{y) = + reg. x -y JH(x)JF(v)==^1+r<*. x —y -h2 JH(x)JH(y) = , _ y + reg. ; , , ; , ,
1
h2
+
(1.14)
hjH{y)
^(*W») = - 2 ( r r ^ T^T + wg -
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which (by putting h = 1) is sl(2) at level — A. The fields £± generate the chiral algebra V, i.e., the linear space V is spanned by the (repeated) derivatives and normal ordered products of f ±. The object of our interest is the coset V.m := j ^
(1.15a)
y
i.e., the set of fields in V that commute with the horizontal subalgebra sl(2) C sl(2) C V spanned by the charges QA=
2VifdxiA^
A = E,F, H.
(1.15b)
It is straightforward to verify that the quantum versions of the invariants in (1.5), given by Wij := ($>&>) - ( e l ° # > ) ,
g > := d%,
(1.16)
belong to Pti(2)- In the classical limit V,ni) becomes the differential ring V,\(2) and we know that the vector space Pw(2) is spanned by the (repeated) derivatives and products of the Witj. From this we can conclude that P,i(2) ls spanned by the derivatives and normal ordered products of the Wij. The OPE's of the generating set {W^,;} C V,i(2) read
Wi.i(*)w».,(y) = ( - i ) i + 1 f t £ (' + ')w*,.-+i+i-.(y)a;^
+(- 1 ) , ' & E ( j t')^ , < + , ' + , -» ( y ) a { ^ +(-l)^.g(^^M+;+i_cW^
, rt (-^^+1[(i+iy.u+ky.-(i
+2n
+ k)\(j + i)\]
(x_y)i+i+*+i+2
(1-17)
+ r < *-
Observe that, upon the correspondence d^^— <—► d£ 6(x —y), the O P E (1.17) corresponds to the PB (1.10), with a quantum correction given by the last 0(h2) term. In particular, noting that f = ^Wi.o, we can confirm that the central charge of our system is c = — 1, which is a special case of a well-known result about p-y systems. We now come to the main point, namely, the implication of the normal ordered version of the syzygy (1.7). A straightforward calculation, based on the normal ordering rearrange ment identities given, for instance, in [14], leads to the following result: (w,jWkJ)
r • -
- (Wi.tWj,,) + (witiWj,k) =
/ -
, •
» \C'i,kjWj,i+k+i+1 + C?,iiW»,.-+i+«+i + C'iijtkW,
I
(U8a)
277
with linear combination coefficients given by r, c
=
™
[((-!)*+ (-iy + 1 )q +fc)!, (-!)'(< + *)! , (-1)'+1('+J)'1 + I (7TITTJ! (i + it + i)! + (i + i + i)! J •
M1RM (U8b)
Similarly to the classical case, by using only cWo,6 = W^+i,6 + W^o,»+i we can express the generators { Wi^1 V i , j } in terms of a subset of the generators spanning one dimensional subspaces of V21-, Vd:= linear spvn{Wi<j\i +j + 1 =d}, (1.19) for r = 1,2,... any natural number. However, since the r.h.s. of (1.18a) is nonzero for ft ^ 0, it is clear that using also (1.18a) we can now eliminate the remaining generators lying in Vir as well if 2r can be written in the form 2r = i + j + k + l + 2 with pairwise distinct nonnegative integers i,j,k,l. But this is always possible if2r > 0 + 1 + 2 + 3 + 2 = 8, which implies that the commutant V,i(i) is generated by (repeated) derivatives and normal ordered products of the following finite set of fields: r = iwi,0,
w1<2,
Wi.*,
(1.20)
having scale dimensions 2, 4, 6. This is a drastic difference from the classical case where we need infinitely many generating fields since the r.h.s. of the syzygy (1.7) is zero in the classical case, when h = 0. The (automatically closed, nonlinear) OPE algebra of the fields (1.20) can be found from (1.17). It is also easy to find a generating set of the commutant P,i(2) consisting of T and primary fields with weights 4 and 6. In conclusion, the above construction yields a quantum W(2,4,6) algebra at c = — 1 possessing an infinitely, nonfreely generated classical hmit. Next we shall identify this VV-algebra as the coset of 3/(2) at level — i with respect to the horizontal subalgebra. In order to establish the isomorphism given by the second equality in V _'*(2). ^1(2) := ZTT^ = -ZTZT, sl(2) ~ sl(2f
(1-21)
where sl(2)_i /sl(2) denotes the commutant of the horizontal s/(2) in sl(2)_,
C V, it is
enough to verify that the generators of P»/(2) given by (1.20) can be expressed in terms of the sl(2)_i
currents given by (1.13). The quantum Sugawara Virasoro of the current
algebra is given by 3fif8Ug = (j ■ J) = \{JHJH)
+ {JEJF)
+ {JFJE).
(1-22)
Using the rearrangement identities of [14], one can prove the equality T. ug = f,
(1.23)
278
where T is given by (1.12). Note that the l.h.s. of (1.23) is quartic in the basic fields £±, while the r.h.s. is quadratic (reminding us of the "symmetric space theorem" [15]). Clearly, such an equality is only possible at the quantum level, and in fact the classical analogue of the Sugawara expression (1.22) vanishes identically. Concerning the weight 4 and the weight 6 generators, we can establish the following identities:
(dJ-dJ) = \(Wh0W1<0) - R[J#Wi.o + jjwi.a],
(1.24)
and 1
i
1
t
S8
17
{sfj-sFj) = ^(dw1,oawlfi)-2(wlt0Wifl)-h[^9 wl,o+^e/ wlfi-YWlA].
(1.25)
It is easy to see that using the above identities one can express the generating set (1.20) of P,i(2) m terms of composites of the current J. (Observe that this is possible because quantum corrections are present on the r.h.s. of (1.24) and (1.25)). This proves the relation "P.H2) C sl(2)_^/sl(2). Since we also have sl(2) _ ^ / sl(2) C V.i(2) on account of sl(2)_^ C V, by (1.13), the isomorphism (1.21) has been now established. 2. T h e deformable W(2,4,6) and remarks on diagonal cosets In this section we explain the origin of the 'fourth' deformable W(2,4,6)-algebra, which was unexpectedly found in [6] in addition to the 3 expected deformable algebras with the same weights (the DS type W^-algebras — or 'Casimir algebras' — corresponding to the principal sl(2) embedding in B3, C3 and the bosonic projection of the N = 1 super Virasoro algebra). The explanation will be given in terms of a coset construction. We also present related general considerations on coset constructions of W-algebras, arguing that in the classical case the diagonal cosets generically yield infinitely, nonfreely generated algebras. One can calculate the vacuum character, Xo{q), of the W(2,4,6) constructed in the previous section at c = —1 from either of its coset realizations in (1.21). One obtains (see also [16]) the following formula:
»<.)=n iq) n qip :ii -th *,(,):= xx-ir* 8 *^-- (2.D llnxA1
9 )
m>0
If one compares this with the standard 'vacuum Verma module character' ^2,4,6(9) associ ated to fields with weights 2, 4, 6, given by
h
'
M
:=
n n >o(i-*" + 2 )(i-<" + <xi-*" + s )'
(2 2)
-
279
one finds up to order 20 Xo(?)-^2,4,6(«) = - 9 1 1 ( H - 2 g + 3 3 2 + 6 g 3 + 1 0 9 4 + 1 7 g 5 + 2 7 g 6 + 4 4 g 7 + 6 7 ? 8 + 1 0 5 9 9 + 0 ( 9 1 0 ) ) . (2.3) The fact that all coefficients on the r.h.s. of (2.3) are nonpositive and ^2,4,6(9) is the smallest standard character for which this is the case not only confirms (by the argument of [17,1]) that the coset (1.21) should be a W(2,4,6)-algebra, what we have already proved, but also shows the existence of a first 'null field' at scale dimension 11. The existence of this null field is due to the normal ordered syzygy (1.18). Indeed, at scale dimension 11 eq. (1.18a) yields 3 relations, correspondingly to the 3 different possible choices of pairwise distinct i,j, k, I such that t + j + k + I + 2 = 11. Two linear combinations of these relations arise as derivatives of the relations at scale dimensions 8 and 10 which were used to express the scale dimension 8 and 10 'would-be-generators' (Wi,6 and W^i.s) in terms of the set (1.20). The remaining third relation gives rise to the null field in question. Along these lines, it is also easy to derive the explicit formula of this vanishing nontrivial normal ordered differential polynomial in the generators (1.20), but the formula is not particularly enlightening. What is important is to emphasize the twofold role of the normal ordered relations: A subset of them is responsible for the algebra being finitely generated at the quantum level and the rest give rise to null fields. Let us recall now that it was shown in [7] that the so far unexplained algebra with spins 2, 4 and 6 has a generic null field precisely at this scale dimension. It is also known that the bosonic projection of the N = 1 super Virasoro algebra has a generic null field already at scale dimension 10 [17], whereas the Casimir algebras of B3, C3 have no null fields at c = —1. In conclusion, we can identify the coset algebra (1.21) as the 'fourth' deformable W(2,4,6)-algebra at c = —1. In order to understand how to deform this coset algebra to generic c and thus completely explain the algebra, let us proceed with some general remarks on cosets. Consider a coset of the form (Gk © Gm)/Gk+m, where Q is a simple Lie algebra, Gk is the corresponding affine Kac-Moody algebra at level fc, and Gk+m C Gk®Gm is the diagonal embedding. In such a situation one can show that ,. Gk®Gm Gk /„... hm —= = — , (2.4) m ^ ° ° Gk+m v where the equality holds at the level of algebras. For generic m, the coset algebra on the l.h.s. is a deformation of the coset algebra on the r.h.s., in particular, it has the same spin content of generators. This statement holds for classical as well as quantum W-algebras. The argument presented for the quantum case in [18,19] is roughly the following: The coset generators of the l.h.s. are (/-singlets i n GkffiGm with respect to the horizontal subalgebra
280
G C Gk+m- Denote the currents generating Gk by Ja (a — 1,... ,dimG), those generating Gm by j a - Taking commutators (resp. Poisson brackets) with all (Ja + j„) one concludes from the central terms that the coefficient of a monomial contained in a generator of the coset algebra tends to zero for m —> oo if it contains any j a . This proves the inclusion of the l.h.s. into the r.h.s of (2.4). The equality in (2.4) as well as deformability follow from the fact that to any ^-singlet consisting of the Ja only one can add correction terms containing also the j a such that it commutes with Gk+m [18,19]. In the classical case the deformation of the 'singlet algebra' on the r.h.s. of (2.4) can be made explicit as follows. The £-valued current J generating the algebra Gk satisfies the Poisson brackets iU*),
Mv)}
= £ /.% JcivWx
-y)-k
gah6'(x - y),
(2.5)
c
where flh {gab) denote the structure constants (metric) of G, and similarly for the currents j and (J + j) that generate Gm and Gk+m, respectively. Let P = P(J, dj,..., dnJ) be an arbitrary element of the singlet algebra, i.e., a differential polynomial in the components of J which is invariant under the transformation 6tJ = [e, J] for any constant e G G- The corresponding element of the diagonal coset on the l.h.s. of (2.4) is obtained by replacing J by / , where I:=J-±j,
(2.6a)
m and also replacing d'J by VI, where 2? is the covariant derivative defined by VI:=dI+j^—[J + j,I\, K+ m
(2.6b)
for k, m, (k + m) nonzero. Indeed, for any 5-valued function e(x), under the transformation 6tJ = [e, J]-ke',
6,j = [e,j] -me'
(2.7a)
one has Sf(ViI)=[e,ViI]. (2.7b) This immediately implies that P(I, VI,..., VI) belongs to the coset on the l.h.s. of (2.4), and it' tends to P(J, dJ,..., 9 n J ) as m —» oo, in accordance with (2.4). We shall see later in this paper that covariant derivatives are useful also in many other considerations concerning current algebras, simply because the currents generate gauge transformations. See also ref. [9], which inspired some of our considerations. We now wish to argue that the cosets Gk/G are classically always infinitely generated with infinitely many relations. To see this we note first that invariant theory ([11,12] and
281
references therein) applied to the (/-invariant differential polynomials in the Q-valued current J containing the derivatives dnJ up to a fixed finite order leads to finitely many generators and a finitely generated set of relations. However, the coset on the r.h.s. of (2.4) consists of the ^-invariant differential polynomials with an arbitrary number of derivatives. Thus, in the end, one is looking for invariant polynomials in infinitely many variables, d" J for any n, and therefore the invariant ring is also generated by infinitely many generators and infinitely many relations. In the spirit of Weyl [11], these would be obtained by inserting the infinitely many variables d" J into some finite list of 'typical basic invariants' and a corresponding finite list of 'typical basic relations', which would be given by a first and a second main theorem of invariant theory for the adjoint representation of Q on Q. (Unfortunately, we could not find these theorems in the mathematical literature for the adjoint representation in general, but it might be possible to infer the case of the adjoint representation from more general results and constructions of invariant theory). More precisely, since in our context the infinitely many variables dn J are linearly related by the action of the derivation d, using d one could always write down additional linear relations between those generators differing only in the places where the derivatives have been inserted (like in (1.8)). However, taking all relations into account one is still left with infinitely many generators (and relations). This argument shows that in the classical case the coset on the r.h.s. of (2.4) is infinitely generated with infinitely many relations. Clearly, the same is true for the diagonal cosets (Gk © Qm)/Gk+m by defonnability. Let us illustrate the above in the simplest nontrivial case, the classical singlet algebra
(2 8)
-
im-
Since in the complex case the adjoint representation of the Lie algebra sl(2) is equivalent to the vector representation of o(3), we can directly apply the results in [11] for describing the generators and relations of the ring of invariant polynomials (2.8). More precisely, we can do this provided we forget about the action of the derivation and, for the moment, consider the variables d" J as independent, where J is the sl(2) valued current. According to [11], the invariant polynomials are generated by the quadratic invariants S(m,n):=(dmJ,dnJ)
(Vm,n),
(2.9a)
where (•, •) is given by the trace in the defining representation of s/(2), and the cubic invariants S{p,q,r):={[^J19'J],SFJ) (Vp * q ± r). (2.9b) (This is familiar from many physical applications of the rotation group S0(3), where (2.9a) becomes the usual scalar product of two vectors, and (2.9b) the volume of the
282
parallelepipedon spanned by three vectors). We now quote the basic relations from [11] (Chapter 11.17). Let {mo,mi,m2,m3} be any set of distinct, nonnegative integers, and let {no,ni,n2,n3} be another set of this type (there could be overlap between the two sets). In addition to the relations expressing the obvious symmetry properties of the invariants (2.9), the basic relations are of the following three types. First,
det
S(mo,n 0 ) S(mi,n0) S(m2,n0) S(m3,n0)
5(m0,ni) S(mi,ni) S(m2,ni) S(m 3 , ni)
5(mo,r»2) S(mi,n2) S(m2,n2) S(m3,n2)
S(m0,n3)' S(mi,n3) = 0. S(m2,n3) S(m3,n3).
(2.10a)
Second,
5(mi, m 2 , m 3 ) 5 ( n i , n2,n3) + 2det
S(muni) 5(m2,ni) S(m3,ni)
S(mun2) S(rn2,n2) S(m3,n2)
5(m!,n3) S(m2,Ti3) S(m3,n3)
= 0.
(2.10b)
Third, ^
±S(mi,m2,m3)S(m0,n)
= 0,
(2.10c)
where n is arbitrary and the sum is over the (signed) permutations of {mo,mi,m2,m3}. These would generate all relations between the invariants if the variables dnJ were inde pendent. Taking the action of the derivation into account, we also have the linear relations dS(m, n) = S(m + 1, n) + S(m, n + 1)
(2.11a)
and dS(p,q,r)
= S(p+l,q,r)
+ S(p, q + 1,r) + S{p,q, r + 1),
(2.11b)
where the cubic invariant is of course zero if any of its two arguments coincide. We can use the linear relations in (2.11), which are analogous to (1.8), to introduce a nonrtdundant (minimal) generating set of the differential ring of singlets (2.8). Let N, be the number of generators at scale dimension s in the minimal generating set. Fom (2.11), we find the (classical) generating function, / c i(«) := £ , N,u', to be given by /el(u) =
(u6 - u5 + u2) = u 2 + u 4 + 2 u 6 + 2 u 8 + u 9 + 2 u 1 0 + u n + 2 u 1 2 + u 1 3 + 3 u u + O ( u 1 5 ) . (I-I^X1-"3)
(2.12) This infinite spectrum of classical generating fields2 is to be contrasted with the correspond ing quantum case. We recall [20,1] that, according to character arguments, the quantum 2
Eq. (2.9) defines invariants for any Q and one can confirm already from the quadratic
invariants that the classical coset (2.4) is always infinitely generated.
283
version of the coset (2.8) is expected to yield a finitely generated algebra. Moreover, for generic k the scale dimensions of the quantum generating fields should be those determined by the following (quantum) generating function, fq(u), / , ( u ) = u2 + u*+ 2u 6 -I- 2u 8 -I- u 9 + 2u 10 + un.
(2.13)
The first difference between the classical and quantum generating functions occurs at scale dimension 11, where we have a classical generator but no quantum one in the respective nonredundant generating sets. The explanation lies in the fact that the first classical re lation also occurs at precisely this scale dimension, namely, it is given by (2.10c) with {mo, mi, m2,7713} = {0,1,2,3} and n = 0. Given our experience with the ji-f example, we now expect the following: A redundant, infinite generating set of the quantum coset is obtained by normal ordering the classical generating fields, and for the quantum coset it must be possible to eliminate the 'would-be-generator' at scale dimension 11 due to a quantum correction in the normal ordered version of (2.10c). In a similar fashion, one can also understand the cancellation of one 'would-be-generator' at scale dimension 12. The statement that the quantum generating function (2.13) is correct, which is supported but not rigorously proved by the character 'argument', is clearly equivalent to this cancellation taking place at all higher scale dimensions 3 . The coset sl{2)^®sl{2)m
(2
u )
*'(2)4+„ can now be treated easily: We combine the general remarks on cosets of type (2.4) with the statements on the coset sl(2)k/sl(2). Classically, a generating set for the coset algebra (2.14) can be obtained as follows. In the generators (2.9) one replaces the current J by the current I as given by (2.6a) and substitutes the derivative d by the covariant derivative V (2.6b). The relations in the coset (2.14) are obtained by the same substitutions applied to the relations (2.10), (2.11) in the coset sl(2)k/sl{2). The quantum version of the coset (2.14) is more complicated because, due to the covariant derivative 27, the generators of the quantum algebra cannot be obtained by naively normal ordering the classical generators. At least, deformability ensures that for generic m we have the same number of generators and null fields in the quantum coset sl(2)k ffi 5 K2)m/ s K2)t+m ^ i n t n e c o s e t ■ s '( 2 )*/ s '( 2 )- I n particular, eq. (2.13) means that the quantum coset (2.14) leads to a W(2,4,6,6,8,8,9,10,10,12) (with known truncations for 3
Similarly to the /?-7 example, only a subset of the relations should be needed for the
cancellation, the rest should give rise to generic — in k — null fields. In fact, the first such generic null fields appears at scale dimension 13.
284
integer positive m < 6 [20,1])- Still, the results from invariant theory also simplify the explicit construction of the generators of this quantum coset. Noting that sl(2) is generated by the two subalgebras sl(2) and (7(1) one may restrict the ansatz for invariant fields to normal ordered differential polynomials in the basic invariants (2.9) where each sl(2) valued current J can either be replaced by J 6 sl(2)k or by j 6 s/(2) m . Then, one determines the coefficients in this ansatz by requiring the OPE with the [/(l)-current in the diagonally embedded sl(2) to be regular. This enables one to explicitly construct at least the primary generator of dimension 4 in the coset (2.14) in addition to the Virasoro field. Before proceeding with the explanation of the deformable quantum W(2,4,6), we would like to note a well-known result for the central charge c of the quantum coset (2.14):
Now we return to the starting point of this section and give the explanation of the 'fourth' deformable W(2,4,6). Recall that we have already identified this algebra at c = — 1 as the coset sl(2)_i/sl(2). Eq. (2.4) enables us to deform the quantum coset sl(2)_i /sl(2) to generic c (respective m) in the following manner 4 : J B
i®j|(2) m =4: — a W(2,4,6).
(2.16)
*f(2)m_i In particular, also the null field at scale dimension 11 is deformed to generic c. This shows that the coset (2.16) realizes the previously not understood solution for W(2,4,6). The relation between the central charge c and the level m is given by (2.15): c = c _ i ( m ) = ~ (2m+3Wm+2> • ( ^ e n a v e n o * assumed m to be an integer and therefore we have indeed constructed the algebra for generic c). When looking for minimal models of this W(2,4,6) particular values of the level m will be distinguished. Note that, by an explicit search, a few minimal models of this algebra have been found in [7] for values of c where the level m is an integer. It would certainly be interesting to find out if this is true in general and to better understand the minimal models of the coset algebra (2.16). We conclude the discussion of the example (2.16) by remarks on how the truncation happens at k = — £ in the genetically larger coset algebra (2.14). For the quantum coset sl(2)k/sl(2) we have checked that one 'would-be-generator' for each of the scale dimensions 6, 8 and 9 becomes a null field at k = — i . This probably also applies to the quantum analogue of the classical generator at scale dimension 11. Therefore, the first classical relation, which arises at scale dimension 11, is now not needed to cancel a 'would-begenerator', but can give rise to the first null field (the one we already understood in the /?-7 This observation is due to R. Blumenhagen.
285
realization). By deformability, the same remarks apply to the quantum coset (2.16). The picture in the classical case is less clear. Prom the quantum equivalence in (1.21) and our study of the classical analogue V,t(2) of V,i(2), we expect the classical limit of the quantum coset (2.16) to contain one generator for each positive even scale dimension. However, in the classical case nothing happens to the generators at any value of the level ifc ^ 0, and therefore the set of generators of the 'full classical coset' is encoded in the counting function (2.12) also at k = — ~. This apparent contradiction can probably be explained by the existence of a subring closed under Poisson bracket, containing one generator for each d, 0 < d 6 2Z, in the full classical coset given by the ring of all classical invariants. We expect the classical limit of (2.16) to realize such a proper subring of the full classical coset. Recall that at k = 1 the quantum coset (2.14) gives just the Virasoro algebra. The classical limit of this Virasoro field freely generates a subring of the full classical coset, which is obviously closed under the Poisson bracket. (As noted above, at k = — | we also expect a subring, but an infinitely generated one, to realize the classical limit). A similar remark applies to the cosets G\ © Gm/Gm+i for G any simply laced Lie algebra A, D, E. The quantum versions of these cosets are well-known to give rise to the so-called 'Casimir algebras' (see e.g. [14]) which contain no null fields for generic m. On the other hand, at m = oo the rank (G) classical Casimir invariants (invariants without derivatives of the current) freely generate a subring of the ring of all classical invariants, which is closed under Poisson bracket [21]. Clearly, the deformation of this subring to generic m carries the classical limit of the quantum Casimir algebra. 3. On general cosets and the deformable VV(2,3,4,5)-algebra In this section we give a prescription for finding the generating set for a general class of (classical) cosets, generalizing the results on the diagonal cosets (2.4) discussed previously. In particular, this shows that classical cosets are infinitely, nonfreely generated in general. These results will be illustrated with another example which, as a by-product, also explains the quantum W(2,3,4,5)-algebra found in [8] in addition to the well understood Casimir algebra based on A4 that has the same spectrum of generators. Let VV be any classical W-algebra (including Kac-Moody algebras) generated by finitely many, independent generating fields, and suppose that VV contains a current algebra, GK, as a proper subalgebra. Suppose also that the restriction of the central term of W to GK is nondegenerate, and that it is possible to partition the generating fields of W into the generating fields Ja of GK and a complementary set of generating fields J^- that form primary field multiplets with respect to the current algebra GK- (TO avoid confusion, note that the Jf- need not be Kac-Moody currents). Thus the Poisson brackets between the J„ are similar to those in (2.5), with a nondegenerate matrix gai, except that now we do not
286
require the horizontal subalgebra Q c 8 « to be (semi)simple — in particular, it can contain U{\) factors. Moreover, we have Poisson brackets of the form {J0(*),Jx(y)} = - £ i l ( a ) f . 7 x ( y ) * ( x - y ) ,
(3.1)
where the matrices R(a) = R(a)}i, a = 1 , . . . , d i m ( £ ) , form a — in general reducible — representation of S, R(a)R(b) - R(b)R(a)
= Yl £»*(<:).
(3-2)
c
We are interested in the coset algebra W J-,
(3-3)
i.e., the Poisson bracket algebra carried by the ring of those differential polynomials P
= p(J,dJ,...,
dmJ, J x , dJx,...,
d" J x )
(3.4)
that Poisson commute with the charges Q(e):=
Idxe"(x)Ja(x)
(3.5)
for arbitrary test functions e"(x). We shall show below that the elements of the coset (3.3) are the Q-invariant differential polynomials of the type P = P(J±,VJ±,...,VnJ±),
(3.6)
where VJ1- is the covariant derivative defined by VJ^:=dJ^
+ lj2jb9baR(a)ijf,
(3.7)
with £3 6 gabgbc = 6ac- In particular, the elements of the coset (3.3) can be written as polynomials in J1- = { / x } and its covariant derivatives. The variables in the argument of the r.h.s. of (3.6) belong to the representation R(a) of Q, and P must be invariant under the natural action of Q on its arguments, which means that P must Poisson commute with Q(e) for constant e". The significance of this result is that it reduces the problem of describing the ring carrying the classical coset (3.3) to a standard (although not necessarily easy) problem in the invariant theory of the finite dimensional Lie algebra Q. Thus, applying the same general reasoning as for the diagonal coset, we see that the differential ring of invariants (3.3) must be infinitely, nonfreely generated in general.
287
For the proof we first rewrite the polynomial p in (3.4) as a (uniquely determined) polynomial P = P(J,DJ,...,DmJ,J-L,VJ±,...,VnJ1)
(3.8)
in the new variables VkJ^-, DkJa, where the new derivative DkJ of the S-valued current J is recursively defined by DkJ:=dDk~'lJ+-[J,Dk-lJ]
with
D°J = J.
(3.9)
We are looking for P such that {Q(e),P}
= 0,
(3.10)
and the new variables are advantageous for computing the Poisson bracket since they have simple Poisson brackets with Q(e): {(VkJ±).,Q(t)}
{VkJ±))
= £'*«(«)*
;.« {(DkJ)a
(3.u) lt,(DkJ)U-K(Dkde)a
,Q(t)} =
where e = {ea} is the arbitrary ^-valued test function and the derivative Dk (de) is defined similarly to (3.9), Dk(de)~dDk-'(de)
+ -[J,Dk-1(de)}
with
D° (de) = de.
(3.12)
One easily verifies (3.11) by induction on k (or recalls it from Yang-Mills theory). Because of the derivation property of the Poisson bracket, {Q(e), P} is a linear expression in the algebraically independent parameters dkea, {Q(e),P} = ^ P
M
aie«,
(3.13)
a,*
and thus (3.10) requires the polynomials P 0 ,ti which depend on the same variables as P, to vanish. Let us now single out an index a and look at Pa,km*x, where km*x is the highest value of k that appears in (3.13) for this particular a. It is easy to see from the second line of (3.11) that the contributions to ■?»,*„,„ come from those monomials in the polynomial P that contain (various powers of) the highest derivative of the type (Dlj)a, , _1 given by (i?* "*» j) , which appears in (3.8). Since those monomials are algebraically independent, Pa,kmmx = 0 requires all of them to vanish. This then immediately implies that P in (3.8) cannot depend on the variables (D'J) for any a and I = 0 , 1 , . . . , proving that P must be of the form (3.6). For such a P the requirement that (3.10) must hold for any test function e is equivalent to the same requirement for constant c since no derivative
288
of e appears in the first line of (3.11), completing the proof of our characterization of the elements of the coset (3.3). It is easy to recover the results on the diagonal coset on the l.h.s. of (2.4) from the above. In that case QK, K = k + m, is the diagonal subalgebra in the denominator and J1becomes / in (2.6a). It is also easy to specialize the general result to classical cosets of the type Gk © 'Hm/'Hik+m, where i denotes the Dynkin index of the embedding H C Q. The generators comprising J1- are in this case given by the currents in the complement of "Hik in Gk together with the currents in Hik © W m formed according to (2.6a). From this one can derive the natural generalization of (2.4): hm -£ ">~°° Hik+m
= —-. «
(3.14)
It also interesting to note that this type of coset has subalgebras according to Gk ,_ Gk
289
the charge conjugate doublets by W * and their covariant derivatives by Wa = V'W*. Then a redundant generating set for the coset is given by the (/(l)-primary charge neutral fields and the following composite generators: Ki
:= W+MW~M.
(3.16)
Forgetting about the action of the derivative V, all relations satisfied by the redundant set of generators (3.16) are generated by the following quadratic relations:
Kiukj - «,cWi.cu:W:l = o.
(3-i7)
where the 'statistics factor' e 0| j is defined as e0,j = —1 if both W^ and W4 are fermions and 1 otherwise. The proof that (3.17) generates all relations between the generators (3.16) is a particularly simple version of a standard argument used in invariant theory (see the straightening algorithm in [13]). One has to show that a basis for the linear space of invariant polynomials in the Wa with a given degree can be obtained from (3.16) using (3.17) and (anti-)commutativity of the U^''t. Because the invariant monomials have zero charge they contain an equal number of Wa and Wa , in particular they are even order. We can choose an ordering where the charge alternates. This reduces the problem to finding a basis for monomials of type Wa W^ Wc WJ Clearly, a basis for these monomials is obtained by a lexicographic ordering of the sets {(a,t), (c, k),...} and {(6, j),(d, I),...}. Then observe that, on the one hand, each such monomial can be written as a monomial in the generators (3.16). On the other hand, each set of indices can be independently ordered for monomials in the U^'}h using (3.17) and (anti-)commutativity of the U^'3b. This completes the proof. Finally, we enforce the action of the covariant derivative on the generators (3.16):
wii = u%'i + u:i+l.
(3-i8)
Using (3.18) we can eliminate generators from the set (3.16) in favour of a nonredundant set of generators, for example the generators Ua'{. As usual, the complete set of relations satisfied by the nonredundant generating set Ua'[ can be obtained from (3.17) using (3.18). (We note in passing that the relation for the coset W|/J7(l) discussed in [9], eq. (2.26) of the reference, can be recovered as a particular consequence of (3.17) and (3.18)). The general statements will now be illustrated in the following example: The commutant of the [/(l)-current in the N = 2 super Virasoro algebra, SVIR(iV = 2). The algebra SVIR(7V = 2) is generated by the energy momentum tensor L, a current J and two fermionic fields G± of scale dimension | carrying {/(l)-charge ± 1 . In order to find the complement of the 1/(1) current algebra in SVIR(./V = 2) we first go to a primary basis with respect to
290
the current algebra. This means that we have to replace the energy momentum tensor L by L = L — ^JJ if we fix the normalization such that the central term of J with itself is given by | . Next we introduce the covariant derivative according to (3.7): VL := dL , Q VG±:=dG±±-JG±. c
(3.19)
From (3.16) and the action (3.18) of the covariant derivative V we obtain a nonredundant generating set for the classical coset SVIr^iV = 2)/J7(l):
L = L - J^JJ ,
(3.20a)
{t/°-> = G+2VG" | 0 < j € Z } .
(3.20b)
Furthermore, we obtain from (3.17) the complete set of relations (in addition to (3.18)) satisfied by the redundant set of generators UiJ = (2?'G + )(2?'G~): U^Vk'1 + U'W'i
= 0.
(3.21)
An important special case of (3.21) for the nonredundant set of generators (3.20b) is UOJU°'k = 0
Vj.jfc.
(3.22)
These relations also directly follow from the fact that G* are fermions satisfying the Pauli principle. Note that the nonredundant set of generators (3.20) as well as the set of relations they satisfy are infinite, as expected. Let us now turn to the quantum version of this coset. For generic c, counting the number of invariant fields at a given scale dimension should be the same at the classical and the quantum level. Therefore one can calculate to vacuum character, xoi by counting the number of classical invariants that arise as differential polynomial in L and G±. In this way one obtains Xo(«) - *2.3,4,5(«) = V ( 2 + 4q + 9q2 + 16g3 + 32g4 + 54qi + 96? 6 + 0(q7)),
(3.23)
where ^2,3,4,5 denotes the vacuum character of a freely generated algebra with generators of scale dimension 2, 3, 4 and 5. This suggests the identification S V I
^ = 2 W(2,3,4,5)
(3.24)
for the quantum coset. According to (3.23), our quantum coset has two generic null fields at scale dimension 8. Recall now that the same null field structure has been observed in [8] for
291
the 'second' deformable W(2,3,4,5)-algebra found by direct construction. Therefore the W(2,3,4,5)-algebra appearing in the identification (3.24) must be the 'second' W(2,3,4,5)algebra of [8] (the other deformable W(2,3,4,5)-algebra is the Casimir algebra of At which has no generic null field). The identification (3.24) is further supported by explicit calculations presented in detail in [22]. The energy momentum tensor of the quantum coset is just the normal ordered version of (3.20a). The quantum analogues of the generators of higher scale dimension (3.20b) are more difficult to determine. By commutation with the zero mode of the current it follows that all fields in the coset must be uncharged. It is straightforward to make an ansatz in the uncharged fields and determine those linear combinations that commute with the complete current. One finds precisely one new generator at scale dimensions 3, 4 and 5 with leading terms quadratic in the fermions G*, and by computing the OPEs of these composite fields one recovers [22] the structure constants of the W(2,3,4,5) given in [8]. Similarly as in previous examples, one can argue that normal ordered analogues of the classical relations (3.22) ensure that the quantum coset on the l.h.s. of (3.24) is finitely generated, whereas the corresponding classical coset needs infinitely many generators (3.20). For example, the normal ordered version of the classical relation G+G~ G+G~ = 0 contains a term proportional to what would have been the new generator at scale dimension 6. The central charge c of the coset energy momentum tensor L is obtained by shifting the original central charge c by 1. Inserting the parametrization c(k) of the unitary minimal models of SVIR(7V = 2) by a positive integer k, one obtains
£(fc) = c(fc)-l = 2 £ = i l
(3.25)
Note that this is just the well-known formula for the central charge of Z*-parafennions [23]. In fact, the coset algebra (3.24) is a universal object [22] for the first unitary minimal models of the Casimir algebras based on A*_i which describe the Zt-parafermions [24,25]. Moreover, it is also well known (see e.g. [1,26]) that the Zt-parafermions can be realized using the coset sl(2)/U(l), and therefore also this coset algebra should be a universal object for the Zt-parafermions. It can be verified that the standard character counting argument of [17,1] indeed predicts a W(2,3,4,5) (a finitely generated algebra) for the quantum coset
»7(2)/tf(l). Because the above contradicts an earlier claim [10], we wish to draw the reader's attention to the further evidence in [22], which shows that the claim of [10] that the quantum coset sl(2)k/U(l) requires infinitely many generators (one for each integer scale dimension greater than or equal to two) is incorrect as it stands. First, it can be shown [22] that sl(2)k/U{l) is isomorphic to SVIR(N = 2)/U(l), which we have argued here to be finitely
292
generated. Second, it can be verified explicitly [22] that the quantum coset sl(2)k/U(l) contains the W(2,3,4,5) of [8] as subalgebra. Finally, comparing the vacuum character 5 of this quantum coset, \o in (3.23), to the number of composite fields in the W(2,3,4,5) determined in [8] up to scale dimension 8, proves that no new generator appears in the coset at scale dimensions 6, 7 or 8, contrary to the claim of [10]. Thus we expect that the coset sl(2)k/U(l) is actually isomorphic to the W(2,3,4,5)-algebra with generic null fields constructed in [8], though no complete proof is available at the moment. We hope to present a complete proof along the lines of the /3-y example and character considerations to arbitrary order elsewhere [16]. 4. Orbifolds of W-algebras In this section we show that orbifolds of W-algebras behave very similarly to the cosets discussed in the previous two sections. All known examples of orbifolds are generated finitely at the quantum level, but possess infinitely generated classical analogues with in finitely many relations. One orbifold example that will be discussed here also turns up as the k = 2 special case of the coset (2.14). Namely, the quantum version of the coset ( 2 ) 22 ©37(2) ©sl(2) m ) )//sl(2) leads H (IUasi(Z) 7(2) S K2)m+2 ieaas to 10 aa rv\z, i, 0j-aigeDra isomorpnicto tne Dosomc projec 2 *ost(^)mjm /si(*) m+2 tion of the N = 1 superm +Virasoro algebra [17]. leads to a W(2,4,6)-algebra isomorphic to the bosonic projec 2 tion of the N = 1 super Virasoro algebra [17]. The structure of this quantum W(2,4,6) has been investigated in [17,27,28]. In particular, the first generic null field appears at scale dimension 10. This bosonic projection is a particular case of the more general 'orbifold'construction on W-algebras. Any W-algebra (including Kac-Moody algebras) with nontrivial outer automorphisms Any W-algebra (including Kac-Moody nontrivial outer can be projected onto the invariant subspacealgebras) under thewith automorphism group.automorphisms This so-called can be projected onto the invariant subspace under the automorphism group. This so-called 'orbifolding' leads to another W-algebra. For simplicity, we here restrict our attention to Z 2 automorphisms p that act on the finitely many generators {Wa | a G I U K} as follows: p(Wa) =Wa Va e £ , (4.1) p{Wb) = -Wh V6 6 I . We can divide the index set T into two subsets: A set T\ referring to bosonic fields and a set J2 referring to fermionic fields transforming nontrivially under the automorphism p. It is easy to determine a generating set classically. Note that the nontrivial ^-invariant differential polynomials are even order in the {Wt, | 6 6 I } . Plainly, every even order poly nomial can be regarded as a polynomial in quadratic expressions. Therefore the quadratic expressions formed out of the {Wj | b € 1} generate the orbifold together with the invariant 5
Note that the corresponding formula (4.14) in [10] contains a misprint: The exponent of f(q) should be 2, not 3.
293
fields {Wa | a e AC}. A redundant set of quadratic generators is given by:
xilt ■•= wf ° wj»
6, c e J, o < i,j e z
(4.2)
where W4 := d'Wj. The derivative acts on the generators (4.2) like in eq. (1.8): dXii^Xg'+Xi*1.
(4.3)
Using the action of the derivative (4.3) and paying attention to the Pauli principle for the fermionic generators, i.e., that fermions have odd Grassmann parity, one can choose the following minimal set of generators for the orbifold: Wa, a e K
(invariant generators) ,
X°;> : = Wbd> Wc, i
b < c, 6, c e I , 0 < j e Z , (4.4)
= Wdd Wd,
deli, 0<;'e2Z
(square of bosons) ,
= Wed>We,
e € J 2 , 0 < j e 2Z + 1
(square of fermions)
where '6 < c' denotes some ordering of the original generators. Eq. (4.4) shows that Z2 orbifolds are always infinitely generated at the classical level. Note that a (redundant) set of quantum generators can be obtained just by normal ordering (4.4). In order to find the complete set of relations we first regard all Wa as independent. The complete set of relations satisfied by the redundant set of generators (4.2) is generated by K'!c - «,cX% = 0,
(4.5a)
Xi?Xi-
(4.5b)
where «t)C = — 1 if both Wi, and Wc are fermions, and t\,tC = 1 otherwise. (Clearly, choosing certain indices in (4.5) equal leads to trivial relations). The proof that (4.5) indeed generate all relations is very similar to the one presented below (3.17) and therefore we omit it. It is straightforward to derive the relations satisfied by the nonredundant set of gener ators (4.4) from (4.5). One simply has to recursively apply (4.3) (which encodes the action of the derivative) in order to express the relations (4.5) in terms of the generators (4.4). Next, we further elaborate some of these relations for two examples and discuss their impact on the quantum case. One of the simplest examples of orbifolds is the bosonic projection of the N = 1 super Virasoro algebra that we have already mentioned. The N = 1 super Virasoro algebra is the extension of the Virasoro algebra L by a primary scale dimension | fermion G. According to (4.4), a nonredundant set of generators for the classical orbifold is L,
$n:=GdnG
for all odd n.
(4.6)
294
In particular, this orbifold has one generator at each positive even scale dimension. Using the notation of (4.4) we have the identification $ n = X°'n if we omit the irrelevant lower indices. From (4.5b) one reads off 0 = X°<>X°<' + X°<°X'<1 = X°-'X0-' because X°'° = 0. In terms of the generators (4.6) these infinitely many relations read 0 = $"*m = 0
for any
0 < n, m e 2Z + 1.
(4.7)
In this case the particular subset (4.7) of relations for the nonredundant set of generators can also immediately be inferred from the Pauli-principle: $ n * m = (GdnG)(GdmG) = —G2(dnG)(dmG) = 0. However, (4.5) encodes more relations. For example (4.5) and (4.3) imply X^&X0'1 = A - 0 - 1 ^ 2 ' 1 + 2A 1 - 2 + A 0 - 3 ) = A ^ A 1 - 2 = - A 0 ' 1 A 1 ' 2 . For the nonredundant set of generators this implies the following relation at scale dimension 10: &&&
= 0.
(4.8)
It is also straightforward to verify (4.8) directly: * 1 5 2 * 1 = (GdG)d2(GdG) = 2 2 i G{dG){&G)(dG) + 2G(dG) (9 G) + G(dG)G{9 G) = 0. The first and second term on the r.h.s. vanish because (dG)2 = 0, the last term is zero because G2 = 0. Now we explain how the classical relations make the quantum version of the bosonic projection of the N = 1 super Virasoro algebra generated by just three fields of scale dimension 2, 4 and 6. First, one checks that the normal ordered analogue of the classical relation $ ' $ ' = 0 contains a correction term proportional to $ 5 (for the explicit expression see (A.2) in appendix A). Thus, the field $ 5 with scale dimension 8 does not give rise to a new generator in the quantum case and there is no relation at scale dimension 8 in the quantum orbifold. Similarly, the normal ordered counterpart of the classical relation $ 3 $ * = 0 picks up correction terms containing $ 7 (eq. (A.3) in appendix A). This shows that also at scale dimension 10, upon normal ordering, a classical relation cancels a 'wouldbe-generator'. It follows from general results on W-algebras that this already ensures that the quantum orbifold under discussion at least contains a W(2,4,6) as subalgebra. We have not yet used the classical relation (4.8). Indeed, on the quantum level there is a generic null field at scale dimension 10, which is the normal ordered counterpart of this classical relation (see eq. (A.4) in appendix A for an explicit formula). So far one might have the impression that relations arise in orbifolds just because of the Pauli principle. Note that (4.5) also encodes infinitely many relations for orbifolds of bosonic algebras. In order to illustrate these relations and their impact also in the purely bosonic case we briefly comment on a bosonic example. Consider two commuting copies of the Virasoro algebra (L\ and L2) with equal central charge. Then W := L\ — Li is primary with respect to L := L\ + Li- Furthermore, p(L) = L and p(W) = — W is
295
an automorphism of this W(2,2). According to (4.4) the subspace invariant under p is generated, in the classical case, by the following fields: L,
* " := Wd"W
for all even n.
(4.9)
Again, we obtain one generator at each positive even scale dimension. In this case rewriting the relations (4.5) for the redundant set (4.3) in terms of the nonredundant set (4.4) is slightly more complicated. Using the notation Xl'> = W^W^ one checks that from (4.3) 00 01 0 2 0 2 and (4.5a) ^{X^X ' ) = SX^X ' + 2X°' $ X°< and d X°'° = 2X1'1 + 2X°<2. Using (4.5b) it is straightforward to check that d2(Xa-°X0'0) + 6X°'°d2X0-0 + 8A-°'°X0'2 = 0. This relation arises at scale dimension 10, which is the lowest scale dimension admitting a relation. In terms of the generators (4.9) it reads a 2 ( * 0 * 0 ) - 6 * 0 a 2 * 0 + 8*°4 2 = 0.
(4.10)
Turning now to the quantum case one can check that the normal ordered counterpart of (4.10) is not identically zero, but contains correction terms including the scale dimension 10 field $ 6 (the explicit formula is eq. (A.6) in appendix A). This indicates that the Z2 orbifold of the quantum W(2,2) is a W(2,4,6,8) - a finitely generated algebra, which can be confirmed by an inspection of its vacuum character (see appendix A). 5. A classical first class Hamiltonian reduction In order to convince the reader that at the classical level infinitely, nonfreely generated algebras generically arise in all reduction procedures applied to finitely, freely generated algebras, here we present an example of a first class Hamiltonian reduction where this is the case. Our starting algebra will be the DS type W^ -algebra (see e.g. [4]) belonging to the sl(2) embedding S associated to the long root of Q = B^. We next describe the structure of this W^-algebra. The root diagram of the Lie algebra Q = Bi consists of the vectors ± e i , ±e2, ±(ei ±e2), and the algebra is spanned by the Cartan-Weyl basis E±ex,
E±t2,
£±(ei±e,),
Htl,
He,,
(5.1)
normalized by [Hei ,Eei] = Eti. We consider the sl(2) subalgebra 5 = span{M-, M0, M+} belonging to the long root (ei + e2), M± := E±(et+e7h
Mo:=\(Htl+Htl).
(5.2)
296
The adjoint representation of Bi decomposes under 5 as 10 = 3 x 1 + 2 x 2 + 3 and the generating fields of the W^-algebra are the components of the 'highest weight gauge' current, j\n,(x) € Ker (adw + ), parametrized as j h w ( x ) = / + ( * ) £ _ ( „ _ „ , + Io(x)(Htl 1 1 + -Z+(x)Ee, + -Z-(z)Etl
- HC7) + / _ ( * ) £ . , _ „ (5-3) +C(x)M+
.
The fields 7o,± form an s/(2) Kac-Moody subalgebra of the Wj-algebra, {J 0 (x),/ ± (y)} = ± J ± ( y ) 6 ( x - y ) , {/„(*),/o(y)} = ^ ' ( x - y ) ,
(5.4)
{/+(*), J_(y)} = 2I0(x)6(x - y) + KS'(X - y) , where K is a nonzero constant. The fields Z± are bosonic fields with conforms! weight | with respect to the Virasoro L := i (£ + / _ / + + i j ) , and form a doublet under the s/(2) Kac-Moody subalgebra; in particular they have io-charge ± | - This fixes almost all the Poisson brackets. The Poisson brackets of Z± read {Z±(x),
Z ± (y)} = ±2/c [ 4 ( y ) « - 2J ± (y)*'] ,
{Z_(x), Z + (y)} = 2[£ - (/_/+ + II + Kf0)](y)6 + 4KI0(y)6'
- 2**6" .
We are interested in the classical Hamiltonian reduction of this Wf-algebra defined by the first class constraint /+(*) = 0. (5.6) The gauge group generated by this constraint acts according to
h —* h i Z+ —» Z+ , Z . - . Z . -
(5.7) tZ+,
/_ —► /_ - 2el0 + Kt', where e(x) is arbitrary. The problem is just to describe the ring H. of those differential poly nomials in the basic fields L, Io, Z+, Z-, /_ which are invariant under the traasfonnation rule (5.7). By naive counting we expect that the reduced system should have 4 'functional degrees of freedom'. We have the 3 invariant fields L, I0, Z+ and can easily construct a fourth
297
invariant with the aid of the rational gauge fixing implemented by putting e = -g- in (5.7), whereby /_ — > R = ^
with
B~Zll--2Z+Z-I0
+ K(Z'_Z+-Z-Z'+).
(5.8)
The scale dimension 4 differential polynomial B is gauge invariant. Why is our problem not completely trivial? If we were looking for the differential rational gauge invariants then {Io,Z+,L, R} would clearly be a free generating set. However, since it is impossible to make sense of quantum analogues of rational invariants, we are interested in the differential polynomial invariants, and, perhaps contrary to a naive expectation, the set {/o, Z+,L, B} is not a generating set for R. For example, the scale dimension 6 invariant K € R given by K .=
(KB'Z'+
- KBZ1; -
-
2BI0Z'+)
(5.9)
cannot be expressed as a differential polynomial in the set {IQ,Z+,L,B}, be checked to be a differential polynomial in the basic fields.
although it can
Observe also that if we include K into the generating set of R then it will contain the 5 element subset {Io,Z+,L,B,K} subject to the differential-algebraic relation Z+K - KB'Z'+
+ KBZ'I
+ 2BI0Z'+
= 0.
(5.10)
In a sense the problem is to find the higher scale dimension analogues of the invariant K (5.9) and the relation (5.10). It can be shown (for a proof, see appendix B) that the ring H, is generated by the following gauge invariant differential polynomials: L,
Jo,
Z+,
Pi,h
(5.11)
where, for arbitrary nonnegative integers i, j , Pi,i = d'Z+WZ-
- PZ+WZ-
+ -^2V"-1I-
(diZ+d'-aZ+
( ; J -di~'Z+djZ+
(l
(5.12) and V := d — -7o is a covariant derivative. These generators of R are of course not independent. They obey the fundamental nonlinear relations given by PijPkj PijdkZ+
~ Pi,kPj,i + PijPj,k = 0, - Pi,kd>Z+ + PitkffZ+
= 0,
(5.13a) (5.13b)
298
where i,j, ifc, / are arbitrary nonnegative integers, and the linear relations given by (5.14) VPi,j = P,, J + 1 + Pi+u The reader may observe that (5.13-14) are similar to the relations (1.6-8), the reason for this is contained in construction given in appendix B. The generating set (5.11) is redundant on account of the linear relations (5.14), and using (5.14) like in section 1 we can find a minimal generating set, for instance by keeping only the generators Pij, out of the Pij. However, it is unavoidable that the minimal generating set of % consists of infinitely many generators subject to infinitely many relations. For completeness, we also note that the relation given by (5.10) is recovered from (5.13b) by taking t = 0, j = 1, k = 2 and observing that B in (5.8) is just — KPI$, K in (5.9) is proportional to Pi,2, and P^fi = X'Pi.oWe also wish to remark that the reductions related to the so-called W^-algebras, which have been partially treated in the appendix of [4], are very similar to the above example; the invariant ring is infinitely generated in those cases, too. The W22,,-cases and the above example are covered by the more general model when one takes a Kac-Moody or W-algebra that contains an sl(2) Kac-Moody subalgebra and imposes a first class constraint of the type (5.6). We hope to further analyze this class of classical reductions and their quantum analogues in a future publication. 6. Discussion In this paper we pointed out a new class of finitely (but nonfreely) generated deformable quantum W-algebras, which consists of the algebras possessing infinitely generated classical limits obeying infinitely many differential-algebraic relations. The existence of this class of W-algebras has not been noted previously, although part of the results needed was already known in the literature. Our main observation, derived from the examples, is that the infnitely many relations satisfied by the classical generators have the following twofold impact on the corresponding quantum W-algebra. First, using a proper subset of the normal ordered relations one can eliminate the infinitely many 'would-be-generators' in favour of a finite set of quantum generating fields. Second, the generating fields in this finite set are still not independent due to the rest of the normal ordered relations that give rise to generic null fields. These generic null fields are nontrivial normal ordered differential polynomials in the generating fields that exist for generic c and vanish identically on the defining vacuum representation of the quantum W-algebra. As a terminological aside, we propose to say that
299
a finitely generated deformable quantum W-algebra is nonfreely generated if such generic null fields are present. To be precise, we fully demonstrated the above mentioned statements only in the 07 example. In the other examples we treated the first few relations and confirmed by character countings that the pairwise cancellation of classical generators against classical relations should happen upon normal ordering also at higher orders. It is a very interesting open question whether this mechanism works to all orders in every case, or - if not - what are the conditions? At least to our knowledge, no example (including sl(2)/U(l) - see section 3) is known for a quantum coset (or other reduced algebra) obtained from a finitely generated algebra for which infinitely many generators are required to describe the reduced quantum W-algebra. Invariant theory ([11-13]) played an important role in our considerations. That this theory should be relevant for W-algebras derives from the fact that, indeed, all known deformable W-algebras can be obtained by reducing simple free field like linear systems or affine Kac-Moody algebras, and in reductions one is always interested in the invariants. The class of invariants most often considered in invariant theory is the polynomial class and in our context the relevant class of invariants is the differential polynomial class, which is not very different. Since, as we have seen throughout the paper, the generators and relations of the differential ring of classical invariants arising in a reduction know a lot about the generators and generic null fields of the corresponding quantum W-algebra, a more extensive application of invariant theory to W-algebras should be a fruitful undertaking. In this paper we emphasized that in a generic situation the classical coset, orbifold and first class reduction procedures yield reduced classical systems carried by infinitely, nonfreely generated differential rings of invariants. (Incidentally, as far as we know, the classical coset and orbifold reductions lead to infinitely, nonfreely generated classical systems without any nontrivial exception). To avoid confusion, we should also stress that this does not exclude the existence of a (possibly finitely generated) subring closed under Poisson bracket in such a way that only the subring is recovered from the classical limit of a quantum Walgebra resulting from the corresponding quantum reduction procedure. In particular, if the quantum reduction yields a W-algebra which is generated finitely without generic null fields, this is expected to be the case. For instance, this happens for the coset realization of 'Casimir algebras' (W-algebras in the DS class for principal embeddings), which possess finitely, freely generated classical limits (automatically obtained from classical DS reduction). This provides us with an example where in the classical limit of a quantum W-algebra resulting from a quantum (coset) reduction one recovers only a finitely generated subring of the full ring of invariants resulting from the analogous classical (coset) reduction. We wish to mention that in [29] DS type classical W-algebras based on B„ and C„
300
have been recovered from invariant subspaces of those based on some At by 'folding'. In our sense of 'orbifolding' these subspaces are generated by the invariant generators according to eq. (4.4), and thus represent only a proper subring of the classical orbifold. It should also be noted that the quantum orbifolds of the Casimir algebras based on At in general have no subalgebras corresponding to Casimir algebras based on a different simple Lie algebra [22]. Finally, we wish to point out that although the finitely but nonfreely generated class of deformable quantum W-algebras considered in this paper seems to be more complicated than the already reasonably well understood class of W-algebras obtained from DS type reductions, it is also relevant for 'physical' applications. For instance, a universal object for the 2 * parafermions (which have been widely used in the literature — see e.g. [1,23,26]) belongs to this class. Furthermore, in some cases one might want not to include any fermions into the symmetry algebra (for example because they are not observable, or because - from a mathematical point of view - purely bosonic symmetry algebras are sometimes easier to handle), which automatically leads to orbifolds belonging to this new class. The orbifolds obtained from bosonic projection are the chiral algebras of GSO [30] projected models that occur in superstring theory. Acknowledgements We wish to thank R. Blumenhagen, W. Eholzer, K. Hornfeck, R. Hubel, M. RSsgen, W. Nahm, L. O'Raifeartaigh and I. Tsutsui for discussions and for reading the manuscript. We are also grateful to P. Bouwknegt, A. Feingold and M. Scheunert for correspondence and for pointing out useful references to us. JdB was sponsored in part by NSF grant 9309888, and LF by the AvH Stiftung.
301
Appendix A: Details on two quantum orbifolds This appendix contains the normal ordered versions of some classical relations for the orbifolds discussed in sect. 4. The formulae below have been obtained on computer by using the OPE package of [31]. First we study the bosonic projection of the N = 1 super Virasoro algebra. Conventions are fixed by the following OPEs of the energy momentum tensor L and the spin | fermion G: 2 w ?/ \f, s * ( c / 2 k ) dl(w)\ L(z)L{w) = h ' + , V ; 2 + —±-± + reg. , V (z — wp (z — w)2 2—wJ TI ^ , N t (V2G(w) dG(w)\ /A , ,
G{z)G{w)^(^ + \ (z — w)3
2 -M)+reg.. z - wI
In order to be able to compare with the classical case we have explicitly introduced the Planck constant h in (A.l). The normal ordered version of the simplest classical relation $ 1 $ 1 = 0 becomes: ((GdG)(GdG)) = n(192hQ-3lc{G?G) + 7 < C + 1 2 » W 6 ) - I ^ ± ^ ( G 9 G ) \
i/U
- ^-((Gd^G)L)
% £t
i.O
+ ((GdG^L)
+ 3(9 2 (GaG)i)
- 3(d(GdG)dL)
- h\{L*L) - h7-(dlcn) +
h^-JJ^&L
(A-2) Apart from the quantized counterpart (Gd*G) of the classical generator $ on the r.h.s., eq. (A.2) is a polynomial in the energy momentum tensor L and the dimension 4 and dimension 6 generators (GdG) and (Gd^G). Therefore, (G&G) can be ehminated and does not give rise to a new generator. Note that the r.h.s. of (A.2) vanishes in the classical limit h —► 0, as it should. Similarly, normal ordering the classical relation $ 3 $ ' = 0 leads to: 5
((Gc?G)(GdG))
= h(l28h8-25c(G?G)
+
+ ^ ^ ^ ( G d G ) + 5(d2(GdftG)L) -
5
-(P(GdG)L)
c
-±l^&(Gc?G)
- ^{(G*d)L)
+ ^((606)8*1) + k\(L*L)
+
+ h\(dt#L)
20c+
-
lh
2™
-
d<(Gc?G)
6(d(G?G)dL) 7
-(d(GdG)d^L)
-
ft^j"7***). (A.3)
302
Using (A.2) one can eliminate (Gd*G) in (A.3). Apart from the term (Gd7G) both sides of (A.3) are polynomials in the generators of scale dimension 2, 4 and 6. This permits one to eliminate also (Gd7G), which corresponds to the classical scale dimension 10 generator $ 7 . Naturally, the r.h.s. of (A.3) vanishes in the limit h —► 0. Finally, the normal ordered counterpart of (4.8) reads
((GdG)#(GdG)) = h(8{1f~c)(Gd7G) \
+£ ± ^ ^ ( ^ 0 ) -
olo
2\)
+ ^ ± p ^ ( G d G ) - ^((G
+ %(&(C!)L) 3
12
^±^d"(G^G)
- ((6*6)#L) +
^((GdGWL)
6
- 3(5 2 (GaG)a 2 L) -
0
l(&{GdG)dL) D
- l(d*(GdG)L)
+ h£(L&L)
+
+ hheflPL) + h^LPD 2V
'
36v
hj(dLPL)
'
n322c^53h&>l). 10080
I
(A.4) After eliminating (G&G) from (A.2) and (Gd7G) from (A.3) the identity (A.4) is precisely the generic null field at scale dimension 10 in the bosonic projection of the quantum N = 1 super Virasoro algebra.
The quantum version of the W(2,2) obtained from two commuting copies of the Vira soro algebra has the following OPEs: r ^ ? / x = h* ( c / 2 L(z)L(w) +, 2£(«0' + — dt(w)\ ^ + reg. , \ ( z —ui)4 (z - to)2 z—wl
\{z — w)*
(z — w)2
z — wl
where we have again kept the Planck constant. Now one can compute that the normal
303
ordered counterpart of eq. (4.10) is:
&({WW)(WW)) - 6((WW)d2(WW)) + 8((WW)(W'd2W')) = n(*7e-£13h(wdfiw)-
^c+43iVdi(Wdiw) + 7-^^d*{Wd2w) +
z^cP(ww)
+ 20((Wd*W)L) + 36((Wra2Wr)a2I) + 28(d(Wd2W)dL) - 28(a2(Wd*W)L) - A{d{WW)d^L) - 20(d2(WW)d2L) - ^■(d3(WW)dl) + 4(5«(W'W,)L) + hliLtfL) - hl(dL&L) - hliePLpL) + hhanpL) o
o
o
-
hls*%\8089ihd^t].
b
J
. . . . (A.6) Using (A.6) one can express (Wd^W) as a polynomial in the generators L, (WW), (W&W) and (Wd*W). This ensures that the Z2 orbifold of W(2,2) has no dimension 10 generator. Again, the r.h.s. of (A.6) vanishes in the limit h —* 0 and it is not possible to eliminate this generator at the classical level. In the case of W(2,2) we also would like to present a character argument indicating that one does not need new generators at higher dimensions either. Similarly to eq. (2.2), let ^2,4,6,8(9) be the vacuum character of a W(2,4,6,8) without relations. It is straightforward to calculate the character Xo(?) of the submodule of the W(2,2) vacuum module invariant under p. Up to order 29, we obtain for the difference of these two characters Xo(q) ~ 4>2,4,«M = -<212(1 + 2 ? + 5<72 + 9q3 + 295 + 536 + 83q7 + 1 3 V + 214«9 + 340g10 + 510? n + 784 9 12 + 1153g13 + 1720?14 + 2491? 15 + 3634?16 + 5183g17 + C(? 1 8 )). (A.7) All coefficients are nonpositive as expected. In particular, we read off from (A.7) that the first generic null field appears at scale dimension 12. For more details on quantum orbifolds we refer the interested reader to [22].
304
Appendix B: The invariants in the Hamiltonian reduction example In this appendix we show that the generating set of the ring "R. of differential polyno mials in L, Io, Z+, Z-, I- invariant under the gauge group (5.7) is given by (5.11-14) as stated in section 5. We shall do this by a construction which reduces the problem of finding the generating set of "R to a problem in the invariant theory of the group SL(2). Note first that since L does not mix with the other variables under the transformation (5.7), it can be factored out from the problem, i.e., % is generated by L and the invariants depending on IQ , Z+, Z-, I-. Similarly, IQ can also be factored out if we introduce the new variables L:=L,
i0:=Io,
Z+:=Z+,
Z-:=GZ-,
L := GI-,
(B.l)
where G is given by
G(x) := exp (- i I* dt I0(t)\ .
(B.2)
Indeed, in terms of these variables the gauge transformation rule (5.7) becomes L -* L,
i0-*
i0,
Z+ -* Z+,
Z--*Z--
eZ+,
/ _ - » / _ + itde,
(B.3)
with l := Gt
(B.4)
being arbitrary since e in (5.7) was arbitrary. Let P(L, Io,Z+, Z-, I-) be an arbitrary differential polynomial in the original variables and P(L,Io,Z+,Z-,I-) an arbitrary differential polynomial in the new variables. Decom pose P as a sum J ^ t Pk, where Pk contains the terms of degree k, where we assign degree 1 to Z- and J_, and degree 0 to the other variables. Decompose P as P = 2~2k ^* * n *^ e same way. The map F from tilded polynomials to untilded ones defined by F:£pt(L,/o,Z+,Z_,/_)~£G-*Pt(L,/o,Z+,GZ_,G/_) *
(B.5a)
k
is invertibe, and the inverse F~l is given by f" 1
:^flk(L,/o>Z+,Z_,/_)^^C*P/k(Z>/o,Z+lG-1Z_,G-1J_). k
(B.5b)
k
This map naturally induces a one-to-one map between the respective invariant differential polynomials. According to the above, it is enough to describe the differential polynomial invariants in the tilded variables 7_, Z+, Z_ under the transformation rule (B.3), which we now take in its (equivalent) infinitesimal form, 6L = Kde,
SZ+ = 0,
6Z- = -eZ+.
(B.6)
305
It is also convenient to introduce the notation /< l) = S , /_,
C+°:=9i2+,
d°:=^-,
$,:=&€,
(B.7)
and let / , C+> C-i 0 denote the corresponding infinite component vectors. Purely alge braically, the problem is to find the most general polynomial P(C_, (+, I) which is is invari ant under
St1*
= K6W,
6^T = 0, 6^ = -Y,(iy:-m)0m
(B.8)
ro>0
for arbitrary 9. Prom computing the variation of P using the chain rule, P must satisfy K-
dP
^
1 1
a/t" - )
n\M-m)
dP
„
£(^?^
/
„
dP
(-« ^y-)- <">
Consider now the decomposition of P according to the different powers of / , given by 8 P = £ Q
r
where
Q r (C-,C + ) A/) = A r Q r (C_, C+,/),
(B.10)
r>0
which leads to a refined form of (B.9), namely,
*a7(^-L(^J<+
^ 7 ) = ° ' (r = 0,l,...).
(B.11)
This implies that every invariant polynomial P is uniquely determined by its /-independent term Qo- On the other hand, taking m = r = 0 in (B.ll) we obtain that Qo is subject to
£CI°S = 0,
(B.12)
and the point is that this equation has a simple group theoretic meaning. To see this take the standard action of the Lie algebra sl(2), with generators E, H, F, on the variables Q. ,
*-ci° = Ci°,
«»Ci.° = o,
*FCi 0 = d , ) ,
* F d 0 = 0,
**d" = d'\
«»d° = -d'\
(B.13)
and extend this by the Leibniz rule to an action of s/(2) on the ring of polynomials in the infinitely many doublets Q'. Clearly, (B.12) just defines the subring of 'highest weight polynomials', i.e., the kernel of Sg. Using the representation theory of sl(2) it is not hard The new letter Q is used since this decomposition is different from that in (B.5).
306
to see that the kernel of SE is generated by the pairwise symplectic scalar products of the different doublets and the highest weight components of the doublets themselves, given by «,,>:= C i
0
^ - d°dJ),
Vijtj,
and c i ' \ V/.
(B.14)
(For instance, one can observe that the polynomials depending on a finite subset of the doublets and having definite degrees of homogeneity in those variables are an invariant subspace and using this one can show inductively that (B.14) indeed generates the kernel of 6E)- One can also easily verify the relations wij + witi=0,
(B.15)
w%,jv>k,i - Wi^Wjj + Wijw^k = 0,
mjtf
- «x.*C+:) + t»>,*C+> = o,
(B.16)
(B.17)
which are analogous to (1.6-7) in section 1. Moreover, if we write tf> = wk}00 = ci* ) Cl° o) - C(-k)<:ix) with
d ° ° ) := 1, Ci°°) := 0,
(B.18)
and let the indices r, s, p, q run over the nonnegative integers and oo, then we can uniformly write (B.15-17) as l»r,, + W.,r = 0,
(B.19)
U>p,«UV,« - WPtrWqi, + WPl,Wq
(B.20)
Then we can apply the 'straightening algorithm' given in Chapter 3 of [13] to show that (B.19-20) imply all the relations satisfied by the generating set (B.14) of the ring of 'highest weight polynomials'. More precisely, this would be true if the variables Q. were indepen dent, but now we have the derivation 3 Q / = Q. , which implies the extra linear relation 5Wr,5 = U>r+1,» + U>r,»+1-
(B.21)
At this point the solution space of (B.12) is fully under control and to derive the generating set of the gauge invariant differential polynomials all one has to do now is to follow the above construction backwards. First one solves the recursion relation ( B . l l ) taking any of the elements in (B.14) for Qo- Using also (B.7), this then yields the generating set of the invariants under (B.6). Then one returns to the original variables by means of (B.5). At the end of the day, one obtains Pij given by (5.12) from u>ij in (B.14) by this procedure. Moreover, one can trace back the relations given by (5.13-14) to corresponding relations in (B. 19-21). Since it is completely straightforward from here on, we omit the details of this derivation of the statement of section 5.
307
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P. Bouwknegt, K. Schoutens, W-Symmetry in Conformal Field Theory, Phys. Rep. 223 (1993) p. 183
[2]
P. Bowcock, G.M.T. Watts, On the Classification of Quantum W'-Algebras, Nucl. Phys. B379 (1992) p. 63
[3]
J. de Boer, T. Tjin, The Relation between Quantum W Algebras and Lie Algebras, preprint THU-93/05 (1993), IFTA-02-93, hep-th/9302006, to appear in Commun. Math. Phys.
[4]
L. Feher, L. O'Raifeartaigh, P. Ruelle, I. Tsutsui, On the Completeness of the Set of Classical W-Algebras Obtained from DS Reductions, preprint BONN-HE-93-14 (1993), DIAS-STP-93-02, hep-th/9304125, to appear in Commun. Math. Phys.
[5]
L. Feher, L. O'Raifeartaigh, I. Tsutsui, The Vacuum Preserving Lie Algebra of a Classical W-Algebra, Phys. Lett. B316 (1993) p. 275
[6]
H.G. Kausch, G.M.T. Watts, A Study of W-Algebras Using Jacobi Identities, Nucl. Phys. B354 (1991) p. 740
[7]
W. Eholzer, A. Honecker, R. Hiibel, How Complete is the Classification of WSymmetrxes?, Phys. Lett. B308 (1993) p. 42 7
[8]
K. Hornfeck, W-Algebras with Set of Primary Fields of Dimensions (3,4,5) and (3,4,5,6), Nucl. Phys. B407 (1993) p. 237
[9]
F. Delduc, L. Frappat, P. Sorba, F. Toppan, E. Ragoucy, Rational W Algebras From Composite Operators, Phys. Lett. B318 (1993) p. 457
[10] I. Bakas, E. Kiritsis, Beyond the Large N Limit: Non-Linear yVx as Symmetry of the SL(2, R )/U(l) Coset Model, Int. Jour. Mod. Phys. A7, Suppl. 1A (1992) p. 55 [II] H. Weyl, The Classical Groups, Their Invariants and Representations, Princeton, New Jersey, Princeton University Press (1946) [12] R. Howe, 'The Classical Groups' and Invariants of Binary Forms, Proc. Symposia Pure Mathematics 48 (1988), p. 133; Remarks on Classical Invariant Theory, Trans. AMS 313 (1989), p. 539 [13] J. Kung, G.-C. Rota, The Invariant Theory of Binary Forms, Bulletin of the AMS 10 (1984), p. 27 [14] F.A. Bais, P. Bouwknegt, M. Surridge, K. Schoutens, Extensions of the Virasoro Al gebra Constructed from Kac-Moody Algebras Using Higher Order Casimir Invariants, Nucl. Phys. B304 (1988) p. 348 [15] P. Goddard, W. Nahm, D. Olive, Symmetric Spaces, Sugawara's Energy Momentum Tensor in Two Dimensions and Free Fermions, Phys. Lett. B160 (1985) p. I l l 7
Note that a remark on the classification of 'exceptional' W-algebras in this reference is slightly misleading because it was not recognized that W(2,8) at c = — ™ and c — — 3 | | * are related to minimal models of the Casimir algebras of E% and E-j respectively.
308
[16] J. de Boer, L. Feher et al, in preparation [17] P. Bouwknegt, Extended Conformal Algebras from Kac-Moody Algebras, Proceedings of the meeting 'Infinite dimensional Lie algebras and Groups', CIRM, Luminy, Marseille (1988) p. 527 [18] P. Goddard, A. Schwimmer, Unitary Construction of Extended Conformal Algebras, Phys. Lett. B206 (1988) p. 62 [19] P. Bowcock, P. Goddard, Coset Constructions and Extended Conformal Algebras, Nucl. Phys. B305 (1988) p. 685 [20] R. Blumenhagen, W-Algebren in Konformer BONN-IR-91-06 (1991)
Quantenfeldtheorie,
Diplomarbeit
[21] J. Balog, L. Feher, L. O'Raifeartaigh, P. Forgacs, A. Wipf, Toda Theory and W-Algebra from a Gauged WZNW Point of View, Ann. Phys. 203 (1990) p. 76 [22] R. Blumenhagen, W. Eholzer, A. Honecker, K. Hornfeck, R. Hiibel, Cosets and Uni fying W-Algebras, BONN preprint, in preparation [23] V.A. Fateev, A.B. Zamolodchikov, Nonlocal (Parafermion) Currents in Two-Dimen sional Conformal Quantum Field Theory and Self-Dual Critical Points in ~Z.s -Sym metric Statistical Systems, Sov. Phys. J E T P 62 (1985) p. 215 [24] F.A. Bais, P. Bouwknegt, M. Surridge, K. Schoutens, Coset Construction for Extended Virasoro Algebras, Nucl. Phys. B304 (1988) p. 371 [25] V.A. Fateev, S.L. Lukyanov, The Models of Two-Dimensional Conformal Quantum Field Theory with Z„ Symmetry, Int. Jour, of Mod. Phys. A 3 (1988) p. 507 [26] F. Ravanini, Informal Introduction to Extended Algebras and Conformal Field Theories with c > 1, preprint NORDITA-89/21P (1989) [27] H.G. Kausch, Chiral Algebras in Conformal Field Theory, Ph.D. thesis, Cambridge University, September 1991 [28] A. Honecker, A Note on the Algebraic Evaluation of Correlators in Local Chiral Con formal Field Theory, preprint BONN-HE-92-25 (1992), hep-th/9209029 [29] L. Frappat, E. Ragoucy, P. Sorba, Folding the W Algebras, Nucl. Phys. B404 (1993) p. 805 [30] F. Gliozzi, J. Scherk, D. Olive, Supersymmetry, Supergravity Theories and the Dual Spinor Model, Nucl. Phys. B122 (1977) p. 253 [31] K. Thielemans, A Mathematica Package for Computing Operator Product Expansions, Int. Jour. Mod. Phys. C 2 (1991) p. 787
311 Reprinted with permission from International Journal of Modem Physics A Vol. 3, No. 2, pp. 507-520,1988 © 1988 World Scientific Publishing Company
THE MODELS OF TWO-DIMENSIONAL CONFORMAL QUANTUM FIELD THEORY WITH Z. SYMMETRY V. A. FATEEV International Centre for Theoretical Physics, Trieste, Italy* and S. L. LYKYANOV Landau Institute for Theoretical Physics, Moscow, USSR Received 20 August 1987
An infinite set of conformally invariant solutions of the two-dimensional quantum field theory, possessing a global symmetry Z, is constructed. These solutions can describe the critical behavior of Z, symmetric statistical systems.
1. Introduction One of the main problems of the second order phase transition theory is the classification of all possible types of critical behavior and the calculation of the corresponding critical exponents. If one accepts the hypothesis of the conformal in variance of the large-scale critical fluctuations1-2 this problem reduces to the con struction of all conformally-invariant solutions of the Euclidean quantumfieldtheory. Several infinite series of such solutions have been recently found in two dimen sions.3-14 Some of them are shown to describe the known critical (or multicritical) behavior of various two-dimensional models including Ising model3 and its Z„ general izations,4 the Ashkin-Teller model,6 etc. There is even hope of constructing in this way something like a "periodic table" of the two-dimensional critical and multicritical phenomena. The solutions found so far possess as a rule infinite dimensional symmetries which are richer than conformal invariance itself, and include the Virasoro algebra [L B ,LJ = (n - m)Ln+m + — (n3 - n)Sn+m,0
(1.1)
as a subalgebra. Examples of these symmetries are superconformal,7-8 N = 2 extended supersymmetry,5,911 "parafermionic"4,510 and Kac-Moody12 symmetries. Recently in the paper13 the series of the exact solutions possessing the symmetry * Permanent address: Landau Institute for Theoretical Physics, Moscow, USSR
312 508
V. A. Fateev <* S. L. Lykyanov
generated by the conserved current W3{z) of spin 3 was constructed. In this paper we introduce the infinite series of exact conformally invariant solutions having the addi tional symmetry generated by conserved currents Wk{z) (k — 3,4,..., n) of spin sk = k. These currents together with the stress-energy tensor T(z) form a closed operator algebra (Wm algebra). The models of this series possess global Z„ symmetry and are indexed by two positive integers n and p (n = 2,3,...,p = n + I, n + 2,...); we denote them as [Z<"]. The central charge C in (1.1) for these models takes the values
and the spectrum of anomalous dimensions of Wn invariant ("ancestor") fields is given by the formula Afl/I') = A(/,
U/».'
W
12 ["l (Ph - (P + 1)/,>«T - «(«2 - 1) 24p(p + 1)
(1.3a)
Here /,, // (i = 1,..., n — 1) are positive integers satisfying the inequalities: I/,J£P;
Z V S P - 1 ;
(l.3b)
and vectors a>, (i = 1,..., n — 1) are the fundamental weights of the Lie algebra sl(n), subjected to conditions mk
for k <, s.
(1.4)
The ancestor fields <&(///') having the dimensions (1.3) together with their "descendents" form a closed operator algebra. Its structure qualitatively corresponds to the idea of treating the sets of integers (/) = (/,,...,/„_,) and (/') as the highest weights of a finite-dimensional representation of sl(n). The correlation functions of the fields (///') are given in terms of multiple contour integrals generalizing the Feigin-Fuchs integrals.14,17 The models [Z„(rt] contain some known solutions. So, the models [ Z 2 W ] coin cide with the models [Afp] 3,16 connected with strongly degenerate representation of Virasoro algebra; the models [Z 3 (r> ] were constructed earlier in Ref. 13 and the models [Z„("+1)] coincide with the models [Z,,]* which describe the critical behavior of Z, Ising models. We think that models [Z„
313 The Models of Two-Dimensional Conformal Quantum ...
509
exactly correspond to the critical exponents which characterize the critical points of "solvable lattice models whose states are dominant integral weights of /l,,.,' 1 '" constructed in a recent paper.20 2. The Structure of Wm Algebra Let us consider two-dimensional conformal quantum field theory, which involves besides the right and left components of stress energy tensor T(z) and T(z) also the set of conserved local currents Wk(z)(W;(z)) (k = 3,4,..., n) with spins sk = k (Jk = -k). The fields Wi(W^) depend only on variable Z = x, + ix2 (Z = x, — ix2), i.e. have conformal dimensions (fc,0)(0,&)). It will be convenient for us to denote the field T(z) by W2(z) (f(z) = W2) and also identity operator / by W0. In the sequel, we shall concentrate our attention on the right components Wk(z), keeping in mind that left components Wk(z) have the same properties. Let {A} be the space of localfieldsforming an operator algebra for some quantum field theory and H^zJejA}, k = 0, 2, ..., n. In this space one can introduce the operators Wk(s) (s = 0, ± 1,..., ± 2) by means of the operator product expansions: Wk(s)A(z,z) = (j) ^ ( C - xrk-lWk{r)A{z,z).
(2.1)
Here A is anyfieldbelonging to {A} and integration is performed over a small contour encircling point z. We assume that the operators Wk(s) form an associative algebra (W„ algebra) with nonlinear commutation relations of the following kind: [H51(»i),W{1(s2)]=
£ •i
ftJ,lI'A"l'(si.s2l«i,-,«F)Hi1(«i).-»5>,)
£ ip " l
(2.2a)
«fi
where the integers u,,..., up are subject to the conditions: £ u, = s, + s2,
Mj £ u2 £ • • • £ up
(2.2b)
and if«, = u,+1, then i, > il+1. (The products of type (2.2a) usually are called as normally ordered; in the sequel we shall denote them by the symbol::.) We also suppose that the structure coefficients b of this algebra satisfy the following restrictions: (i) The operators W2(s) = L, form a subalgebra (1.1); (ii) The coefficientsfr/,'/,"'"are different from zero only in the case where: I h :£ h + h ~ 2, (*'t
'Vii.J2 ^ ");
(2-3)
(Hi) The coefficients b}&; ''(0,0|0,... ,0) = 0; (2.4) (iv) If in this algebra we choose a basis in such a way that all fields Wk(z) with k = 3, ..., n will be primary conformal fields, normalized by the conditions (Wi(z)Wk(f))y =
314
510
V. A. Fateev A S. L. Lykyanov Q
&lz~1} ■ - then all the structure coefficients b will depend only on one free parameter which is the central charge C in (1.1). We note that the above restrictions (i)-(iv) generalize the properties of W3 algebra constructed by Zamolodchikov in paper 15 by direct solution of associativity condi tions (Jacobi identities). For n > 3 such a method for constructing an example of W„ algebra seems to be extremely complicated; therefore we shall satisfy the Jacobi identities by constructing the exact representation of nontrivial Wn algebra in the universal covering algebra of the Heisenberg algebra. To do it we introduce (n — 1) component free massless scalar field $(z,z) — +(z) + $(z), if = (^,..., ^..j) with the two point functions = -25 y logz
(2.5)
j
z'
(s = 0,±l,...)
(2.6a)
which form the Heisenberg algebra [fliteiW^)] = ^jS,5 5l+JJi0 .
(2.6b)
Let us define in the universal covering algebra H„_, of algebra (2.6) the system of fields Wk{z) (k = 0,2,..., n) in the following way. We consider the formal differential operator
where the symbol:: denotes the normal ordering of the fields $(z) and the n vectors h, (i = l,...,n) form a overcomplete system in (n — l)-dimensional Euclidean space, satisfying the conditions J>« = 0, hrhj = 5u-l/n.
(2.8)
Using the usual rules for the commutation of differential operators we can represent the product R„ in the form
315 The Models of Two-Dimensional Conformal Quantum ... 511
Rn = lWk(z)(iz0j2£j
*
(2.9)
which determines completely the fields Wk(z). In particular
*-j;^*-o
(no)
W2 = \ Z :(K-d,M*j-dM
+faot (» - fc)M,2* = - ^ ( A * ) 2 : + foopd2*
where the vector p = 1/2 £ (n+ 1 -2fc)ht
(2.11)
*=i
p2 =
n(n 2 _ 1 i)
(212)
One can easily check that the field W2(z) = T(z) defined by Eq. (2.10) generates the Virasoro algebra (1.1) with a central charge: C = (n - 1) - 24a0p2 = (n - 1)(1 - 2n(n + l)ag).
(2.13)
The correct asymptotic behavior T{z) ~ z"* as z-* oo3 which is necessary for conformal symmetry to be unbroken, can be set up by imposing appropriate asymp totic conditions for the field <^(z): ♦(z)~2«« 0 logz
(2.14)
where at,, = a0p. di, In the classical case the transformation (2.7)-(2.9) from the fields u, = —- to the fields oz Wk(z) is known as Miura transformation. The properties of this transformation are described in detail in the review 18. In particular, it follows from the results contained C dz in this paper that the Poisson bracket for the variables Wj(s) = (n — z*+* ' Wj(z) can be expressed in a bilinear form; i.e. represented as" * The authors are obliged to T. Hovanova and V. G. Drinfeld for having attracted their attention on this important point
316
512
V. A. Fateev AS.L.
Lykyanov
'l'l «l+»2-»l+»2
where i, + i2 £ j t + j2 - 2 and fc/^O, 0/0,0) = 0. (Here the bracket (2.15) is calculated using the Eqs. (2.6) where in (2.6b) we have to change the commutator to classical Poisson bracket.) The quantization of the fields Wj(z) leads to the deformation of coefficients b in Eq. (2.15) and to the changing of the usual product to the normally ordered product of operators Wj{s). The calculation of commutation relations for the operators Wj(s) will be described in detail in our sequal paper. Here we shall write only the commutators of operators W^s) with the operators L, = W2(s) and W3(0) which give us the possibility to prove that fields Wj(z) generate the quantum Wn algebra and to determine all coefficients b in (2.2) using the associativity condition. [L„ Wj(k)l = (p(j - 1) - k)Wj(p + k) - t (i«oV2Yin~J\fAJP.,Wj-,(P
+ k)
(2.16a)
[_W3(% WJLk)] = 2*0,.. - \)WJ+l(k) + (J2ia0)(2j - 3 + k)k\Vj(k)
n,=i
in— jy.
{j,--a>
+ BlWj_Jk)\.
(2.16b)
Here the coefficients A'p%1, ££,, C£ are: „_p(p-l)-(p-q+l)
^ • ' " C , + ' V 4n a 0 2
J + l
2
) (2.16c)
K, = (-ncstr + (q;i+'(-)* - cj«2) v
/«-i
i
._,_,
( n - i ) ( g - i)\
where in the last formula: k = 2i for even k and 2i — 1 for odd k. The corresponding coefficients b in Eq. (2.15) can be obtained from Eqs. (2.16) if we put in the Eq. (2.16c) a 0 = oo.
317 The Models of Two-Dimensional Conformal Quantum ...
513
3. The Space of Fields of Wm Invariant Quantum Field Theory and the Free Field Representation The space {A} of local fields in Wm®Wn invariant quantum field theory can be classified in terms of representations oiWH®Wn algebra i.e. decomposed as
M} = ©[•,],
(3-D
where [O,,] denotes an irreducible representation of W„ x Wn. Each of the subspaces [,,] contains one "ancestor"field
(3.2)
with some number parameters wk(y) and wk(y). The set of numbers [w(y)] s [w2(y)... w »(?)]> [w(y)] characterize completely the representation [Oy] = [[»v(y)]]. The subspace [y] consists of thefieldsgenerated from the "ancestor" field
ft,)
(3.3a)
where 1, i f £ f t = 2a0 (3.3b)
G(Pi,.,ftv)= < 0, if £ ft #21*0.
One can easily check that the fields Vt(z) satisfy the Eqs. (3.2) with the parameters [w(|l)] which are determined by the most singular term in the operator product expansion: Wk(z) Vf(0) = ^
K,(0) + 0(z-*+1).
(3.4)
It follows from Eqs. (2.7) and (2.9) for thefieldsWk(z) that the numbers w»(fl) can be obtained from the relation:
318 514
V. A. Fateev A S. L. Lykyanov
If we apply the Eq. (3.5) to the functions *Pj = z* (j = 0,1,..., n — 2) we shall obtain the system of linear equations for the parameters wk(f): (iyfir fl [(» - m + ; > 0 - K K = t 7T^Tr7(«a0^)*»v(,.*(P). m-0
(3.6)
*-0 (J — K)\
The solution of this system has the form: w*(P) = (-«V2)*
£
n(«o(*-™) + K / » .
(3.7a)
in particular w2(P) = A(P) = p 2 - 2 « 0 p .
(3.7b)
We note that the left-hand side of Eq. (3.6) is invariant under the following discrete transformation of the parameters p -»P': h « P + ao'n = h IB 'p + a0m',
(3.8)
where numbers m' are obtained from the numbers m = (1,2,..., n) by some permuta tion PeS„. So, it is the n\ different values of parameters P that correspond to the given set of numbers [w(P)]. In particular [w(P)] = [w(2ot0 — p*)], where vector p* is defined by the relation: P* h, = p h ^ .
The transformation p->2<x0 — p* corresponds to the permutation (l,2,...,n)-» (n,n- 1.....1). The representation [
4. Completely Degenerate Representations and Kac Spectrum Almost all known solutions to the conformal quantum field theory are associated with degenerate representations of additional symmetry algebras (see Refs. 3, 8, 10, and 13). Therefore it seems to be important to study the degenerate representations of Wn algebra. We shall say that representation [
319 The Models of Two-Dimensional Conformal Quantum ...
515
of fields, obtained by the application of the operators Wk(s) with s < 0 to the "ancestor" field
for n > 0
(4.1) L0XH = W2XN = (A +
N)xs
where the positive integer N is called the degeneration level. If a null vector appears it should be set equal to zero since otherwise the representation [^[w]] will be reducible. In this way we shall obtain an irreducible degenerate representation [4>[w]] which does not contain fields corresponding to the null vector and its own descendents. Certainly, if there is more than one null vector one should set each to zero. We shall call "completely degenerate" the representation [
where the vectors e, (y = 1,..., n — 1) form a basis in the system of positive roots of Lie algebra sl(n) and are determined by the relations: ei = h i - h j + 1 ;
e,-e, = 2 5 u - ^ + l i J - ^ M + 1 ;
e.-fy = <5U - 5 j + 1 J ; e,- • p = 1. (4.3)
If the parameters a± satisfy the equation: <x+ + a_ = a 0 , a+ • a_ = —1/2
(4.4)
then the operators Q]±] commute with all the operators Wk(s). To prove this statement it is enough to show that the singular part of the operator product expansion of the fields Wk(tj) and V}{±)(z) - :cfa*eJ*I): can be represented in the form: WMV/^z)
= ^Xfati)
+ 0(1)
(4.5)
or RMVj{±\z)
= ^ J£ x'JLz,i,)^
+ 0(1).
(4.6)
320
516
V.A.Fateev&S.L.Lykyanov
To calculate the operator product expansion (4.6) we note, that differential operators d — act only on the variable t\ and that according to Eq. (4.3), only the two successive drf ( h, dh\( h,+. 5A\ rd r terms:: I ia.0J2— H—'-= • — 11 ia v 0 J2 + -*-= • —- I: in the product R. will give a conV di\ Ji dftj\ Ji di\) tribution to the singular part of this expansion. One can check directly that if param eters oc± satisfy the Eqs. (4.4) then we have:
4((^S
+ (1)
(4.7)
°
from this it follows that the operator product expansion RH(tf) Vf ± \z) has the form (4.6). Using the operators Qj±} which commute with operators Wk(s) one can construct in a standard way the null vectors x*,(P)e[j] = [tp] and obtain in this way the corresponding restrictions on the parameters p. This procedure for the case of W3 algebras is described in detail in paper 13. The generalization to the case with n > 3 is trivial. So, we shall write here only the equations for the parameters 0 which correspond (modulo the transformation (3.8)) to the completely degenerate representa tions of WH algebra. These equations have a form: e, P = ot+(/ - I,) + «_(/ - /DO' = 1,...,« - 1)
(4.8)
where /„ /,' are positive integers. In the case when Eq. (4.8) is fulfilled the representation [ty] will contain (n — 1) null vectors XN,(P) with degrees of degeneration N, = /,/,'. The solution of the Eq. (4.8) can be written in the form:
« / m = P('i
/.-ii/;,...,/;-,) = "f («+ o -/,) + « - ( i -/,'))«„
(4.9)
where the vectors o, (i = 1,..., n — 1) determine the fundamental weights of Lie algebra sl(n), satisfying the conditions: («,•€,) = «„.
(4.10)
By inserting the vectors P into (3.7) we obtain the sets of numbers [w(///')] which determine the Kac spectrum of completely degenerate representations of the W„ algebra. In particular the anomalous dimensions of completely degeneratefieldshave the form:
321 The Models of Two-Dimensional Conformal Quantum ...
A(//P) = w2(///') = P f (/,a+ + /;<x_)«J2 - « 0 2 .
517
(4.11)
5. Correlation Functions, Operator Algebra and "Minimal Models" Let us denote byfl>(///')the completely degenerate "ancestor" fields
(5.1a)
where we have temporarily omitted the dependence on the variables zt. The free field representation of Wn algebra and the "ancestor" fields <&(///')-► Vf(lin(V2ao-fWn) allows us to construct, in the standard way, (see Refs. 13, and 14) the integral repre sentation for correlation functions (5.la). In fact, this correlator up to a multiplicative normalization constant can be represented by the following integral:
<wz t )...w^nfff<$><w + >««>)ffctdtfirw)), (5ib> }=\ \
«=i
j
where in (5.1b) the freefieldexpectation value (3.3) is implied. P(i) denotes either P(/,//,;) or 2«0 — p*(/(//|), and the integration is performed over some nontrivial manifold which is closed on the Riemann surface corresponding to the multivalued function integrand in (4.2). The correlation function (5.1a) does not vanish provided the integers Mit M', in (5.1b) can be appropriately chosen to satisfy (3.3b), i.e. £ m + «+ 1 Ma + a_ "f Mfr = 2« 0 . i=i
j=\
(5.2)
j-i
Let us associate with everyfield
(5.3)
i-i
If the parameter p = 2<x+ is irrational then Eq. (5.2) can be satisfied only if Z„ charges q± are conserved i.e.: I « ± ( i ) = 0 (mod.n).
(5.4)
The analysis of correlation functions (5.1) shows that degenerate "ancestor" fields
(5.5)
322
518
V. A. Fateev dS.L.
Lykyanov
The sets of numbers (s/s') which contribute to the right-hand side of Eq. (5.5) at fixed sets (///') and (m/m') determine the "selection rules" or the "qualitative structure" of the operator algebra. The qualitative structure of (5.5) corresponds to the idea of treating the sets (///') and (m/m1) as the highest weights of the finite dimensional representations of sl(n) x sl(n). The fields <&(///') are associated with the corresponding representations of sl(n) x sl(n) whereas the operator product expansion (5.5) has the same "qualitative structure" as the associated sl(n) x sl(n) Clebsch-Gordon decom position. For the case n = 2, 3 these "selection rules" were obtained in Refs. 3,13. In general, the operator algebra (5.5) involves infinitely many completely degenerate fields $(///')• But there is a possibility to get a closed operator algebra with a finite number of irreducible representations of W„ algebra, i.e. the "minimal model" of WH invariant field theory. Namely, it can be shown that if the quantity p — 2ai = — takes positive rational values P= ^
(5.6)
where p and p' are relatively prime positive integers, the space of fields
M}=
©
©
[*(*//')]
(5.7)
I?:,' /,*/>'-1 L"-i'.' * P - '
form a closed operator algebra. The similar fact is known for the other models of conformal quantum field theories associated with degenerate representations of addi tional symmetry algebra (see Refs. 3,10, and 13). If the condition (5.7) is satisfied then we have to do the following identification of the fields
(5.8)
where
('*)
=
(«II—k + l»*n—* + 2» — »*fi-l»P' ~~ 2 ^ *i»*l» — »'«—*—l) i=l
w) = (/;-*+i, /;-*«. • • • J.-i. P - "f ii, i[
/;_»_!>
<=i
because these fields have the same values of parameters [w]: !>(///')] = lw(lj',)l
s=l
n - 1.
(5.9)
The identification (5.8) provides additional restrictions to the "qualitative structure" of (5.5) which, in particular, shows that minimal model (5.7) closes as operator algebra.
323
The Models of Two-Dimensional
Conformal Quantum ... 519
The "main series" of the minimal models corresponding to the choice p' = p + 1 in (5.6) is of special interest. We denote these models with p = n + 1, n + 2,... as [Zl)
0(//n-exp(^9(///')W/')
(5-10)
where q(l/l') = kq+(l) - (k + \)q.(l'). 6. Discussion In previous sections the infinite set of conformally invariant solutions to the twodimensional quantum field theory possessing global Z„ symmetry was described. The important problem basically involved so far is to describe a class of statistical systems having the critical behavior [ZB(P']. We plan to discuss this problem in a following paper. Here we note only that the simplest (at fixed n) models [Z,,"^1'] have a central charge
n+ 2 and coincide with [Z„] models, constructed earlier in Ref. 4. These models describe, in particular, the critical points of Z„ Ising models. In this case the following "ancestor" fields <&(///') (modulo the identification (5.8)) in the model [ZB'"+ "] correspond to the spin fields ak and thermal operators £0) of the model [Z„]:
., n — l
[It = 1,1 = 1, . . . , / i t - 1 .
324
520 V. A. Fateev 4 S. L. Lykyanov ™ ■ /n . , . k(n — k) . ^ j(j + 1) The fields ak and e u ' have the dimensions dk = — — — and D^ = 2nfn + 2) ' n+2 correspondingly. Acknowledgments
The authors are grateful to A. Belavin, V. Drinfeld, B. Feigin, T. Hovanova, A. Zamolodchikov and S. R. Wadia for many fruitful discussions. One of us (V. F.) is grateful to Professor Abdus Salam for kind hospitality at the I.C.T.P. in Trieste, where this work was finished. References 1. A. M. Polyakov, Pis ma Zh. Eksp. Teor. Fiz. 12 (1970) 538 (JETP Lett. 12 (1970) 381). 2. A. Z. Patashinski and V. L. Pokrovskii, Fluctuation Theory of Phase Transitions (Pergamon, Oxford, 1979). 3. A. A. Belavin, A. M. Polyakov, and A. B. Zamolodchikov, Nucl. Phys. B241 (1984) 333. 4. A. B. Zamolodchikov, and V. A. Fateev, Zh. Eksp. Teor. Fiz. 89(1985) 1575. 5. A. B. Zamolodchikov, and V. A. Fateev, Zh. Eksp. Teor. Fiz. 90 (1986) 1553. 6. Al. B. Zamolodchikov, Zh. Eksp. Teor. Fiz. 90 (1986) 1675. 7. M. Bershadsky, V. Knizhnik and M. Teitelman, Phys. Lett. B151 (1985) 21. 8. M. Eichencher, Phys. Lett. B151 (1985) 26. 9. P. Di Vecchia, J. L. Petersen and H. B. Zhang, Phys. Lett. B162 (1985) 327. 10. A. B. Zamolodchikov, and V. A. Fateev, Teor. Mat. Fiz. 71 (1987) 163. 11. W. Boucher, D. Friedan, and A. Kent, Phys. Lett. B172 (1986) 316. 12. V. G. Knizhnik, and A. B. Zamolodchikov, Nucl. Phys. B247 (1984) 83. 13. A. B. Zamolodchikov, and V. A. Fateev, Nucl. Phys. B280 (1987) 644. 14. VI. S. Dotsenko, and V. A. Fateev, Nucl. Phys. B240 [FS. 12] (1984) 312; Nucl. Phys. B251 (1985) 691. 15. A. B. Zamolodchikov, Teor. Mat. Fiz. 59(1985) 108. 16. D. Friedan, Z. Qiu, and S. Shenker, Phys. Rev. Lett. 52 (1984) 1575. 17. B. L. Feigin, and D. B. Fuchs, Funktc. Anal. Pril. 16 (1982) 47. 18. V. G. Drinfeld, and D. B. Sokolov, VINITI24 (1984) 81 (in Russian). 19. P. Goddard, A. Kent, and D. Olive, Phys. Lett. B152 (1985) 88. 20. M. Jimbo, T. Miwa, M. Okado, "Solvable Lattice Models Whose States are Dominant Integral Weights of i4„_„" Kyoto University preprint RIMS-572 (1987).
325
Reprinted with permission from Sov. J. Nucl. Phys. Vol. 49, No. 5, pp. 925-932, May 1989 © 1989 American Institute of Physics
Exactly soluble models of conf ormal quantum field theory associated with the simple Lie algebra D„ S. L Luk'yanovandV.A. Fateev L D. Landau Instilutt ofThtorttical Physics (Submitted 10 June 1988) Yad. Fiz.49,1491-150* (May 1989) We construct a class of exactly soluble models of two-dimensional conformal quantum field theory, which describes certain critical points of RSOS sutistical systems, associated with the D, series of simple Lie algebras. The infinite-dimensional symmetry algebras of these models are obtained by quantization of the classical Hamiltonian structures of generalized KdV equations.
1. INTRODUCTION The group of conformal transformations in two dimen sions is infinite-dimensional and therefore A. M. Polyakov's hypothesis on conformal invariance of critical fluctuations' turned out to be the most fruitful in the investigation of criti cal behavior of two-dimensional statistical systems. The space of fields of two-dimensional Euclidean field theory, equivalent to the sutistical system at the point of phase tran sition of the II kind, may be classified in terms of irreducible represenutions of the Virasoro algebra [t,, £,,]-
(1.1)
which generates the conformal transformations of the mod e l Among the irreducible represenutions of the algebra (1.1) one may single out the so-called degenerate represen utions. 2 J Their properties are reminiscent of the finite-di mensional represenutions of simple Lie algebras; in particu lar there exists an analog to the usual Clebsch-Gordan decomposition of two irreducible represenutions. This per mits the construction, for particular values of the central charge c of the Virasoro algebra (1.1), of exactly soluble models of conformal quantum field theory, containing a fi nite number of degenerate represenutions.M They are usually denoted as \MP ] ( p — 3,4). Soon after the publica tion of the ground-laying paper by A. A. Belavin, A. M. Potyakov, and A. & Zamolodchikov3 a class of sutistical systems was constructed whose critical behavior was de scribed by these models.5* However, the models \Mr) cer tainly do not exhaust all classes of critical behavior. At this time a large number of exactly soluble models of two-dimen sional conformal field theory have been constructed which are different from [M, ] . ' " " They are all characterized by possessing, along with the conformal invariance connected with the energy-momentum tensor, additional symmetries generated by conserved currents. The following were consid ered for the symmetry algebra: the superconformal symme try algebra,'•* its Af = 2 extension,*"" and the symmetry generated by parafermionic currents""'3 and by the KacMoody algebra.14 A large class of exactly soluble models [Z,"\ (p = n + 1,...) was constructed in Ref. 15, which include a substantial number of previously known solutions, for example the [Mr ]-models, the Z. -models with parafer mionic symmetry, and the Z,-symmetric models construct ed in Ref. 16. The [Zj/*] solutions of conformal quantum field theory are endowed with a large algebra of additional symmetries, which contain, along with the energy-momen tum tensor, conserved local currents { Wk (z)}, _^ _. with 925
spins sk = k, and are connected with the simple Lie algebra /*„_,. Sutistical systems corresponding to the [ Z i " ] models were constructed in Ref. 18. The aim of this article is the construction of the class of models [D',"] (n =4,5,...; p = 2n - 1, 2n,...) of confor mal quantum field theory associated with the simple Lie al gebra D,, whose additional symmetries are generated by lo cal currents/Hz) and {If „ (z)}».,,..j,_i with spins * = « and s = 2k (A = 1 n — 1) respectively. In these models the central charge c of the Virasoro algebra (1.1) Ukes on the value c-n(l-(2n-2)(2/ 1 -l)/j>(()+l)), (1.2) and the spectrum of anomalous dimensions of the primary fields is determined by the relations A(l|n-A(t
'.I'.'
'.'-)
- ^ [ I ] , >!,-0>+l)l.')».]' - ( n - l ) n ( 2 n - l ) }/l2p(p+i),
(1.3a)
where the positive integers/,,/,'(/- 1,...^)) are constrained by the conditions l,+2Xi'.+'.-'+'.
'.'+22ji,'-H.'-,-H.'«;p, (1.3b)
and the vectors u, constitute the fundamental weights of the Lie algebra Dm. The matrix of scalar products of the funda mental weights of the Lie algebra Z>., needed for the calcula tions using formula (1.3a), has the form tt*«>w*»mt
Km
U>M.-,-«.B.-*/2,
K*
•».-,«.— (n-2)/4;
•„'—».'-,—n/4.
(1.3c)
The primary fields
326
Z, m Zt group for even n and with the Z4 group for odd n. The [D1."] models describe the critical behavior of the statistical systems recently constructed in Ref. 20. They also include a number of previously known solutions. Thus, the [D'.1"] models may be reduced to the Z*,-models of Ising, l2 and toe [D'mu-l>] models describe special cases of the critical behavior of the Ashkin-Teller" model.
By making use of this notation the Poisson bracket associat ed with the simple Lie algebra D, may be written in the following elegant fashion23: ((,, M - 2 T r [ ( / ? r ) . ( R X ) ] , (2.6a)
2. THE STRUCTURE OFTHE WO. ALQEMA
where the symbol P+ for the pseudodifferential operator />(x) = Z«; 0 .. t />,(x)</
In the papers of Reft. IS and 20 it was demonstrated on the example of the Gel'fand-Diki bracket that the quantiza tion of symplectic structures connected with integrable nonlinear equations gives rise to non trivial algebras, which turn out to be useful for the construction of exactly soluble mod els of conformal quantum field theory. For this reason we shall briefly describe the Poinon structure associated with the simple Lie algebra />,. A detailed discussion of this ques tion may be found in the review in Ref. 22. We therefore consider the formal rafndodifferential operator
*(«)-*.(*)+/<*) (-^ )"/<*).
(2.1a)
{X„ l,)-TTlRXf(dltlx)-'i).
(2.6b)
{).., X,)-'/.Tr[fl((d/<Ji)-'«],
(2.6c)
M«)-Z».w(^)'.
The simplest proof that the bracket defined by (2.6) satisfies the Jacobi identity makes use of the Miury transfor mation:
/M-[(-l>"(£+f.M)...(^+fc<»>)]-l. ,d
(2.2) This means, in particular, that in the set { W, (x)},.,___,. _, only (» - 1) fields are independent On the space of func tional! of the form
)-J
V ( / 0 - idzFU.W
tP„-,),
(2.3)
whereFisa polynomial in the variables/tx) and Wk (x),the Poinon structure may be detned by specifying the bracket for an arbitrary pair of linear functional!. It is straightfor ward to verify that an arbitrary linear functional of/tr) and Wk (x) may be represented in the form V < « ) - M / ) +Mfl.), where
(2.4a)
X.(/)-Jdx«(x)/(x),
(2.4b)
/d
\
■•■(■S-frM).
X- E ( ^ ) '"«.(*)•
It is obvious that the pseudodifferential operator (2.8b) sat isfies the relations (2.1) and (2.2), i.e., the transformation (2.8) specifies the imaging of the set of fields { ? * ( * ) } * _ i _ » , defined on the segment [ - 1,1],into the system/tx), {*"« (*)}, which also contains n independent functions. The remarkable property of the Miury transfor mation is the fact that it is Hamiltonian, which means that if one specifies on the system offields{ ?»OOh _!...„. the sim ple Poisson bracket {?.(*), ! , ( » ) > - « « 6 ' ( x - » ) ,
(2-9)
then upon the transformation (2.8) it will go over into the nontrivial relations (2.6). An analysis of the relations (2.6) and (2.8) leads to the following natural method of quantization of the Poisson structure (2.6) associated with the simple Lie algebra Z>„. Let us denote by v, the algebra over C with generators ak (*), * «= 1,..., it, i€ Z, satisfying the commutation rela tions [a,(«), «,(«)]-2u8„., Aiy (2.10) In the algebra y, one may construct the n-component massless scalar field «>(z) — (f>, (z),..., e>„ (z))
(24c)
le Adler functional Tr P for the pseudodifferential opera■P(x) -Z ( ^,(x)(
»>
(2.8b)
a<»,(»)
,, , V
,.
01
h-TiiRJC],
(2S
•am-**)-
«.«-(ir + £^«(in <«« AW—*♦(*)- (± ) " " - £ ( - ±)""~W.M.
v
* W - ( ^ + , . W )...(-+,.(x))
where
The functions fix) and Wk(x) (* - 1....M - 1) are smooth images of the [ — 1,1] segment in C Let the differ ential operator A,(x) satisfy the adjoint condition
(2.7)
(2.11)
In the following it will be convenient to make use of the operator product concept. We recall that the operator prod uct of the fields A (z) and * ( f ) is defined by the condition
,,llim.MW»(t),
W>l*l.
(2.12)
(2.5) The commutation relations (2.10) are equivalent to the fol
ia*
Sev.J.Nuct.Phys.4*(5).Msy19a9
S. LLuk'yanovandV.A.FaM«v
B2«
327
lowing operator product of the fields f',{z) 9<'U)<»i'(S)
andojj(f):
2(i-S)-'o„+ : v'(<)v/<e> : •
(2.13)
Here the colon to the left and right denotes normal ordering, i.e., operators a , U ) with » < 0 entering the product :«?,'(x)yy'(f): are placed to the left of operators ak («) with u>0. Let r„ denote the universal enveloping algebra of y,, i.e., r . is generated by all possible dements of the form :a,(ij)...fl|(j ; ', )...a. isZ)...a, ( £ ) : . In T. we construct the field /[*) according to the formula
The commutation relations for the operators At) and/lu) may be obtained by making use of the singular part of the operator product (2.13):
(■-n-1
x{
ta-iA-i
I I (»-2*-u-0+ I I
(n+f-ojWu(«+■»)• (2.20)
,W.[:(iri+^M)...(ip^ Atwrttonl.
+ 2"V(*))=] •!•
(2.14)
In view of the problem of ordering of the operators a, (j) it turns out to be difficult to use the relation (2.8b) for the construction of the quantum fields Wu (z). We shall there fore define these fields by generalizing formula (2.6c). Let us consider the singular part of the operator product/U)/t£).Itcon tains poles of order no higher than In and is a symmetric function of z and £. By making use of elemen tary induction one shows readily that the singular part of the operator product f{z)f[§) can be represented in the form
/M/UW-lHs-W'M. +£<-l)"*(«-5)-"—'^.-.(W-W+^WHOU). a—I
i~l,
(2.1J)
which unambiguously defines the (a — 1) fields { i y u (*)}»- 1..J.-1Tbe numerical coefficients {^t h - i _ _ * - i are chosen by considerations of convenience and determine the normalization of the fields { Wu (*)}» _ , „ . _ i • Let us set fc-t
^. - I I [2<(2«+i) •2a.*-il;
f2-")
then, for example, W.it) •/.: (•'(«))■: +lo*»"(s). The vector p satisfies the relations
Z
,
,.
,
(n-l)n(2n-l)
(2.17)
,, .
(«-()«•, P' — , (218) where {a,}, _,_..,. is an orthonormal basis of the n-dimensional Euclidean space R,. Let 04} e T. be the space of local fields. The fields {/(*), W u ( z ) | * - 1 « — 1} 6 C4}determineasetofop erators WD. -{WltU),A')\k-\ «-l;»6Z}with the help of the operator expansions W*WA(i)-f£-(\-t)»*-lWm<\)A{i), MA(i)-fP-(\-t)'*-'l(\iA(t). 927
Sov J Nod PHvK«(5).M»y 1999
(2.19a) (2.19b)
(/(•). W » ( » ) l -
:/0>)HV«M :
£
(2.21)
f>f.»+'-<*■
where C,, ( ?) are numerical coefficients and the symbol ■A P) Wm (r): denotes normal ordering, i.e., l
"
Wm(r)f(p),
p>r.
The commutation relations (2.21) constitute the quan tum analog of formula (2.6b). This means that in the limit aj — oo the commutator of the operators, [ / W . Wu (») ] . goes over into the classical Poiason bracket of the corre sponding linear functionals. The commutation relations [ W-u W,Wu (u) ] maybe determinedfromformulas(2.20) and (2.21) and the associativity condition of the algebra WD.. Using formula (2.17) it is not hard to show that the operators Lk m W, (*) form the Virasoro algebra (1.1) with central charge e-n-2V<«.,-'t(l-4a.,(A-l)(2n-l)).
(2J3)
Relation (2.21) was verified on a number of special cases, however we do not possess at this time a complete proof of it. It is nevertheless possible to prove a remarkable property of the operators of the WD. algebra, which to a large extent determines their utility in the construction of exactly soluble models of conformal quantum field theory. Aaacrtloa 2. The operators/l*), Wu (*) e WD. commute with the set of operators {Qj * ' } , _ , _ , e T.: (?;*'- f d, V<" ( « ) . f it: . x p l i a ^ d ) ] =; e
(2.24)
c
here the parameters a t satisfy the relations <x*+a--a„ o.ou—'/;,
(2.25)
and the vectors {tl)l.i _, constitute a system of simple positive roots of the simple Lie algebra D., i.e., e,-o,-<j,.„ / - I e.-e.-.-t-o..
n-1;
(2.26a) (2.26b)
It follows from formula (2.20) that it is sufficient to prove the assertion for operators /fa), seZ We begin with the case./ — n. For the proof of the equality «?:*', / ( ' ) ] - 0 , f«Z, (2-27) it is sufficient to show that the singular part of the operator product of the fields Av) »nd Kl*'(*) = :exp[uz t e„*U) J: can be represented in the form S.L.Luk'yanovandV.A.FaHev
927
328
/ ( i ) ) V i * ' ( i ) - — X(z,„)+0(1), at
z~n.
(2.28)
In order to develop the operator product /(17) Ki* '(z) we make use of Wick's theorem. Here it is necessary to take into account the fact that in view of the relation (2.26b) the fields e„«)(z) entering the operator V'.1 '(z) have nonzero con tractions with only the last two factors :(-fa„-2" 2 cV <Ji7 + 2" " V . - , (»7»2" " V ; (»): in the product/! 17). It is not hard to see that if the parameters a t satisfy the rela tions (2.25), then
(±^1-^V-
W
— i - l £ W + 0 ( 1 ) . (2.29)
from which follows the result that the operator product /(17) Ki*'(z) has the form (2.28). The proof of the relations [#*'■/(•) 1-0, J < » - 1 . ««Z, (2-30) is in essence no different from the case,/ — n. This happens because the additional term — iaji/pj{.rf) + q>/+, (17))^/ dn, which is present in the product :( — iait-2,nB/d>i + 2 - " V ; ( i 7 ) X - i « o - 2 , " a / f t 7 - r 2 - " V ; - . e 7 > f c . has zero contraction with the field *>•<» fy ~ f>« 1 S.REmUEIlTATKMSOFTrCraaHtYrWUaHT VECTOR OFTHE HP. ALOEBHA, STRONQLV OeQEMERATE REPRESENTATIONS In this Section we will discuss representations of the WD. algebra. The most interestingfromthe point of view of physical applications are the representations of the highest weight vector." The space of such a representaion [ ♦ » ) is generated by the WD, -invariant (primary) field ♦ , , which satisfies the equations /(«)®,-rT,(t)«»,-0, * - l n - l j «>0; /(0) *■-/«>,; Wu(0)«,—»»«>,
(3.1)
with certain numerical parameters/and wlk. The set of pa rameters S, - {/, uij, I* - 1 « - 1} completely deter mines the representation [
One may verify that the fields V,{z) satisfy equations (3.1). i.e., are WD, -invariant fields (4>(<5.) - V,). Assertion 3. The set of parameters { . ( 3 ) constitutes an independent system of symmetric polynomials in the vari ables 6, = ( 3 - a 0 p ) , K ( P — a , ) , (/'= 1 n), invar iant with respect to the action of the Weyl group of the sim ple Lie algebra D.. The parameter / i s the coefficient of the most singular term in the operator product /(z)V,(0)-/z"V',+O(z—•),
1-0,
(3.5)
and therefore
M 2* T i " 2%,pH • • •( 2*T«7-^'H •' -{-Z-tyJlitMn-Da.).
(3.6)
Upon making use of the definition of the vector p, Eq. (2.18), the relation (3.6) may be rewritten in the form /-(-2*«)"9,...e.. (3.7) The symmetric polynomial (3.7) is invariant with respect to all possible permutations of the parameters 6, and transfor mations 6, xx -$, ( i f y ) . The totality of such transforma tions forms the Weyl group of the simple Lie algebra D,," which we shall denote in the following by V(D,). In order to demonstrate that the numbers { » a } » . I . J , . I are also symmetric polynomials, invariant with respect to the group V(D,), we make use of the fact that the fields { Wj* ( * ) } » _ ! „ , _ , are connected with the singular part of the operator product/U)/U), Eq. (2.15),
/■to/(W-II : [(7-2-^ + «VM-2-») x ( ^ 2 * i j + oy($).2-»)-(s-5)-].l.
(3.8)
Consequently, the numbers {wu },.,___. _, satisfy the rela tion
X
(T 2 £-2'''V'f.)-<'-H •»
- Z (-1>~M.-.(z-j)-"-"u>„(i-»+6-")+0(D-
<M».).. • Vt, '=*)>- 11 (S,-!,)*^ where
(3.9) 1,
G(p„.
...w-
H
■ 0,
928
2jp,_2o#,
2_iPH'*2a4>
Sov.J. Nud Phys.49(5), May 1989
(3.4b)
After going over from the variables z and £ to the variables x, andx, z-expx„
5-expi,,
(3.10)
the formula (3.9) takes on the form S. L Luk'yanov and V. A. Fateev
928
329
tation of the highest-weight vector is irreducible. We shall call the representation [
xsh'"-'(*,-*,) +0(1), x,-x,.
(3.11)
In this fashion the numbers iv u can be determined by com parison of the coefficients of different degree of singularity in the expression
(-»-n((iri)'+(2*fr-V)., - ( - D - i (-iri>.[(^2»l)'+(2Shi-)""P i -J],2 s "- , * , (-l)" _ 4 ^.-.»ttCbfcx$h , , 4 -" , x+{?(l), x-x,-xt-0.
(3.12)
Here
P.(9,»
8.')-
2 J •<"•••*?.
<313>
e^-o.(l-/,)+a-(l-I,'),
This completes the proof of assertion 3. Because the order of the group V(D.) is 2" - 'n! it fol lows that there are 2"" 'nt values of the parameters p corre sponding to a given set of numbers 8m. In particular, the group element I , € V(D,)
I_I
corresponds to the transformation 0—2a, - P*. where the vector P* is defined by the relations
(-1
n,
(3.19)
where /, and /,' are positive integers. When relations (3.19) are satisfied the representation [ Vg ] will contain n indepen dent null vectors with degrees of degeneracy N, = /, /;. The solution of Eqs. (3.19) may be represented in the form
aam-Ki
„_2* : , , - l{ "" « - « * + * • * - f „ l-»-2*+l.
( 3 1 8 )
with some integer N (degree of degeneracy). In that case the representation turns out to be irreducible. In order to obtain an irreducible representation we should set the vector Xn together with the entire subspace [%N ] equal to zero. The representation [ ♦ ( 5 , ) ] may contain several independent vectors XH, (X/t, < [XN, ] • <W) • I" order to make the repre sentation irreducible it is necessary to factor the space [ ♦ ( 5 . ) 1 by all subspaces [xit, ] • We shall call the represen tation [4>((5,)] strongly degenerate if it contains no fewer than n independent null vectors. The operators Q\± ' (j= 1 n) introduced in Sec. 1 permit the construction of the null vectors ^JV( P) in a stan dard manner, leading to restrictions on the parameters P corresponding to strongly degenerate representations. The corresponding procedure for the WA, algebra was described in detail in Ref. 16. We therefore present here only the equa tions for the vectors p which define the strongly degenerate representations of the WD, algebra:
are elementary symmetric polynomials in the variables {'*}<_ i_« • I" particular, A-ll>,-^,-2a#-e*-a.,. (3.14)
p-_p, K
n-l: »>0);
W.(0)x»-(o+A')x»etc.,
tt
'.-.i'.'
c.)
■
-Z,ia,(l-J,)+a-(l-J/)l«.,
< 3M >
where the vectors u, are the fundamental weights of the simple Lie algebra D, and satisfy the relations •>*,-«*
(3.21)
In accord with assertion 3 proved above, the numbers 5, = {w2k, f\k = 1 (i — 1) are independent symmetric polynomials in the coordinates 8,, invariant under theaction of the Weyl group V(D,) on the vector 8 — — 2 r . i (<*»'. +<*-'')•»( i for example:
(3.16)
A(/|I')-Wi(«IO-[]C (a.'. + «-'i')"i] -<*•*• <3-22'
The representation [ ♦ „ ) = [*(.5,)] = [ ^ ] of the WD, algebra in r , may be constructed by applying to the primary field Vf the operators/! j). Wlk (j) withj<0. Here one must also identify the representations [ Ve ] with (V r ], for which the vectors P and P' are related by the equations
Since the entire Weyl group can be generated by the reflections S, (j = 1 n) through hyperplanes orthogonal to the simple positive roots ey (Ref. 23): i,3-?-(e^)e,. i-\ n, (3.23)
P-0.-.S (&-<«.), 4 - V ( D . ) .
(3.17)
for example [ U l a a l K ^ . f . ] . The most important problem of representation theory is
it follows that the sets of integers obtained from the set Vi I','},i. i. ....; '< i',' > 1 by the action of the basis transforma tions S, correspond to the same values of the numbers w2t a n d / We note that
clarification of the circumstances under which the represen ts
Sov.J. Nud. Ptiys. 4» (5). May 1989
S. L Luk'yanov and V. A. FatMv
929
330
S,{W)-Ur^MU-Cj;),
(3.24)
where C„ is the Cartan matrix of the simple Lie algebra D,, and no summation over the index y is intended. 4. OPERATOR ALQEBRA AND CORRELATION FUNCTIONS Or STRONGLY DEGENERATE FIELDS We consider the two-dimensional conform*] quantum field theory containing, beside the energy-momentum tensor which generates conformal transformations, chiral sets of conserved local currents { / U ) . " ' « U ) | * - 1 » — 1} and {J[l), Wu (I)I* = 1 n - 1} with spins » ( / ) - it, r ( l * ' u ) - 2 * a n d j ( 7 ) - = - i , * ( f f \ » ) - -^respective ly. The fields/(x), Wu (*) (7(1), WM (I)) depend on the variable i«x, + i t , ( I • x, - ix,) only. We assume that thefieldsfrom each set generate a closed WD. algebra. The space of fields of the WD, • WO.-invariant field theory may be classified by the irreducible representations of the WD, • WD, algebra, i.e., represented in the form Ml-
(4-»>
S l«>l*..*.)l.
where [4(6.2,)] denotes the irreducible representation of the WD. • WD, algebra. Let us denote by * ( / | / ' ) the strongly degenerate pri maryfields4><0. (/ |/'))and consider the L-point correlation functions of the form <w(i,|J.';s.)...w(li|li';iO>. (4.2a) where we have omitted the dependence on the variables I,. The representation of the WD, algebra and the invariant tMt*U\l')-yt(iU; (Ps*-f ( /i/'> )in terms of free fields, described in the previous Section, permits the construction by standard methods of an integral representation for the correlation functions (4.2a)." The correlator (4.2a) may be, accurate up to normalization, associated with >
"t
{nnk",c(t|") X n^n,l"vr'(n.'")V(,(i,)...V,t(Jt)),
(4.2b)
where the expectation value in (4.2b) is carried out in accor dance with formula (3.4), 0 ( 0 denotes either 0(/, |/J) or 2a, — 0* (/, |/,'), and the integration is over noncontractible contours closed on the Riemann surface of the integrand. The correlation functions (4.2b) are nonvanishing if it is possible to choose integers At,, At', 0 — 1 n) in such a way that the condition (3.4b) is satisfied:
L «-i
yi
<4-3)
f>
? ( 0 + O . 2 J H^+OL-ZJ Af/e,-2o.. >-i >«i
If (i is odd, then we associate with the field 4>(/1/') one Z4charge q*. and one 2^-charge ?_: ♦(')-2 £ (»-«.)*-2 + »('.+'.-i) (mod4), (4.4b) ? . ( J ' ) - 2 X | (l-i.')*-2+n(J.'+;.'-,) (mod4),
Let the numbers o + and a_ be incommensurate. It is then easily verified by multiplying both sides of Eq. (4.3) by to, (j— ],..., n) and using relations (1.3c), (3.21) that the con dition of integrality for the numbers M, (M \) requires con servation of the Zj-charges q'l'"' ( q'l'-'") for n - Ik, or the Z^-charge q+ ( q_) for it «• Ik + 1, i.e., i
H «"'"' 0)-0(mod2),
n-2k,
(4.Sa)
(-• 5Lo.O)-0(mod4),
n-2*+l.
(4.5b)
»—t
An analysis of the correlation functions (4.2) shows that the fields 4>(/|/') form a closed operator algebra, i.e., that the operator product expansion of thefields♦ ( /1/') and 4>(m|m') at nearby points may be represented symbolically in the form q>(l\n
C(';,T.'1,1„-,[w(«|«')l.
(*•«)
where the expression in the square brackets includes the con tribution offieldsbelonging to the representation |
For even n we associate with each field
S. MINIMAL MODELS
« 1 " ( ' ) - Z (l-«*(mod2),
If the numbersa., ando_ satisfying relation (2.25) are incommensurate, then the operator algebra (4.6) contains fields 4>(/1/') for all possible sett of numbers (/) and (/'). If. however, the parameters a+ and a . satisfy the relation
q? ( 0 - l . + l . - . ( m o d 2 ) , (4.4a)
V-" V')-Yi
030
q?' ( / ' ) - < . ' + C (mod 2).
Sov. J. Nud. Phys. 4» (5). May 1969
2o."
aja--plp,
(5.1)
where; and/)' are relatively prime integers, then afieldtheo ry can be constructed containing afinitenumber of primary S. LLuk'yanovandV.A.FatMv
930
331
fields
,(',
'.i'.'
• • .,1.1!.'
'.')-c i/-..I/+J>
',-,,vy,... V), / - I
"■
(5.2)
and the group turns out to be isomorphic to V(Dn) X * „ , where r . - { X « / ? „ UpZ, j-i,..., n)-Z»,+...+Za„ (5.3) is an Abelian group and the symbol X denotes the semidirect product. To describe the finite set of fields forming the closed operator algebra, we need certain facts about groups relating to the root systems of simple Lie groups. The proof of the assertions given below can be found in the book, Ref. 23. Let us denote by I", the free Abelian group r.-{XmR„
X»,«Z, / - I
(Xu.)e,-t,>0.
d];!,'«,)e,-V>0,
f-l
*-l
element I e AfV(X) such that 2 1 € C„, where C, denotes the closure of the open manifold C, £ X„, i.e., the chamber C„ is a fundamental region for the action of the group AJVIX) in the Euclidean space R,. In order to construct the fundamental region for the action of the group V(X) X FT, it is necessary to make use, along with assertion 4, of the following property: Tm/ T. sC(Jf), where C(X) is the universal center of the Lie algebra X In the case of the/J. Lie algebra C(X)=Z, » Z, for n even and Z4 for n odd. Therefore the fundamental re gion for the action of the group V(X) X r „ in the Euclidean space R, consists of the chamber Q , in which the identifica tions generated by the universal center have been performed. The fundamental region for the group C ( f l , ) x r . turns out to be closely related to the finite sets of fields that form the closed operator algebra associated with the simple Lie group D,. Namely, analysis of the structure constants (4.6) shows, in the case when the numbers o , and a _ are commensurate, Eq. (3.1), that the set of strongly degenerate fields with the numbers (/1/') restricted by the conditions Yi '.<■>.(-«.)-1.+2C+ ■ • • +'.-.) + ! . - . + ! . < » ' - 1 . Sov. J. Nud. Phy». *» (9). May 1969
n,
(.1
(5.5) forms a closed operator algebra (minimal model). Here it is necessary to carry out in the chamber (5.5) the identifica tions due to the action of the universal center, which is iso morphic to Z4 for the case n = Ik + 1 and consists of the four elements 1, R,R *,R \ while for n even it is isomorphic to Z, • Zf and generated by R2 and Q. Here the identifications R and Q are defined by the relations Hi
W
O - C -
- ! , - , - ! . , M/...
k.p'-l,-2{k+...+l.-.)
(,',»-/■,'
-2((.'+...+C)-C-!.',i,'), (/
l.\l.' -;..,-;. i C
'.')-(/..
(„p'-i,-2 (!,+ ...+!„-,)
i,-, B _( 1 '_2(j 1 '+... +C)
-i'.-,-v). (5.6)
n)-Ze,+ . . . +Ze., (5.4)
where {e,} ; _ ,.__. now denotes the system of simple positive roots of the simple Lie algebra X, normalized by the condi tion e2 = 2. The group V(X) X1%. where K(X) is the Weyl group of the Lie algebra X, a called the aSne Weyl group AfV(X). Let the vector — e„ —m.e, + ••• + /n„e„ (m, are positive integers) denote the highest root of the Lie algebra X. It is clear that — e,, is the highest weight of the adjoint representation of the Lie algebra X. The manifold C„ e R, satisfying the conditions C0 — {f e R„ fe, >0, / = 1 n; {(. — ej) < 1} will be called the fundamental chamber of the group AfV(jr). Assertkra 4. For an arbitrary vector Ij € R, there exists an
931
H!,'«,(-e,)-J,'+2(V+...+'.'-i)+J.'-.+J.'«;»-l,
Of greatest interest from the physical point of view is the "principal series" of minimal models, corresponding to the choice p'=p+ 1. In that case the parameter a2, = (o» + 0 O 2 — \p(.p+ 1) and the central charge c in (2.23) takes on the value (1.2). By employing the method developed in Ref. 24 it can be shown that minimal models of the principal series with /> =« 2n — 1, 2A,... satisfy the positivity condition.4 We denote such models by [ £ . " ] • The [ £ „ " ] models contain spinless local fields 4>(/|/') with di mensions A ( / | / ' ) , determined by the formulas (1.3). We note that as a consequence of the parameters s t and a_ being commensurate and of the identifications (5.6), the separate conservation of the plus and minus charges (4.4) is violated in the minimal models and only certain linear combinations are conserved, which for the [ £ , " ] models are given by: q'"-"'(l\l')-mql"-'" ( 0 - ( m + l ) , L " " ' (1"), m-J>(mod2),
<5-7a>
n-2*;
9 (l|r)-"><;.U)-(m-l-t)iJ-(0.
m-p(moAi).
n-2k+t. (5.7b)
At the same time the operator algebra of these models is invariant under the transformations 4>(l|n-e*p(juy l -'")®Uin. n - 2 * ;
(5.8a)
®(i|n-exp(Y«)(l|0,
(5-8t>)
n-2*+l.
In conclusion the authors take this opportunity to ex press gratitude to A. A. Belavin, V, G. Drinfel'd, A. B. Zamolodchikov, B. L. FeTgin, and T. G. Khovanova for useful comments and discussions. S. L Luk'yanov and V. A. Fatasv
931
332
'A. M. Polyakov. Pb'ma Zh. Eksp. Teor. Fit 12. 538 (1970) (JETP Lett 12,311 (1970)]. "B L. Fdfjn and D. B Fuks, Funku. AnalU It. 47 (1982) | Functional Analysis 16. 114(1912)]. 'A. A Belavin, A. M. Polyakov, and A. B. Zamokxlchikov, Nucl. Phys. B241,333(I9M). 'D Friedan, Z. Qiu, and S. Sneaker, Phys. Rev. Lett. 52,1575 (1914). 'O. F. Andrews. R 1 Bailer, and P. J. Forener. J. Statist Phys. 3S. 193 (1984). *D. A. Hue, Phys. Rev. B 30, 3908 (1984). 'M. Bershadaky, V. Knizhnik. and M. Teitelman, Phyt Lett. 1S1B, 31 (1985). *H. EidMakerr, Phys. Lett 131B, 26 (198S). •P. Di Vecchia. J. L Pettnen. and R B. Zhenj, Phya. Lett 1(2B. 327 (1985). "W. Boucher, D. Friedan, and A Kent. Phya. Lett. 172B. 316 (1986). " V. A. Fateev and A. B. Zamnlnrtrtlkov, Zh. Ekap. Teor Fir. M, 13S3 (1986) ISov. Phya. JETP(3,913(1986)). "V. A. Fateev end A B. ZarnntnnVhikov, Zh. Ekap. Tear. Fix. M. 380 (1985) [Sov. Phya. JETP(2,215(1985)]. "V. A. Fatecv and A. B. Zanolodchikov, Teor. Mat. Fix. 71.163 (1987) [Theor. Math. Phya. (USSR) 71.451 (1987)).
932
Sov.J. NJd. Phys. 4»(5). May 1969
"V. G. Knizhnik and A. B. Zamolodehikov. Nucl. Phya. B247. S3 (1984). "S. L Luk'yanov and V. A. Fateev. Zh Ekap. Teor. Fit 94. 23 (1988) ISov. Phya. JETP (7,447 (1988)]. "A. B. Zamolodrhikov am) V A Fateev. Nucl. Phya. B280,644 (1987). "A.B Zamokxlchikov. Zh Ekap.Teor Fu 90.1808(1986) (Sov.Phya, JETP (3. 1061 (1986)]. "M. Jimbo, T. Miva, and M. Okado, Mod. Phya. Lett. B1, 73 (1987). "V. S. Dotaenko and V. A. Fateev, N»cL Phyt. B240.312 (1984); B2S1, 691 (1985). " E Date, M. Jimbo, T. Miwa, and M. Okado, Kyoto Univ. preprint. Rima-S9c 1917. "S L Luk'yanov, Funkta. Analiz 22. 1 (1988). "V. O. DrinfeTd and V. V. Sokolov, Sovremennye problemy matematiki (Contemporary problems in mathematica), VINIT1. Moacow. 1984, p. 81. : 'M. Goto and F. Grocahaaa, Semiaunple Lie Algebras, M. Dekker, New York, 1978 (Ruts. Iran*)., Mir, Moacow, 1981). "P Ooddard, A. Kent, and D. Olive, Phya. Lett 1S2B, 88 (1985). Translated by Adam M. Kneer
S. L. Luk'yanov and V. A FatMv
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Reprinted with permission from Communications in Mathematical Physics Vol. 126, pp. 49-83,1989 © 1989 Springer-Veriag
Hidden SL(n) Symmetry in Conformal Field Theories Michael Bershadsky and Hirosi Ooguri* The Institute for Advanced Study, Princeton, New Jersey 08540, USA
This paper is dedicated to the memory of Vadik G. Knizhnik Abstract We prove that an irreducible representation of the Virasoro algebra can be extracted from an irreducible representation space of the SL(2,$) current algebra by putting a constraint on the latter using the Becchi-RouetStora-Tyutin formalism. Thus there is a SL(2,0t) symmetry in the Virasoro algebra, but it is gauged and hidden. This construction of the Virasoro algebra is the quantum analogue of the Hamiltonian reduction. We then are naturally lead to consider a constrained SL(2,&1) Wess-Zumino-Witten model. This system is also related to quantum field theory of coadjoint orbit of the Virasoro group. Based on this result, we present a canonical derivation of the SL(2,3t) current algebra in Polyakov's theory of two-dimensional gravity; it is a manifestation of the SU2,9t) symmetry in conformal field theory hidden by the quantum Hamiltonian reduction. We also discuss the quantum Hamiltonian reduction of the SL(n,0t) current algebra and its relation to the Wn -algebra of Zamolodchikov. This makes it possible to define a natural generalization of the geometric action for the WB-algebra despite its non-Lie-algebraic nature. 1. Introduction Among various favourable properties of string theory as a candidate for the unified theory of everything, the uniqueness of target spacetime dimensions is one of the most appealing. It is therefore crucial to know whether string theory is possible off the critical dimensions. This question is also relevant in understanding the large-Nc limit of QCD in four dimensions, and many attempts have been made to solve string theory below criticality. Kazakov and Migdal [1] have studied various statistical models on triangulated random surfaces, and computed scaling dimensions. Last year Polyakov examined the two-dimensional gravity induced
* On leave of absence from Department of Physics, University of Tokyo, Tokyo 113, Japan
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M. Bershadsky and H. Ooguri
by conformal field theory, and found that there is an SL(2,0l) current algebra [2]. This result opened the way to solve the off-critical string theory. Later Knizhnik, Polyakov and Zamolodchikov exploited this observation to evaluate scaling dimensions of planar random surfaces [3]. Their result shows complete agreement with previous computations by Kazakov and Migdal. This seems to suggest the validity of Polyakov's observation. Still, the way the SL{2,M) current algebra emerges is like a bolt out of the blue. He computed correlation functions of metrics using the Ward identity of the energy-momentum tensor, and showed that they contain the SL(2,31) current algebra. One of the motivations of this paper is to obtain a canonical derivation of this current algebra and to understand the structure of the off-critical string theory. It has been suspected by several people that there should be hidden relations between the Virasoro algebra and the SL{2,3t) current algebra, and in general, between the W^-algebra and the SL(n,0l) current algebra. The W^-algebra is an extension of the Virasoro algebra with additional chiral operators of spin-n [4]. For example, Fateev and Lykyanov [5] computed highest weights of completely degenerate representations of the WB-algebra, and found that they can be expressed in terms of highest weights of the SL{n,3f) algebra. There is also an intriguing connection with the classical version of these algebras observed in the context of the Korteweg-de Vries type Eqs. [6]. Consider a dual space of the SL{n,3t) loop algebra. This space is endowed with a natural Poisson bracket, and we may regard it as a classical phase space. This phase space has a certain symmetry, and one may consider the reduced phase space with respect to this symmetry. The Poisson bracket for the reduced phase space turns out to be the classical version of the W„-algebra. This procedure is called the Hamiltonian reduction. In this paper, we develop the quantum analogue of the Hamiltonian reduction. We replace the Poisson bracket by a commutation relation of operators, and the classical phase space by an irreducible representation of the algebra. An attempt in this direction was initiated by Belavin [7]. The irreducible representation spaces of the Virasoro algebra are extracted from those of the SL(2,#) current algebra by imposing a certain constraint on the latter. Consider an irreducible repre sentation space of the current algebra. In classical mechanics, we put a constraint J"(z)= 1 to reduce the phase space of the loop algebra. Quantum mechanically, we introduce a set of ghosts and define the Becchi-Rouet-Stora-Tyutin (BRST) operator associated with this constraint. It is then proved that a quotient Ker(QBRST)/Im(QBRST) is isomorphic to an irreducible representation space of the Virasoro algebra. The idea of our proof is the following. Both the Virasoro algebra [8] and the SL(2,#) current algebra [10] have realizations in terms of free bosons. Although such realizations are highly reducible, there are BRST-like operators whose cohomologies are isomorphic to irreducible representations of these algebras [12,13]. The point is that the BRST-like operators for these algebras are equivalent modulo trivial operators with respect to the BRST operator GBRST for the constraint J-(z)=l. We are then naturally lead to consider the SL(2) Wess-Zumino-Witten (WZW)
335
Hidden SUn) Symmetry in Conformal Field Theories
51
model with one of its right-moving currents, J (z\ being gauged as
The physical Hilbert space of its right-moving sector gives irreducible represent ations of the Virasoro algebra. Thus there is a SL(2) symmetry in the Virasoro representations, but it is gauged and is not observable. This system is also equivalent to quantum field theory of the coadjoint orbit of the Virasoro group. The geometric quantization of the Virasoro group was previously discussed by Witten [14]. Based on this result, we present a canonical derivation of the SL(2) current algebra in the induced gravity; it is a manifestation of the hidden SL(2) symmetry in conformal field theory. In understanding various aspects of conformal field theories, it has proved fruitful to explore the interplay between the Virasoro algebra and the complex geometry of Riemann surfaces. Is there also some geometrical structure behind the Wn-algebra? To answer this question, we must understand what kind of symmetry the Wn-algebra implies. The Virasoro algebra is the consequence of reparametrization and Weyl scaling invariance of a field theory, and the structure of these symmetries is encoded into the geometric action of the Virasoro algebra. Thus the first step to appreciate the geometric aspect of the H^-algebra would be to construct a geometric action for this algebra. The W„ -algebra is not a Lie algebra, but an algebra with quadratic relations. Usually a geometric action is defined for a Lie group, and one might suspect that there should be no such action for the W„-algebra. Still the quantum Hamiltonian reduction makes it possible to define a natural generalization of the geometric action for the W^-algebra. The paper is organized as follows. In Sect. 2, we study an effective theory of gaugefieldscoupled to the WZW model. This gives a prototype of our construction of induced gravity in later sections. Section 3 is devoted to proving the quantum Hamiltonian reduction. In this section, wefirstrecapitulate the classical Hamiltonian reduction following the result of Drinfeld and Sokolov [6]. A reader may wish to skip this part in the first reading. We then prove the quantum Hamiltonian reduction in the case of SL(2,&1) exploiting the free boson realizations of the Virasoro and the current algebras. We also discuss the quantum Hamiltonian reduction of the SL(n,0t) current algebra and its relation to the W„-algebra. In Sect. 4, we consider the constrained WZW model. Due to the quantum Hamiltonian reduction, this system gives irreducible representations of the Virasoro algebra. At the classical level, the constrained WZW model is equivalent to the field theory of the coadjoint orbits of the Virasoro group. We then discuss the quantization of the Virasoro group. These results are applied to the induced gravity in Sect. 5. It turns out that the quantum gravity is equivalent to the quantum field theory of the coadjoint orbits of the Virasoro group, which, in turn, is related to the constrained SL(2,31) WZW model. In the last section, we consider a generalized geometric action for the W^-algebra, and discuss its symmetries. Notation and Conventions. In this paper, we employ the Lorentzian signature
336
52
M. Bershadsky and H. Ooguri
metric in two-dimensions. To avoid complication in notation, we denote light-cone coordinates by z = t + x and z = t — x, where x and t are space and time coordinates respectively. The z-dependent sector is often called the right-mover and the z-dependent sector is the left-mover. Throughout this paper, SL(ri) is meant to be SL(n,U). 2, Gauge Field Coupled to Wess-Zumino-Witten Model In this section, we describe an effective theory of gauge fields coupled to the WZW model following Polyakov [15]. The cocycle condition of WZW action plays a central role in understanding the dynamics of the effective theory. This is a prototype of our construction of induced gravity in later sections. The effective action r(A) for the gauge field A coupled to the WZW model is given by exp(«r(/f)) = / e x p ( + i J ^ ; f V ' ) \ \
°n
\
/ I WZW model
= llg-1dglexp(ikSvzw(g)
+ iSd^A'>J^
(1)
Ja=~tr(t°dgg-1), where f* is a generator of the gauge group. Since r(A) is also a generating functional for correlation functions of the currents J", the operator product expansion f** J°(Z)J"(W) ~ 1— z—w
kll J<(W)+-r—i^, (z — w)
when applied to Eq. (1), implies the following functional differential equation for r(A): {8«d
+ f^A»(z,z))^-= -^dA'(z,z). (2) oA(z,z) an Let us now quantize the gauge field A with this action r(A). The correlation function is given by = jldAtf"^)-
■Aa"(zn)ei™.
(3)
From the functional differential Eq. (2) for r(A), one can derive the following identity, A'(Z) n A"<(WJ))=y I^L/A'M J
I
Tz — w, \
k + 2c, 2
n Ab)(»j) j*t
■$(£?(&**'»)■
(4)
after changing normalization of the gauge field, A-*(k + 2cv)A. Here cv is the dual
337
Hidden SL(n) Symmetry in Conformal Field Theories
53
Coxeter number of the gauge group. Thus the correlation function of gauge fields make the current algebra of level k = - (k + 2cv). Deriving Eq. (4), we performed integration by parts in the functional integral (3). There we used the anomalous transformation property of the functional integral measure {P
(5)
07t
This is where the shift — k -* — (k + 2cv) of the level comes from. We can also compute the effective action r(A) of the gauge fields directly. Using the cocycle condition of the WZW action [16,17], Sv„(Ug) = Swzw(0) + Sm„(U) -\i±\x(U-1
dU)(Sgg " l ),
(6)
the right-hand side of Eq. (1) can be rewritten as exp (ir(A~)) = exp ( -
(7)
l
where U is related to A as A = U~ dU. Since the measure [g~ dg~\ is invariant under the left action of the gauge group g-> U~ lg, the result of the o-integration is independent of U. Thus we obtain r(A) = - kSwzw(U), A = U~1W.
(8)
It is easy to check that r(A) in the above solves the functional differential Eq. (2). In fact Eq. (2) is the infinitesimal version of the cocycle condition of the WZW action. Now we can compute the correlation function (3) of the gauge fields as <*'(*,)•■• A""(zn)> = J [«M] A«(zx)■ ■ ■ A°"{zn)exp(- ikSWIV(U)) = J [1/ " l d lTM"(fi) • • • A-(zu) exp ( - i(k + 2cv)Swzv(U)). (9) The shift of the factor — k -»• — (k + 2cv) in front of the WZW action is due to the Jacobian under the change of variable A-*U. [
(10)
From the above Eq. (9), it is clear that the correlation functions of the gauge fields make the current algebra of level k = — (k + 2cv). It is also possible to consider the gaugefieldin the presence of several primary fields
a
A
(11)
where
-%„*,).
(12)
As in the case of the effective action, we can derive the functional differential
338
M. Bcrshadsky and H. Ooguri
54
equation for SH as b& (S°*d + f<*(z,z))J1-— dA(z,z)
i ( k = —( --dA'(z,z)+ 87C\ 2
" X Wz-wJ (=i
\ \S. J
(13)
From this equation, it is easy to show that the correlation function of the gauge fields
(14)
behaves as <^Hz^)---^(zJ>wl...Wn~^:^<^2(z2)---^(zJ>Wl...w„, Zl W
~ J
(15)
With slight abuse of notation, one may express the above as Aa(z) 0(w, w) ~ -
-f
z—w
4>(w, w).
(16)
It is clear that the highest weight state of the right-moving current algebra of level k corresponds to the lowest weight state 1 of the induced left-moving current algebra of level — (k + 2cv). 3. SL(n) Symmetry Hidden in W,-Algebra In this and the next section, we develop tools to study an effective theory of gravity coupled to conformal field theory. In this section, we point out that there is an SL(n) symmetry hidden in the WH-algebra. The relation between classical versions of the WH and the SL{n) current algebras has been known in the context of the Korteweg-de Vries type equations. Consider a dual space of the SL(n) loop algebra. This space has a natural Poisson bracket, and can be regarded as a classical phase space. This phase space has a certain symmetry, and one may reduce it with respect to this symmetry. The Poisson bracket of the reduced phase space turns out to be the classical version of the W^-algebra. We review this classical Hamiltonian reduction briefly following the paper by Drinfeld and Sokolov [6]. The rest of this paper is understandable without knowing the classical Hamiltonian reduction, and the reader may wish to skip this part for the first reading. We then develop the quantum analogue of this Hamiltonian reduction. 3.1 Classical Hamiltonian Reduction. For the purpose of illustration, let us start with the finite dimensional situation. Let M be a finite dimensional phase space. This means that M is implemented with a non-degenerate symplectic form co, which defines a Poisson bracket {,}PB. Suppose that a group G acts on M while preserving the symplectic form <w. The group G is then the symmetry of the phase space M. Now we are going to define the reduced phase space with respect to this symmetry.
1
By the lowest weight state, we mean the one with respect to the zero mode of the current algebra
339
Hidden SL(n) Symmetry in Conformal Field Theories
55
Each element e of #, the Lie algebra of the symmetry group G, defines a vector field ve on the phase space. Assume that for each ee'S there is a function He(x) on Af such that veF(x) = {He{x),F(x)}PB for any function F(x) on Af.
(17)
In this case the symmetry is called Hamiltonian. Associated with this Hamiltonian structure of the symmetry G, there is a canonical momentum mapping P from the phase space Af into the dual of the Lie algebra $* defined as xeM->P(x)e9*:
(18) l
For some e*e#* consider a level set of the momentum P~ (e*) = Mg. <= Af, and let Gg. be a stationary subgroup of G mapping Af,. into itself. One may then consider the quotient space Af^/G,., which has a natural symplectic structure (for a proof see for example Appendix 5 of a book by Arnold [18]). This defines the reduced phase space. Now we are going to apply this construction to the case when Af is a dual space of SL(n)k, the level-fc central extension of SL(n)-loop algebra. In this case, the symmetry algebra & will be a subalgebra of SLin^ given below. To be more explicit, an element of SL{n)k is a pair (A(z),a0) where A(z) is the mapping from circle into SL(n) and a0 is a constant number. The commutator of this algebra is given by l(A{z\ a0), (B(z), M ] = (UOO, B{z)l
k$ tr (A(z)dzB(z))dz).
(19)
The dual space of SL(n)k is defined with respect to the following pairing: <x,a> = §ti(J(z)A(z))dz+ x0a0 x = (J{z), x0)e(SL(n)kr, a = (A(z), a0)eSl+n)k.
(20)
The Poisson bracket of the phase space Af = (SL(n)k)* is defined as {Ja(z), Jb(w) }PB = /«* J'(w)S(z - w) + ^ 5«>5'(z - w), {xo,Ja(z)}PB = 0, {xo,yo}pB = 0,
(21)
where J«(z) = tr(fV(z)). We consider a subalgebra IS of SUji)k consisting of pairs e = {E(z),e0) with E(x) in the Borel subalgebra of SL(ri) (subalgebra generated by strictly upper triangular matrices). The action of # on Af = (SL(n)k)* is coadjointly defined as xeAf-»Ad*(x)eAf
(ee<$),
(22)
where
(23)
and Ade is the adjoint action of ee<8 on SL{n)k. Now that we have the phase space Af = (SL(n)k)* with the symmetry # =
340
56
M. Bershadsky and H. Oogun
(subalgebra of SL(n)k), we can define a reduced phase space with respect to this symmetry. We are going to show that the Poisson bracket in the reduced phase space gives the classical W.-algebra. The dual space <8* is isomorphic to the quotient (SL(n)t)*/(l/(x),0) where U{x) belongs to the Borel subgroup of SL(n). As a representative of a point in #*, one may take e* = {E*(z), l)e(SL(n)k)*, where E*{z) is in the form ^ • . 1 0 . * 1
0
••• 0^ 0 - 0 1
(24)
0
1
v* *
* *J
For such choice of e*, the level set Mg, of the momentum mapping P consists of (J{z), 1) where J(z) is also of the form (24). This condition is expressed in terms of the currents J~"(z) as simple root, fl, if a is simp JO otherwise,
(25)
for any positive root a. The stationary subgroup G«. of M^ consists of pairs (U(z), 1), where U(z) belongs to the Borel subgroup of SL(n). It acts on M„. by a coadjoint action. To be explicit, U-l--dtUU'K
Ad J(J(z)) = UJ{z)
(26)
In order to describe the Poisson bracket on reduced phase space let us consider some specific coordinate system on M^/G^. Exploiting the gauge symmetry (26) one can always put J(z) into the form (*i
J(z) =
0 0
1
0
1 «^3
0 0
0\ 0 1
0
lo
0
•••
0 0
n-l
0
6
(27)
1
where J ] ^ = 0. It is convenient to introduce the fields
(29)
341
Hidden SL(n) Symmetry in Confonnal Field Theories
57
where Ktj is Cartan matrix of SL(ri). They are the Poisson brackets of the free scalar fields. What happens if one chooses another choice of gauge slice? For example, instead of Eq. (24), one may also reduce J(z) to the following form:
J(z) =
0 0 0 0 «»
1 0 0 0 "»-l
•••
0\ 0
i
6
0
0
1
"„-2
«2
0 )
0 1 0
0 0
(30)
In order to clarify the relation between these two sets of coordinates, let us consider the differential equation ((k/2)dz — J(z))~v(z) = 0, where "P(z) is a n-dimensional vector. Due to the following form of this equation /
* 1 0 1
0 0
( »i(z)
0 = 0,
0
* * * *
X
1
(31)
Vn-lU)
one can eliminate all the components of the vector U(z) but v^z) and obtain an nlh order differential equation SC\J]vl(z) = 0 for t>,(z). It is easy to show that the differential operator <£ [J] is invariant under the gauge transformation (26). Thus by computing SC[J~\ in two cases, (27) and (30), and identifying them, we get the relation in a compact form as
n(^.-^))=-z«»-^)(^,y, «o=-i, ",=o.
(32)
This relation is known as the Miura transformation in the theory of the Korteweg-de Vries type equations. Using this relation we can rewrite the Poisson bracket (29) in terms of Uj. The fields Uj make an associative algebra with quadratic relations known as the Gelfand-Dickey algebra, {u,(z)«j(w)}„ = C^z - w) + F*j(z - w)uk + D$(z - w)ukut.
(33)
For the case of SL{2) the algebra (33) reduces to the standard Lie algebra {K(Z)U(W)}PB = (du(w)
+ 2u(w)d + k2d3)S(z - w),
(34)
and this is the classical version of the Virasoro algebra. The case of SL(3) gives us the first non-trivial example of an algebra with a quadratic relation which is the classical version of W3-algebra discovered by Zamolodchikov [4]. In general algebras (33) correspond to W„-algebras of spin n. For more details we refer the reader to the original papers [6,7,19].
342
M. Bershadsky and H. Ooguri
58
3.2 Quantum Hamiltonian Reduction; Case ofSL{2). Now we are going to develop the quantum analogue of the Hamiltonian reduction. To motivate our construction, let us start with some numerology in the case of SL(2) current algebra. For the level-k SL(2) current algebra, J + (z)J'(W)
2
—P(yV) +
Z —W
-
^
(Z — Wf
+1 j3(2)./±(w)~^J»,
fe/2 j3iz)J*{w)„^—^t
(35)
z— w (z — w) there is a canonical definition of an energy-momentum tensor (the Sugawara construction):
W>(*> = j^jT.-J'Wizl.
(36)
With respect to this energy-momentum tensor, the currents J±,J3 behave as conformal fields of weight 1. In order to put the constraint J~{z) = 1 consistently with the conformal invariance, this property of TSLW is not convenient, and we wish to deform the energy-momentum tensor so that the confonnal weight of J~ vanishes [7,20], TiatnnA(z) = TSLm{z) - dJHz).
(37)
The central charge for this improved energy-momentum tensor is 15 — ck(2, = r.—^ T ^ -— 6 KOK==15^--6(fc + 2). (38) 7 r T-—„ k+2 k+2 On the other hand, a conformal anomaly for a degenerate representation of the Virasoro algebra is given by the formula cvir=l-6^—«L=i3 -6p/q. pq p/q Substituting p/q = k + 2 in Eq. (39), we obtain the relation
(39)
4 2 = 1 3 - ^ - 6 ( K + 2) = 4 * 2 , 2 , - 2 .
(40)
We note that the difference of 4*2(2) and c $ is independent of k. In fact — 2 is equal to the conformal anomaly of a ghost system (b(z), c(z)) of weights (0,1). Ghosts of such weights naturally emerge if we put the constraint J"(z)= 1 using the Becchi-Rouet-Stora-Tyutin (BRST) formalism. This observation leads us to the following conjecture. Consider an irreducible representation space of the level-K SL(2) current algebra Jf fl{2) and the Fock space of the ghost system 3tfhjC. The BRST operator defined by Gwr = $^(.r(*)-l)c(z) is nilpotent
QBRST =
0» an£ l o n e
ma
y consider the cohomology
(41) HQBKST
with respect
343
Hidden SUn) Symmetry in Conformal Field Theories
59
to the BRST charge, w
QBKSTO^SLU, ® -*V)
= Ker (QBRST)flm (QBRST).
(42)
The claim is that this cohomology is isomorphic to an irreducible representation space MCi*> of the Virasoro algebra with c = c£/(2) — 2,2
#<wC*W>®-*V)--*1B-
<43)
The rest of this subsection is devoted to proving this theorem. In the classical Hamiltonian reduction discussed in the previous section, we considered a subspace of the total phase space restricted by J'(z) = 1. The reduced phase space was then defined as a space of orbits in this subspace generated by J~(z) through Poisson bracket. Here quantum mechanically, the physical subspace is defined by the constraint QBRSTI V> = 0 in the total Hilbert space, and the reduced Hilbert space is the space of orbits of the BRST charge. As a matter of fact, the total energy-momentum tensor T°»\z) = Timproyed(z) + 8b(z)c(z)
(44)
acting on Jflskll2) ® $fb,c commutes with the BRST charge since the BRST current (J~(z) — l)c(z) is a field of weight 1 with respect to 7nou,(z). It is also easy to convince oneself that this total energy-momentum tensor is not a BRST exact operator, T"""1^) # {QBRST. *}• One can, for example, examine the grade-2 physical subspace in the descendants of the vacuum state |0> SL(2) ®|0> M . The BRST cohomology of this subspace is one-dimensional and generated by L'f'f1 acting on the vacuum. Therefore it is clear that the Virasoro algebra with c = c£2(2) — 2 acts on the reduced Hilbert space HQBRST{JfSL(2) ® Jtfb,c). The issue is whether the representation is irreducible. To prove the irreducibility of the reduced Hilbert space, it is useful to employ the realization of the SL(2) current algebra in terms of a scalar field
(45)
as J + (z)= - /?(z)(v(z))2 + ia+y(z)d
We are informed by A. A. Beilinson and T. Eguchi that a similar construction was suggested by B. L. Feigin
344
60
M. Bershadsky and H. Oogun
In this realization, the ghosts (b, c) and (/?, y) make a pair of BRST doublets, which is called the Kugo-Ojima quartet [11]. We are going to prove the following lemma. Lemma (Quartet Confinement). # QBRST(-*% ® -*V, ® * V )
* *
9
-
(47)
This lemma means that the ghosts simply decouple from the physical subspace. The proof of this lemma goes as follows. Consider the following projection operator &, ^:jr,®jr / t , y <8)jf 6 , c ^^(8)|0> / , > y ®|0> t , c .
(48)
Here the vacua |0>#>y and |0>ti<. are defined by ft,|0>,,y = Q, &„|0\ c = 0 (n = 0) yJ0>,,, = a, cJ0>fc,c = 0 (ro£l).
(49)
The zero modes of the bosonic ghosts, /?0 and y0 obey the commutation relation [/Wo] = l. If y0 is diagonalized, fj0 can be regarded as a differential operator,
(50)
/*o= A Sy0 Though the projection operator 9 does not commute with it as pv» = ei°0e-i° = eyop
(51) 6BRST»
we
can modify (52)
0
so that i* * commute with CBRSTNow we show that 1 — f*0' is BRST exact. Following the paper by Kugo and Ojima [11], we introduce a set of operators P^N) (N = 1,2,3,...) defined inductively as j " »g i
+i
I (c-n^-^K
+ y_„i*w- l)(Pn ~ **>))•
(53)
These operators P1™ commute with CBRST. In fact, for N — l,/*"' is a BRST exact operator,
+ h I (?-^" , ) ^ + r-^",)^)N .20
(54)
345
Hidden SL(n) Symmetry in Conformal Field Theories
61
It is easy to see that they are complete, 1 ^ = 1 .
(55)
Therefore any physical state | ¥*> annihilated by QBRST is written as (56) This means that the physical state | V> is equivalent to its projection onto ^
(5?)
2
i.e. upto a BRST exact operator, T oUl is equal to TFF(z), which is in the same form as that in the free boson realization of the Virasoro algebra developed by Dotsenko and Fateev [8] (also called the Feigin-Fuchs realization). Thus one may suspect that there is a close connection between these free boson realizations of the Virasoro and the SL(2) current algebras.3 Let us recall the free boson realization of the Virasoro algebra by Dotsenko and Fateev. They assume that the scalarfield
■?P£s:subspace with charge (1 — r)<x+ + (1 — s)a_ I a_ =
1.
In this realization, primary fields interwine subspaces of different 1/(1) charges, and their correlation functions vanish in general due to the conservation of the 1/(1) charge. To get meaningful results, we must introduce charge screening operators iKi(z), *£(*) = «***'• Since their operator product expansion with TFF(z) is total derivative, rFF(zW¥1r(w)~dJ^0±(w)\
(59)
(60)
3 D. Bernard and G. Felder have examined degenerate representations of the SU2) current algebra using the free boson realization (46). They also found the intriguing relation between the representations of the Virasoro and the SL(2) current algebra, which is potentially related to our observations here. We thank them for informing as of their result before publication
(58)
346
M. Bershadsky and H. Oogun
62
we can insert their contour integrals in correlation functions to satisfy the total charge conservation without spoiling the Ward identities. The realization of the Virasoro algebra in Jtf^^ is highly reducible. It was pointed out by Felder [12] that one can extract an irreducible representation out of Jf J;1 by using the charge screening operators. Following Thorn [21], he introduced an operator QyiT defined by contour integrals of the screening operators. It is nilpotent Qlir = 0, and generates the following spectral sequence:
He then proved that this spectral sequence is exact, Ker (Qvir) = Im (Qvir), except at the middle Fock space JVl£3) with l^rgp-1,
l^s^tf-1,
qs<pr.
(62)
The cohomology at the middle Fock space is isomorphic to an irreducible representation space of the Virasoro algebra Jt1'^ with a highest weight Ar, = i((a + r + a_s) 2 -(a + +a_) 2 ), *W*HQ„Jjr™).
(63)
For the SIJ2) current algebra, there are also two screening operators*
(64)
which satisfy
■/WWW) * aJjz^ °± ("))•
< 65 >
Since all the singular terms in the operator product expansions are total derivatives, we can insert contour integrals of these screening operators into correlation functions without spoiling their Ward identities. As in the case of the Virasoro algebra, one can construct a nilpotent operator QSL(2) from the screening operators. In the case of the Virasoro algebra, the spectral sequence (61) is exact except at one point Jf(,,s), where the cohomology HQvlt is isomorphic to an irreducible representation of the Virasoro algebra. The corresponding statement in the case of the SL(2) current algebra, i.e. exactness of the spectral sequence of QSUD except at Jtr^-'^Jf^and Jtf*sL(2) = (irreducible representation of .the current algebra) ^a.Mi.W'®-***). is now being worked out by Bernard and Felder [13].
(66)
* The definition iltsui) ma Y be subtle, for it involves a negative power of /?(z) when k is greater than — 2. In extracting an irreducible representation from jff-*' as described below, however, one needs to use only one of these screening operators, say 4>SUD which is well-defined [13]. (This is also the case for the Virasoro algebra [12].) Thus this subtlety is not relevant to our construction here
347
Hidden SL{n) Symmetry in Conformal Field Theories
63
The screening operators for the Virasoro and the SL(2) current algebra are equivalent to each other modulo BRST exact operators, {QBKT.*(*)efa-*,)} ik + 2)
*SL(2)(Z) =
f l-8(z)' fe.OO = **(*) + JQBRST, *_m
) Hzy^l.
(67)
This implies that the BRST-like operators gvir and QSL(2) are also related as GSLU, =
evi, + {0BRSr.*}-
(68)
In deriving these relations, it is crucial that J~(z) is constrained to be a non-vanishing constant (in our convention J~(z) = 1). If we had chosen QBRST = §(dz/2ni)J~(z)c(z), QSL(2) would have been a BRST exact operator. Now we are ready to prove the main theorem of this subsection (43). The quartet confinement (47) and the result by Felder (63) implies ■ W * HQ,JK-S))
=* «Qv i , 0 «c B R S T « , , I , ®^/..,®^.c)-
(69)
Since QSL(2) commutes with Qat(ST,HQ!IL(2)°HQeKaT is also well-defined. We now show that it is equivalent to the right-hand side in the above. Consider kernels of C,ir and QSL(2) on Ker(gBRST). Thanks to Eq. (68), (2SL(2)| V>eIm(e BRST )~e v J •P>eIm(eBRSr).
(70)
On the other hand, due to the quartet confinement of ghosts, images of Qyit and QSL(2) are equivalent modulo QBRST when considered on Ker(QBRST). Hence we obtain - wQsL(2)° H 0 B R S T « " »
(7i)
The next step is to relate HSL(2)°HQmsT in the above to HQBKST{JfSL(2)). Following the result of Bernard and Felder (66), we may identify M^LID w i t h HQsL(2). Thus what we need to prove is H
Qs,.w
° ^QBRST -
# C B R S T ° HQsi.m
(72)
■
For general nilpotent operators Qj and Q2 which commute with each other, HQl°HQl is not neccessarily valid. To find a sufficient condition for this to be valid, let us consider the following spectral sequence of the double complex generated by Q, and Q2, HQ,°HQ2-
IQ2
Q±v
i-l, m- 1 ' ' « - l.ift- 1
1(22
IQz
Quv r
IQ2
n,m - 1 ' n,m- 1
I
®uv
fi2
r
2u
n+l,«i * n+ l . m - 1
IQi
348
M. Bershadsky and H. Ooguri
64
IQ2
IQ2
* ¥n- l,m+l
* vn,m+ 1
IQ2
\Q2
IQ2 ' r«+l,m+l
IQ2
Here a pair of indices (n,m) of KB(1I denotes a double-grading with respect to Qx and Q2; where Q1 = CBRST and 62 — 6st<2)>" is the ghost number and m is related to the 1/(1) charge. Now we prove the following lemma. Lemma (I) Assume (1) the horizontal sequence is exact except at VH=0m and the vertical sequence is exact except at Vmm=0, and (2) the horizontal sequence isfinite,i.e. for a sufficiently large N, VN+ l m = {0} and V_N_lm = {0} for any m. Then Ker(e 1 e 2 ) = Ker(e 1 )0Ker(e 2 )
(74)
holds on VH>-„ and K_mit with n^0, m>0. (II) Under these assumptions, HQl°HQl(V00) = HQ2°HQ,(V0 0 ). When Qi = GBRST and Q2 = QSLW t n e assumptions of this lemma are satisfied. The assumption (1) is the consequence of the quartet confinement of the ghosts and the result of Bernard and Felder [13]. Concerning the assumption (2), we note that both QBRST SLn^ Qsu2) commute with the total energy-momentum tensor TMM\z) given by Eq. (44). Thus we may restrict VKm's to be in the same eigenspace with respect to LQ0"1. In this case, the ghost numbers of states are bounded below and above, and the horizontal sequence terminates beyond these bounds. The first part of the lemma is proved by mathematical induction. We first show that, if the lemma holds at KB+li_(lB+1)(K_(II+1)im+1), so does VB,-m(F_„,„,). By repeating this procedure finite times, we arrive at an edge of the horizontal sequence, where the lemma can be easily checked explicitly. Since Ker(61Q2)z>Ker(Q1)©Ker(Q2) is obvious, we just need to show Ker(exe 2 ) <= Ker(e 1 )©Ker(e 2 ). ' 'n+l.-m-l
*
i Vn,-m^
K. +li _» —
.
(75)
1 "ll+l,-M+l
Take an arbitrary element v of Ker(Q1g2)lvn -m- Since Q2QiV = 0. Qiv belongs to Ker(Q2)IK,♦!,-„• By the assumption (1), there is some element A of V„+j _ _ ^m + ^ > such that Ql v = Q2k. Such A should satisfy dQ 2 A = 0. According to the assumption of the induction, A belongs to Ker(Qi)©Ker(Q2)> a n ^ i* c a n be written as A = Q 1 v 1 +Q 2 v 2 by the assumption (2). Substituting this into QiV = Q2X, we obtain Q1(v-Q2v1) = 0, i.e. t)-Q2v1eKer(<21) and ueKertQj^Kerfg^.Thus we proved Ker(6,2 2 ) <= Ker(Q1)©Ker(Q2). This is what we wanted to show. By interchanging Qt and Q 2 , we can also prove Ker(Qt Q2) = K e r ( d ) © Ker(Q2) on " — n,m'
349
Hidden SL(n) Symmetry in Conlbrmal Field Theories
65
Let us have a look at the right edge of the horizontal sequence, -^.-«-0.
(76)
It is obvious that KWi_m = Ker(Qi)|Kw _m. Thus we obtain Ker(eiQ2)|JVi_MczKN,_m = Ker(G1)lKN,.m «=Ker(Q1)©Kcr(Q2)|Kw>.iii.
(77)
Thus Ker(6,e 2 ) = Ker(Q,)®Ker(e 2 ) holds at the right edge. At the left edge 0 ^
V-N,m —>
1
(78)
0—>V_N„+l-
1 the assumption of the induction is trivially satisfied for K_ N _ lin+1 =0. This completes the proof of the first part of the lemma. Next we prove the following equality at V0t0: H o» tv \Ker(Q1)nKer(e2) e. e,l o.o; (im^jeim^^ntKer^JnKer^,))-
l
'
Since the right-hand side is symmetric with respect to Ql and Q2, the second part of the lemma follows from this equality. A class [w] in HQl°HQ2 is given by veV0t0 satisfying Gi»eQ2(»Y-i). Q2v = 0,
(80)
and taken modulo fii(Ker(e2)|,,_ti0)©G2(Ko,_,). ^0.-1
I V-i.
►
1 ,0
> '0,0
1
^1.-1
1 ►
^1.0
(81)
1
Let us rewrite the first condition on v; QiV = Q2X for some A in Klf_i. Since A belongs to Ker(6,Q2)lv, _,, it can be written as ^ = 2,6, + Q2e2 thanks to the first part of the lemma. Thus the first condition becomes 6i(t , -Q2 £ i) = 0 for some eleV0i-1. Since the representative v of the class [w] is chosen modulo 62(^0,-1)' exploit this freedom to set Qlv = 0.
(82) we can
(83)
We have shown the following equality „
oH 01
(v QA
,_ Ker(e,)nKer(Q 2 ) ° "Q 1 (Ker(Q 2 )| v . 1 , o )©(e 2 (K 0 ,_ 1 )nKer(e 1 )| Ko , o )" 0)
K)
350
M. Bershadsky and H. Oogun
66 Finally we prove
GiKcr(e 2 )| K . 1 , 0 = e i (K_ 1>0 )nKcr(e 2 )| Ko>0 .
(85)
It is clear that ei(Ker(e2)lK-I..)«=Qi(^-1.o)nKer(G2)lK„..(86) On the other hand, any element of d(K_ t 0)nKer(Q2)\v0.<> IS written as g,s with eeKer(QlQ2)\v_10. Thanks to the first part of the lemma, e belongs to Ker(Q,)©Ker(e 2 ), and Qte is in Q, (Ker(G2)|K_10). Thus Eq. (85) holds. Combining this with Eq. (84) we obtain Eq. (79). This completes the proof of the lemma. This completes the proof of the quantum Hamiltonian reduction. Theorem (Quantum Hamiltonian Reduction). V*ir*HQmsr{VSL(2)®Vb,c).
(87)
We would like to make two comments. The completely degenerate represen tations of the Virasoro algebra are parametrized by a set of two integers (r, s) with l^r^p— 1, l^s^q— 1, and there are corresponding representations of the $L(2) current algebra. According to Bernard and Felder, the SL(2) current algebra has another class of representations, which corresponds to the case of r = 0. In this case, it is not yet checked whether the assumptions of our theorem (87) hold. Most probably, the cohomology of the nilpotent operator Qyit may not give irreducible representations of the Virasoro algebra. This existence of such represen tations for the current algebra does not contradict our proof. We also remark that this construction may not work if one replaces SL{2,dt) by SU(2). First of all, it is not clear whether the constraint J~ — 1 makes sense in SU(2), for J+ =(J~)*. Another important point is that SU(2) is simply connected while SL(2,3i) is not. The level k of the current algebra related to a completely degenerate representation of the Virasoro algebra is in general fractional (k + 2 = p/q), and so is its highest weight. This is possible only for SL(2), 3.3 Quantum Hamiltonian Reduction; Case of SL(n). The above result can be extended to the case of SL(3) current algebra though it requires more elaborate computations. The SL(3) algebra is generated by six charged currents, J * , J 2 , J j , and two neutral currents, H,,// 2 . The basis is chosen in such a way that these currents correspond to SL(3) generators as 0\ +
J2 .
//,
/0 0 ,0
^3+«
(0 0
(88)
Vo In order to put the constraints Jr(z) = ^ ( z ) = l ,
J3"(z) = 0
(89)
351
Hidden SL(n) Symmetry in Conformal Field Theories
67
consistently with the conformal invariance, we deform the Sugawara energymomentum tensor TSL(3) for the SL(3) current algebra as, Timproved(z) = TSLm - d(H,{z) + H2(z)).
(90)
With respect to this improved energy-momentum tensor, J3 has weight — 1 while JJ" and J2 have weight 0. To put the constraints (89) in the BRST formalism, we must introduce three sets of ghosts, (fc^Cj), (b2,c2) and (b3,c3), with weights (0,1),(0,1) and ( - 1,2) respectively. The BRST charge defined by GBRST = i^WTto~
l)c,(*) + (J 2 "(z)- l)c2(z) + J 3 (z)c 3 (z) + cx(z)c2(z)b3{z)] (91)
acts nilpotently on -#1&(3)®-*V2.3.c,.2.:i- The total energy-momentum commuting with e BRST is ToM(z) = Timproved + 36, (z)c, (z) + 3Mz)c 2 (z) + 2ab3(z)c3(z) + b3(z)8c3(z).
(92)
The free boson realization (46) of Wakimoto and Zamolodchikov can be extended to the case of the SL(3) current algebra as follows. Let us employ two scalar fields q>^ and q>2 and three sets of bosonic ghosts, 0?i,yi),(/? 2 ,y 2 ) a ° d (0 3 , V3), with weights (0,1), (0,1) and ( - 1 , 2 ) respectively.
(93)
It is straightforward to check that the following is a realization of the SL(3) current algebra: •/i + 00= - /Mz)(7i(z))2 + 02(z)y3(z) + (fc+ l)0y1(r) + i«' + y,(z)7 i -d?(z), • T O = ^ ( z M y ^ y ^ z ) - y3(z)) - P2(z)y2(z)2 - /?3(z)y2(z)y3(z) + ia!+y2(z)~e2-d7p(z) + kdy2(z), Jt(z) = Pl(z)((yl(z))2y2(z) -
7l (z)y 3 (z))
- P2(z)y2(z)y3(z)
2
- 03(z)(?3(z)) + kdy3(z) - (k + l)3y1(z)72(z) + ia' + y 3 (z)eV^(z) + ia' + (y 3 (z)-y 1 (z)y 2 (z))? 2 -^(z),
(94)
H,(z) = 2p1(z)y,(z) - p2(z)y2(z) + /?3(z)y3(z) - IV+TJ -^(z), H2(z) = - ^(zjy^z) + 202(z)y2(z) + 03(z)y3(z) - ia'+ 72-d7p(z), Jr(z) = ^i(z) + ?2(z)^3(z), •/2(z) = )?2(z), A"(z) = ^ 3 (z), ?(z) = (
352
M. Bershadsky and H. Ooguri
68 energy-momentum tensor (92), we obtain r°"'(z)=7V 3 (z)-{Q BRirr ,t(z)},
t(z) = y,(z)3M*) + y2(z)db2(z) + 2y3(z)db3(z) + dy3(z)b3(z)-yi8(y2(z)b3(z)),
(95)
with TWl{z) = - i((^,(2)) 2 + (d
(96)
The energy-momentum tensor TWi(z) in the above is in the same form as that in the free boson realization of the W3 algebra (chiral algebra generated by the energy-momentum tensor and a spin-3 chiral operator W3{z)) developed by Fateev and Zamolodchikov [22]. The charge screening operators for W3 algebra are given by ^*>(z) = exp(io47.-?(*)) (a =1,2),
(97)
where
The structure of representations of the W3 algebra has been examined by Mizoguchi [23] using these screening operators. For the SL(3) current algebras, there are also four screening operators *&<*{ = (&(*) + yi WftWr* exp(ta ± 7, -?(z)), *&& = (&(*))"* exp(ia± ?2
(98)
«'+ = -(fe + 3), n_ = l.
(99)
with
It is easy to check that the screening operators of the W3 and the SL(3) current algebras coincide modulo BRST exact operators. Although the representation theory of SL(2) current algebra has not yet been worked out, it is plausible that the construction of irreducible representations using the screening operators (98) along the line of refs. (12,13) extends to the case of SL(3). If this is the case, one can employ the argument used for the relation between the Virasoro and the SL(2) current algebra to show that the BRST cohomology in the physical subspace of IS *^*L(3)®^I>I 2,3,c,,2.3 isomorphic to an irreducible representation space of the W3 algebra. We have explored the relation between the Virasoro and the SL(2) algebras and the W3 and the SL(3) current algebras. It is then natural to expect that such relation between the Wn and the SL(n) current algebras persists for an arbitrary value of n. There are some suggestive feature to support this expectation. The central charge for the Sugawara energy-momentum tensor TSL{n) for the level-fc
353
Hidden Sb(n) Symmetry in Conformal Field Theories
69
SL(n) current algebra is (n2 — l)k/(k + n). Let us deform the energy-momentum tensor as TlmprovedOO = TSLW{z)
~ % dH(z)
(100)
(H(z) is an (n — l)-dimensional vector of Cartan generators and ? is a sum of positive roots) so that we can put constraints on the Borel subalgebra of the SL(n) consistently with the conformal invariance. The central charge of this improved energy-momentum tensor is
4k2(„, = «4 - 1 - n(n2 - l / ^ j - + k + n\
(101)
On ther other hand, the conformal anomaly for a completely degenerate represen tation of the W„ algebra discussed by Fateev and Lykyanov is given by cw„ = (n-l)(l-n(n+l)(-^^-\
(102)
Substituting p/q = k + n, we obtain 4»n = 2n3- n- 1 - n ( n 2 - l)(-j~— + k + n)
= -(n 4 -2n 3 + «) + 4 V
(103)
In order to put constraints on the Borel subalgebra using the BRST for malism, we need j'-sets of ghost systems with weights ( — n + j+l,n — j) for j=l,2,...,n— 1. The sum of conformal anomalies for these ghosts is — (n4—2n3 -I- n) and coincides with the difference between c$n and c£/(B). Another piece of evidence for the relation between the Wn and the SL(n) current algebras comes from their highest weights. The conformal weight in a completely degenerate representation of the W„ algebra is given by A
l
/Vf
v-Y
"("2-l)(p-q)2
where a5j (i = 1,2,..., n — 1) are the fundamental weights of SL(n) normalized as 3,-3j = l -^—^(for i g ;).
(105)
This expression for the highest weight can be rewritten as
A = " l ((1 - r,)(fc + n) - (1 - 5{))3,.
(106)
1=1
This is in the same form as the conformal weight of the spin — A primaryfieldof the SLiti) current algebra with respect to the improved energy-momentum tensor
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M. Bershadsky and H. Ooguri
(100). Thus one may suspect that the following relation holds:
W * ) - * dH(z) + " l t ((» - J)foit*)c,M) + ( « - ; - i)fc0(z)acu(z)) = TWn(z) + {eBRST)*}.
(107)
These observations support the validity of the quantum Hamiltonian reduction of the SL(n) current algebras down to the WH algebra for general value of n. 4. Quantization of the Virasoro Group The analysis of the previous section makes it possible to construct a quantum field theory such that its right-movers give irreducible representation spaces of the Wn-algebra. In the case of n = 2, its classical action turns out to be a geometric action for coadjoint orbit of the Virasoro group. We then discuss quantization of this system. 4.1 Constrained Wess-Zumino-Witten Model. We are going to show that the reduced Hilbert space discussed above naturally emerges if we consider the SUn) Wess-Zumino-Witten (WZW) model and couple the gauge field to the SL{ri) current belonging to the Borel subalgebra. For simplicity we discuss the case of SU2), but extension to the case of SL(n) is straightforward. Let us consider the following system Wofo^HM Kzm (g) + j^A
+
(J- - 1),
J(z)=-k-dg-g-\
(108)
where Swzw(g) is the action of the WZW model. The WZW action obeys the cocycle condition. Sm(Ug) = SKXW(g) + Sm(U) - J ^
ti(U~ lSU)(dgg~l).
(109)
If we restrict U to be in the Borel subgroup of SL(2),Swzw(l/) in the above vanishes. Therefore the gauged WZW action SgtUfei(g,A + ) is invariant under the transformation g^Ug, A+^A+ +ti(U-ldU-t+),
(110)
where U belongs to the Borel subgroup, U = exp(et"). In order to do the functional integration over g and A+, we must divide the measure by the volume of this Borel gauge symmetry.
Let us fix this gauge invariance using the BRST formalism. The BRST transforms
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Hidden SL(n) Symmetry in Conformal Field Theories
71
of g and A + are defined by replacing the parameter e of the infinitesimal gauge transformation with the Faddev-Popov ghost field c, <Wr(0) = ct'g,
SBRST(A + ) = - be.
(112)
The ghost and anti-ghost transform as <W(c) = 0,
<Wr(*>) = B,
<Wr(B) = 0.
(113)
Here we introduced the Nakanishi-Lautrup auxiliaryfieldB as the BRST transform of b, which will serve as the Laugrange multiplier to impose the gauge-fixing condition. The BRST gauge fixing is done by adding the BRST exact operator to the gauged WZW action S,,,,^,,. The original gauged WZW action is clearly invariant under the BRST transformation, for the BRST transformation for g and A+ is in the same form as the Borel gauge transformation. On the other hand the nilpotency of the BRST transformation implies that the BRST exact operator itself is also BRST invariant. Choice of the BRST exact operator defines a gauge-fixing condition. Here we choose the following gauge-fixing condition:
Wd(M + ) + w ( j ^ > * + * ) = kSvzw(g) + ^bdc
+ i~A
+
(J--l-B).
(114)
Integration over B imposes the gauge-fixing condition A+ = 0, while integration over A* puts the constraint B = J~ — 1. Thus we obtain the relation
= J [g~ ldg, db, dc] exp(ikSKZW(g) - i^bScX
(115)
with the on-shell BRST transformation <Wr(0) = Ct~9> <5BRST(C) = 0 , SBRST(b) = J ' - l .
(H6)
This is the system we have discussed in Sect. 3 in the Hamiltonian formalism. Thus the maximal chiral algebra in the right-moving sector of the constrained WZW model is reduced to the Virasoro algebra. In the path integral (111), we can also integrate over A+ first. We then obtain ^gauge"vl]me)^J"(z)-1)eXp(tfcS-(g))-
(U7)
Using the composition law (109), it is easy to show that the above path integral still has the Borel gauge invariance. Since the SL(2) group is three-dimensional, the original WZW model has three degrees of freedom. The constrained WZW
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model (117) has only one degree of freedom since two are killed by the constraint J~(z) = 1 and the Borel gauge in variance. 4.2 Geometric Action for the Virasoro Group. We have seen that the physical Hilbert space of the gauged WZW model with the constraint J~(z) = 1 contains irreducible representation spaces of the Virasoro algebra. Recently Alekseev and Shatashvili [24] also examined the constrained WZW model from a different point of view. Let us make a digression to convey their idea. They start with solving the constraint J~(z) = 1. If we parametrize the element g of the SL(2) by the GauB product
the Borel gauge invariance g-*Ug allows us to put the gauge-fixing condition 0=0. In this guage, the constraint takes the form In this guage, the constraint takes the form ^X2dF+l=0. On the other hand the WZW action in this gauge becomes On the other hand the WZW action in this gauge becomes
(119)
kSw„(g) = ±ld*z(X-ldX)(X-lSX). (120) Solving the constraint with respect to X and substituting it into the WZW action, we obtain the effective action for F as k 8F kSyit(F)= - — Sd*z^(dFd3F-2{d2Fn (121) Thus the constraint of the gauged WZW model is solved,
f(g^clm^(^^
(122)
The measure [dF] is derived from the Haar measure \_g~ldg~] by reduction of degrees of freedom. The energy-momentum tensor for the theory Svil{F) can be derived using the Nother procedure as k fd3F T
3fd2F\2\
k ,„ ,
--*(T*-2(7*))--*<**>■
,
t w
(123)
Remarkably the right-hand side is the Schwarzian derivative of F. In the conformal field theory, the Schwarzian derivative usually appears as in inhomogeneous term in a coordinate transformation z -»w(z) of an energy-momentum tensor. T(z) - T(W(z))(w'(z))2 - ^
{w(z),z}.
(124)
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Hidden SL{n) Symmetry in Conformal Field Theories -
73
This situation is reminiscent of the following fact about the WZW model. In the WZW model, the current J is given by
J=-\dgg'\ and this is the inhomogeneous term in a chiral gauge transformation g -> Ug of the current J{z)^UJ(z)U~l -^dU(z)U~l(z).
(125)
In mathematical terms, Eqs. (124) and (125) give the coadjoint orbits of the Virasoro and the Kac-Moody groups. Wiegmann [26] and independently Alekseev, Faddeev and Shatashvili [25] have developed a procedure to define a geometric action for a quantum field theory of coadjoint orbits, which in the case of the Kac-Moody group reproduces the ordinary WZW action. Alekseev and Shatashvili [24] applied this procedure to the Virasoro group and found that the geometrical action is precisely given by (121), i.e. Syir(F) is an analogue of the WZW action for the Virasoro group. Let us have a look at the symmetry of the action Svir(F). The original WZW model has both left- and right-moving chiral symmetries, Swzw(U{z)g(z, z) V(z)) = Swzw(g(z, z)).
(126)
For the constrained WZW model, the left-moving chiral transformation g(z, z) -> g(z, z) V(z) is still a symmetry of the system since it keeps the constraint J~ = 1 invariant. Thus the left-moving sector has the SU2) current algebra. On the other hand, the right-moving chiral transformation g(z, z)-* U(z)g(z, z) either changes the constraint or is absorbed into the Borel gauge symmetry of the system. Therefore the constrained WZW model has no current algebra in the right-moving sector. In fact according to the analysis in Sects. 2 and 3, the maximum chiral algebra for the right-mover is just the Virasoro algebra. The left-moving chiral symmetry of the constrained WZW model is reflected to the invariance of the action Svir(F) under the following transformation: F(z,z)->
a{z)F(z,z) + b(z) fa(z) b(z)\ , U(z = eSL(2). c(z)F(z,z) + d(z) \c{z) d(z)J
(127)
4.3 Functional Integral over the Virasoro Group. We have seen that the system defined by the functional integral J[dF]exp(ifcSyir(F))
(128)
is equivalent to the constrained WZW model. The maximal chiral algebra in the right-moving sector is the Virasoro algebra of ck = 13 — 6/(fc + 2) — 6(k + 2), while the left-mover has the SL(2) current algebra of level-/c. In this subsection, we examine the property of this functional integral in more detail. Let us consider a generating functional for correlation functions of energy-momentum tensors
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M. Bershadsky and H. Oogun
defined by exp (i/*(fc)) = J IdF] exp fi*Srir(F) + x\
(129)
The operator product expansion of the energy-momentum tensors T(z)T(W)^(r^—2 + ->—dw)T(W) + - ^ - i \(z — w) z — w ) (z — w) implies the functional differential equation for the generating functional,
(130)
(d- h(z,z)d - M ( Z , z ) ) ^ - r H ) = ^ - 3 3 A ( z . n (131) oh(z, z) 24rc As in the case of the WZW model discussed in Sect. 2, the geometric action Svir(F) for the Virasoro group satisfies the cocycle condition under a diffeomorphism, Svb(Fl»F2) = Svir(^i) + SyiT(F2) + J ^
{F, °F 2 , F2}5F2a"F2, (132)
F1oF2(z,z) = F1(F2(z,z),z).
After the change of variable, z->w = F2(z,z), z-*w = z, in the integral in the right-hand side, this cocycle condition becomes S*(Fi °F2) = S^CFJ + S¥lr(F2) + J ^ /.^F,-1,
{F^w, w), w} ^ * j
i.e. F2(f2(z,z),z) = z.
(133)
It is worthwhile to note that the cocycle condition (133) can be derived from the cocycle condition of the WZW model (6). Since the Virasoro algebra comes from the SL(2) current algebra by reduction of degrees of freedom, it is natural that the cocycle conditions for these symmetries are related. We will come back to this point in Sect. 6. Let us set h = &f2/df2 in Eq. (129). Then we can exploit the cocycle condition to rewrite the path integral (129) as cxp(iT(*)) = exp( - ikSyit(F2)) J [ d F J exp(fcSTlf (F, °F2)) = cxp(-ikSvir(F2))$[.dFl°f2lexp(ilcSyiAFl)).
(134)
If the measure [dFj] was invariant under diffeomorphism F1-*Fi°f2, we would have gotten r(h) = — kSviT(F2). However this is correct only in the classical limit of k-*ao. In fact, using the cocycle condition (133); it is straightforward to check that the solution to the functional differential Eq. (131) is given by (ct/6)Syir(F2) (note that ck/6 -* — k as k -»oo} Thus an additional factor exp (i(ck/6 + k)Syir(F2)) should come from the change of the functional integration measure [dF\°/2]-» LdF.l The measure [dF] has been derived from the Haar measure [ ldg] of the WZW model by reduction of degrees of freedom. In the next section, we
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Hidden SL(n) Symmetry in Conformal Field Theories
75
will encounter another type of measure [[rff]] = [dF°f~\ (F(f{z,z),z) = z). This measure is defined to be diffeomorphism invariant and should be a natural functional integral measure to quantize the Virasoro group. The above observation suggests that these two measures are related as J [
(135)
One can easily check that the right-hand side in the above functional integral correctly reproduces the value of the conformal anomaly ck. We thus claim that the quantum theory of the Virasoro group with the action — (ck/6)Syir(F) is equivalent to the constrained SU2) WZW model of level k. 5. Two-Dimensional Gravity 5.1 SL(2) Symmetry in Gravity. Now we are ready to study the quantum theory of the induced gravity. Consider the gravity coupled to the left-right symmetric conformal field theory. Because of the general covariance, we may choose the light-cone gauge for the metric, d2s = dzdz + h(z, z)dzdz.
(136)
In this gauge, an effective action of the gravity is given as a generating functional for the energy-momentum tensor for the right-movers. Then it should satisfy the functional differential Eq. (131), and the effective action for the light-cone metric is given by the geometric action for the Virasoro group as r(h) = C-±Syir(F), h(z,z) = dJ£4 F(Az,z),z) = z. (137) 6 Sf(z,z) In the light-cone gauge, the Faddeev-Popov determinant does not depend on h. The quantum gravity is then defined by the following functional integral [2]: Kd*]expfesvir(F)\
(138)
Let us make a change of variable in the above functional integral. To parametrize an infinitesimal variation of the metric h, we may introduce a vector field e(z, z) as u -\ , s.u -\ Sf(z + e(z,z),z) h(z,z) + Sh(z,z)= .
(139)
df{z-»[de] + e(z,z),z) The Jacobian for the change of measure [dh] can be easily computed to be The Jacobian for the change of measure [dh] -»[de] can be easily computed to be [rf/i] = det (5"hd + dh)[_d£-] = exp ( - i^Syir(F))[(ie]. (140) It is also straightforward to see It is also straightforward to see \dt\ = \dFon = UdF\\, (141) where [fjfe]] [fjfe]] is is the the diffeomorphism diffeomorphism invariant invariant measure measure for where for F F discussed discussed in in the the last last
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M. Bershadsky and H. Ooguri
76
section. Thus the functional integral (138) is written J[[dF]]exp(-i^*Svlr(F)\
(142)
In Sect. 2, we have shown that the gauge field coupled to the WZW model of level k also makes the WZW model of level — (k + 2cy). We now found that the induced gravity coupled to the conformal field theory with the conformal anomaly ck gives the quantum field theory of the coadjoint orbit of the Virasoro group with the conformal anomaly c = 26 — ck. In the last section, we have shown that the constrained SL(2) WZW model with level k is equivalent to the quantum theory of the Virasoro group with the action — ck/6Syir(F). Because of the relation 26 — ck = c_(Jk+4), the quantum gravity coupled to the conformal field theory with ck is equivalent to the constrained WZW model of level k = — (k + 4), J [[dF]] exp ( - i^^Sylt(F)\ J
= J [dF] exp ( - i(k + 4)Svir(F))
(gauge volume)
Thus the left-moving sector of the gravity has the SL{2) current algebra of level k. This relation between the level k of the current algebra in the induced gravity and the conformal anomaly ck of the original conformal field theory agrees with the result by Knizhnik, Polyakov and Zamolodchikov [3]. So far we have not looked at constraints implied by the light-cone gauge condition of the metric. Originally Knizhnik, Polyakov and Zamolodchikov derived the relation between k and ck by requiring such constraints be imposed consistently. Since the notion of constraints in the induced gravity sounds delicate, we would like to explain the situation using the example of the WZW model. Consider the WZW model coupled to a gauge field A and A as [16] .d2z / _ . , i U . _. k^ S(g;A,A) = kSmzw(g) + l —tr I AJ-AJ + -AgAg-i--AA\.
(144)
This action has the vector gauge invariance g->ugu-\ A-+UAU'1 + duu~\
A-*uAu~l + duu-1.
( 145 )
By setting the gauge-fixing condition A = 0, we obtain the system discussed in Sect. 2. In the BRST formalism, we introduce a set of_ghosts (b,c) in the adjoint representation of the gauge group. The total current JtoUl(z) is given by •/.el = J-^(g-iAg-A) + J^,. ^<
(146)
By making a change of variables (g-*U lg and similar operators on b and c, where A = U~1W), an effective action for the gauge field is extracted, as we have
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Hidden SL(n) Symmetry in Conformal Field Theories
77
seen in Sect. 2. After this [/-dependent chiral gauge transformation, the total current Jtoiai becomes the sum of three currents, J,((k + 2cv)/2)U~ldU and Jtho,t. Since anomalies of these currents are k, — (k + 2cv) and 2cv respectively, the total current is anomaly free. The BRST charge for the vector gauge invariance is then nilpotent. The situation should be the same in the case of the induced gravity, and the total conformal anomaly in the left-moving sector should vanish. The original conformal field theory has an anomaly ck, and the ghosts for the light-cone gauge-fixing add - 26 - 2 = — 28. Then the conformal anomaly in the left-moving sector of the gravity must be 28 — ck = 3k/k + 2 — 6k(k= — (k + 4)). This seems to indicate that the left-moving current algebra of the gravity is also constrained, otherwise the conformal anomaly would be 3k/k + 2. Knizhnik, Polyakov and Zamolodchikov argued that one of the constraints associated with the light-cone gauge fixing is J~ (z) = 0 for the left-moving current algebra of the gravity, and that this constraint shifts the conformal anomaly by — 6k. We think that this aspect of the theory is not well-understood yet and requires further investigation. It should be emphasized that, in our approach, the relation between ck and k is derived independently of these considerations on constraints. We would like to note intriguing numerology concerning the levels of current algebras. In Sect. 2, we have seen that the right-moving current algebra of level k induces the left-moving current algebra of level - (k + 2cv) ( - (/c + 4) for SL{2)). Here we found that the conformalfieldtheory with anomaly ck, whose right-mover has a hidden SL(2) current algebra of level k, induces the left-moving current algebra of level k = - (k + 4) in the gravity. There should be a way to derive the current algebra in the induced gravity directly from the hidden current algebra in the conformal field theory. 5.2 Scaling Dimensions of Planar Random Surface. Let us now discuss how we can compute scaling dimensions of a random surface from the above result. First we would like to remind the reader the definition of scaling dimensions. Consider a partition function for random surfaces with fixed area s/, 4T(J/)=
£
e F
' -
(147>
surfaces
Here the weight r is given by a partition function of some statistical model on the surface. It is expected that the partition function behaves asymptotically as 2'(s/)~s/-3 + 'e-"',
j/-»oo.
(148)
Although K is cutoff dependent, y depends only on the topology of the surface [27,28] and it gives the scaling dimensions of the random surface. In the following we restrict ourselves to the case of planar topology. In this case, the scaling dimensions have been computed for various statistical models on triangulated random surfaces by Kazakov and Migdal [1]. Let us assume that, in the sd-+ao limit, the sum over surfaces in Eq. (147) reduces to a functional integral over an intrinsic metric on the surface, and the weight r is replaced by the effective action T(/i) for the gravity. Then the partition
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M. Bershadsky and H. Ooguri
function is given by sf3^ar(j/)
~ \[dK] <exp( - i \d2zh(z, z)T(z))} = J[df]exp(-i(fc + 4)Syir(F)),
{s/ -> oo)
hJ-f
f(F{z,z),z) = z. of In the light-cone gauge, the area s/ is given by ^ = Jd2z, ( ^ = 1 ) .
(149)
(150)
The value of si is fixed by the range of coordinates (z, z) independently of the dynamical variable h. Thus we can perform the functional integral (149) without any restriction on h. As we noted in Sect. 5, the functional integral (149) has the chiral SL(2) symmetry in the left-moving sector,
aJ^zHbtf y
' '
c(z)F(z,z) + d(z)
K
'
Remember that the relation between F and h is non-local as h = df/df, f{F(z, z), z) = z. With respect to f(z, z), the above transformation becomes \c(z)z + d(z) J The chiral SL(2) transformation of the constrained WZW model turns into a coordinate transformation on the surface. In fact this is the symmetry of the induced action r(h) as well as the measure. Among the SL(2) currents J"(z) in the left-moving sector, P(z) generates the scale transformation z->(l+e(z))z, z-+z.
(153)
Therefore the scaling dimension y is given by the SL{2) spin of the vacuum state of the induced gravity as
Q3 = $P(z)dz.
(154)
In order to compute the scaling dimensions, we need a relation between the conformal weight of the right-moving Virasoro algebra in the original conformal field theory and the SL(2) spin of the left-moving current algebra in the induced gravity. Following previous sections, we regard the right-movers as that of the constrained WZW model. The energy-momentum tensor is then T(z) = ^
T,J'(z)J-(2) - dJ3(z) + db(z)c(z),
(155)
-^c(z)(J-(z)-l)
(156)
and the BRST charge
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Hidden SL(n) Symmetry in Conformal Field Theories
79
is used to define physical states. The physical primary field
The conformal weight A of
(158)
fc + 2
By extending the argument in the last subsection in the presence of primary fields, we can show that the physical field
(159)
Thus right-moving conformal weight A and the left-moving SL{2) spin X are related by Eq. (158). Especially the SL(2) spin of the vacuum state is obtained by putting 4 = 0 in Eq. (158), i.e. either 0 or -{k+ 1). This gives the scaling dimensions of the surface. Since the level k of the SL(2) current algebra is related to the conformal anomaly of the conformal field theory as c» = 13-
k+2
-6(k + 2),
(160)
we obtain the formula
7 = Mck-l±J(ck-l)(ck-2S))
orO.
(161)
This formula agrees with that by Knizhnik, Polyakov and Zamolodchikov [3]. If one chooses the branch (—) in the above, it is also consistent with the analytical and numerical computations of triangulated random surface by Kazakov and Migdal [1]. 6. Geometric Action for Ff,-Algebra In this section, we construct a generalization of a geometric action for the W„-algebra. For simplicity, we discuss the case of n = 3, but a generalization for n > 3 is straightforward. As we have seen in Sects. 3 and 4, irreducible representation spaces of the W3 algebra emerge from the constrained SL{3) WZW model. Following the case of the minimal conformal field theory, we will solve the constraints of the WZW model. The constrained SL(3) WZW model is given by J ^ ^ T i S w r W - I W i ( * ) - W(z))exp(iS w z w ( 3 )). vol(Borel)
(162)
Using the GauB decomposition ( \ 9= V«J>3
0 1
0\ (X 0 0
fi
\0 0
0 0
rv
(\ 0
F3\ 1 0
(163)
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M. Bershadsky and H. Oogun
we may put conditions
(164)
By solving them with respect to X,\i and F2 and substituting them into the WZW action, we obtain the effective theory for F 1 and F 3 . ' (gaugge"voui]me)6(Jr(2)" ^ ^
W
"
1WJ
»(z))eXP(S-to))
= J[iF 1 ,iF,]cxp(ikS irj (F 1 ,F3)).
(165)
Here the effective action SWi for F, and F 3 is given by SwAFM
= ^ J d2z[(A"»3A)(A- > 5i) + (it-l dM/i-l dfi) + ^X~ldXKn~ lfr) + W-~ ^X)(n~ldn)-].
(166)
We have chosen F t and F 3 as dynamical variables of the reduced system, for they do not imply an additional Jacobian factor in the functional integral. We claim that SWi is a natural generalization of a geometric action for the W^-algebra. Especially when F3oc(F1)2, this action reduces to the geometric action for the Virasoro group, SB,3(F1,F3oc(F1)2) = 4Svir(F1).
(167)
As in the case of the SU2) current algebra, the effective action Sw,(FltF3) has the left-moving SL(3) current algebra of level k, while the maximal chiral algebra in the right-moving sector is reduced to the W3 algebra with the conformal anomaly ^ 3 = 5 0 - ^ - 2 4 ( f e + 3).
(168)
The energy-momentum tensor T{z) and the spin-3 generator W3(z) in the right-mover are given by substituting Eq. (164) into T(z)=-^l(X-ldtf
+ {ti-ldn)2
+ (X-idXMji-tdit) + 2d(X~ldX) + d(n-ldfi)l W3(z) oc [(A -1 dX + fi~»dn)(X-»dX)(n~l dfi) -(X-ldX)d{X-ldX-n-ldn)-d2{X-ldX)-].
(169)
Let us have a look at the symmetry of the action SWy After some computations, one can check the following cocycle condition directly. kSWj(Fl °F,F2°F) = kSWi(Flt F3) + 4kSyir(F) + \d2zT(Fu F 3 ; z)%, df F,oF(z,z) = FAF(z,z),S), F(f(zyz),z) = z. (170)
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Hidden SL(n) Symmetry in Conformal Field Theories
81
One can derive this cocycle condition from the cocycle condition of the WZW action (6). Suppose we have fields, U(z, z), g(z, z), both satisfying the constraints (164). In general, the product of U(z,z)g(z,z) does not satisfy these constraints. However, when U is of the form (k 0 U= 0 0
0 0
\ (171)
we can modify the action of U on g as (k 0 0 ■g{F{z,z),z), (U*g)(z,z) = 0 n 0 (172) 1 VO 0 /T V I so that U»g also obeys the constraints. It is easy to see that Swzv(U»g) = SWs(Fl°F,F3°F), and that the cocycle condition for Swzw implies the cocycle condition for SWi. This relation between the cocycle conditions of Swzw and SWi is quite natural, for the Virasoro algebra in the theory with SW} comes from the SL(3) symmetry in Swzw by way of the quantum Hamiltonian reduction. Unfortunately, we have not succeeded in defining a modified action of U on g, U»g, for a general WZW field U. Such a multiplication rule, if exists, defines the full W3 symmetry realized in terms of F, and F 3 , just as a diffeomorphism is realized by a single function F with a product °. This will also make it possible to derive a generalized cocycle condition for SWi corresponding to the full H^3-symmetry. Since the W3-algebra is not a Lie algebra, it would not be straightforward to find such a modified action U»g. Still, we believe that such a construction is possible. For the Wj-symmetry comes from the SL(3) symmetry of Swzw by the quantum Hamiltonian reduction. Let us make some more speculations about the theory with SW}. In the functional integral (165), the measure [dF!,dF 3 ] is derived from the Haar measure [0_1
(173)
In the case of the SL{2), the geometric action Syir(F) described the induced gravity, which is gauge-equivalent to the Liouville model. Therefore we suspect that the constrained SL(3) WZW model is related to the field theory of the Toda molecule, a natural generalization of the Liouville model. Previously Bilal and Gervais [29] have also pointed out that the Toda field theory realizes the W„-algebra. It should be interesting to re-examine their result from the point of view of the quantum Hamiltonian reduction. Proceeding further, we may consider gaugefieldscoupled to chiral currents in a conformal field theory with the W3-algebra. The induced action for the gauge fields would be — ((100 —ck)/24)SB,3(F1,F3). The induced gauge fields will then
366
M. Bershadsky and H. Ooguri
82
make the SL(3) current algebra of level — (k + 6) in the left-mover. If this is the case, we may compute the scaling dimensions of the surface of the "fluctuating W3-geometry." Conformal weight A and W3-charge w0 of the conformal field theory are given by
/
J
w0 oc ( —
\3/2
J
[9(X + fif{X -n)-(k-
/x)3 + 72(fc + 2)2(2A + n)
+ 9(fc + 2)(3(/l + n)2 + (X - n)2 + 4(A2 - |i 2 ))].
(174)
Here X and \i are lowest weights of the hidden SL(3) current algebra. The scaling dimensions 7 of the surface is given from solutions of A(X, n) = 0, w0(A, /1) = 0 as y = X + li = 0,-(k + 2), - 3(fc + 2), - 4(k + 2),
(175)
- 4(* + 2) = Mc - 2 ± J{c - 2)(c - 98)).
(176)
where
Unfortunately we do not know the classical limit of scaling dimension for "fluctuating W3 geometry" which allows one to choose one of the four solutions. Acknowledgements. We would like to thank J. Cohn and G. Moore for discussions and for reading our manuscript. We are grateful to A. Beilinson, D. Bernard, T. Eguchi, G. Felder, D. Gross, A. Migdal, N. Seiberg, E. and H. Veriinde, and E. Witten for useful comments. M.B. is indebted to L. Dickey and T. Khovanova for drawing his interest into the Hamiltonian reduction. H.O. thanks H. Matsumoto, M. Shishikura and H. Tamanoi for discussions on spectral sequence. The work of M.B. is supported by the Alan T. Waterman Award under grant number PHY-881752188, and that of H.O. by the U.S. Department of Energy under grant number DE-AC-02-76ER02220.
References 1. Kazakov, V., Migdal, A.: Recent progress in the theory of noncritical strings. Niels Bohr Institute preprint NBI-HE-88-28, 1988, and referenced therein 2. Polyakov, A.: Quantum gravity in two dimensions. Mod. Phys. Lett. A2, 893-898 (1987) 3. Knizhnik, V., Polyakov, A., Zamolodchikov, A.: Fractal structure of 2-D quantum gravity. Mod. Phys. Lett. A3, 819-826 (1988) 4. Zamolodchikov, A.: Infinite additional symmetries in two-dimensional conformal quantum field theories. Theor. Math. Phys. 63, 1205-1213 (1985) 5. Fateev, V., Lykanov, S.: The models of two-dimensional conformal quantum field theory with Z.-symmetry. Int. J. Mod. Phys. A3, 507-520 (1988) 6. Drinfeld, V., Sokolov, V.: Lie Algebras and Equations of Korteweg-de Vries Type. J. Sov. Math. 30, 1975-2036 (1984) 7. Belavin, A.: On the connection between Zamolodchikov's W-algebras and Kac-Moody algebras. In: Kawamoto, N., Kugo, T. (eds.). Quantum String Theory, Proc. of the Second Yukawa Memorial Symposium, Nishinomiya, Japan 1987, Proceedings in Physics vol. 31, pp. 132-137. Berlin, Heidelberg, New York: Springer 1989; KdV-type equations and IV-Algebras, handwritten manu script, 1988
367
Hidden SL(n) Symmetry in Conformal Field Theories
83
8. Dotsenko, VI, Fateev, V.: Conformal Algebra and Multipoint Correlation Functions in 2D Statistical Models. Nucl. Phys. B240, [FS 12], 312-348 (1984) 9. Wakimoto, M.: Fock Representation of the Affine Lie Algebra A\". Commun. Math. Phys. 104, 605-609(1986) 10. Zamolodchikov, A.: Talk given at Montreal, 1988 11. Kugo, T., Ojima, I.: Manifestly covariant canonical formalism of the Yang-Mills fields theories I. Prog. Theor. Phys. 60, 1869 (1978) 12 Felder, G.: BRST Approach to Minimal Models. Zurich preprint 88-0618, 1988 13. Bernard, D., Felder, G.: Fock representations and BRST cohomology in SL(2) current algebra. Zurich preprint ETH-TH/89-26 14. Witten, E.: Coadjoint orbit of the Virasoro group. Commun. Math. Phys. 114, 1-53 (1988) 15. Polyakov, A.: Lectures given at Les Houches Summer School, Session XLIX, 1988 16. Polyakov, A., Wiegmann, P.: Goldstone fields in two dimensions with multivalued action. Phys. Lett. 141B, 233-228 (1984) 17. Witten, E.: Nonabelian Bosonization in two dimensions. Commun. Math. Phys. 92,455-472 (1984) 18. Arnold, V.: Mathematical methods of classical mechanics, Graduate Texts in Mathematicas vol. 60. Berlin, Heidelberg, New York: Springer 1980 19. Gervais, J.-L., Neveu, A.: Dual String Spectrum in Polyakov's Quantization (II). Mode Expansions. Nucl. Phys. B209, 125-145 (1982) 20. Deformations of the Sugawara energy-momentum tensor were also discussed in, Fredericks, J., Halpern, M.: Conformal deformation by the currents of affine V, Ann. Phys. 188, 258-306 (1988); Sakai, N., Suranyi, P.: Modification of Virasoro Generators by Kac-Moody Generators, Imperial College preprint TP/87-88/36, 1988 21. Thorn, C: Computing the Kac determinant using dual model techniques and more about the No-Ghost theorem. Nucl. Phys. B248, 551 (1984) 22. Fateev, V., Zamolodchikov, A.: Conformal quantum field theory models in two dimensions having Z 3 Symmetry Nucl. Phys. B280, [FS18], 644-660 (1987) 23. Mizoguchi, S.: The Structure of Representations of the W3 Algebra. University of Tokyo preprint, UT-538, 1988 24. Alekseev, A., Shatashivili, S.: Path integral quantization of the coadjoint orbits of the Virasoro group and 2-D gravity. Leningrad preprint LOMI, 1988 25. Alekseev, A.. Faddeev, L., Shatashivili, S.: Quantization of the symplectic orbits of the compact Lie groups by means of the functional integral. Leningrad preprint LOMI, 1988 26. Wiegmann, P.: Multivalued functionals and geometrical approach to quantization of relativistic particles and strings. MIT preprint, 1988 27. Eguchi, T., Kawai, H.: Number of random surfaces on the Lattice and Large-TV gauge theory. Phys. Lett. HOB, 143-147 (1982) 28. Zamolodchikov, A.: On the entropy of random surfaces. Phys. Lett. 117B, 87-90 (1982) 29. Bilal, A., Gervais, J.-L.: Systematic approach to conformal systems with extended Virasoro symmetries. Phys. Lett. 206B, 412-420 (1988)
Communicated by A. Jaffe Received February 21, 1989
368
Reprinted with permission from Nuclear Physics B Vol. 343, pp. 450-466,1990 © 1990 Hsevier Science Publishers B. V. (North-Holland)
ON THE HOMOLOGICAL CONSTRUCTION OF CASIMIR ALGEBRAS Jose M. FIGUEROA-O'FARRILL* Inslituut voor Theoretische Fysica, Universiteit Leuven, Celestijnenlaan 200 D, B-3030 Leuven, Belgium Received 11 April 1990
We propose a BRST (homological) construction of the Casimir extended con formal algebras by quantizing a classical observation of Drinfeld and Sokolov. We give the explicit expression for the Virasoro generators and compute the discrete series of the Casimir algebras. The unitary subseries agrees with that of the coset construction for the case of simply laced algebras. With the help of a free-field realization of the affine algebra, we compute the BRST cohomology of this system with coefficients in a Fock module. This allows us to generalize and prove a conjecture of Bershadsky and Ooguri.
1. Introduction Extended conformal algebras are associative operator product algebras which contain the Virasoro algebra as a subalgebra and are finitely generated by, in addition to the Virasoro generator, holomorphic Virasoro primaries in such a way that the following closure property is satisfied: In the singular part of the operator product expansion (OPE) of these field there appear only Virasoro descendents of the identity and of these primary fields themselves as well as normal-ordered products thereof. Clearly, if we dropped the requirement of these algebras being finitely generated we could always satisfy the closure property by augmenting the number of generators by whichever new primaries appear in the right-hand side of the OPE, but then we would be dealing with objects far too general to offer any hopes of classification. The study of extended conformal algebras is interesting because they are the only hope of classifying rational conformal field theories with c > 1, this being the central problem in conformal field theory. The systematic study of extended conformal algebras was initiated by Zamolodchikov in ref. [1], where he analyzed the possible associative operator algebras generated by a stress tensor (generating a Virasoro subalgebra) and one or more holomorphic primary fields of half-integral conformal weight s < 3 with the above closure property. He found a lot of already existing conformal field theories: free fermions (s = \), affine Lie algebras (s = 1), superVirasoro algebras (s = §), direct * e-mail: [email protected]
369
J.M. Figueroa-O'Farrill / Casimir algebras
451
product of Virasoro algebras (s = 2); as well as two new algebras (s = § and s = 3) which, unlike the others, are not Lie (super)algebras. The case s = § satisfies the associativity condition for a specific value of the central charge (c = - jf); whereas the case 5 = 3 yields an associative operator algebra - called W3 - for all values of the central charge. This extended algebra has been the focus of a lot of recent work and, in particular, it has been shown to be the symmetry algebra of the 3-state Potts model at criticality [2]. In ref. [3], Bouwknegt continued the approach of Zamolodchikov by investigat ing the possible extensions of the Virasoro algebra by a holomorphic primary field of weight s. He argued that if one demands associativity of the resulting operator algebra for generic values of the Virasoro central charge, the only solutions with integer 5 can occur for 5 = 1,2,3,4,6. Other extended algebras have been con structed following this approach: o ^extended superconformal algebras [4,5], and other algebras with an assortment of fields with low spins [6]. However, this approach suffers from the drawback that one must know in advance the Virasoro primaries that occur in the algebra due to the fact that the closure criterion mentioned above allows for normal-ordered products of primaries to appear among the singular terms in the OPE. Abstractly (as Virasoro primaries), there is no way to test whether the field which appears can in fact be written as normal-ordered products of the "primitive" primaries. In fact, the existence of an extended conformal algebra as defined above can only be probed via its explicit construction in terms an underlying associative conformal field theory like the one corresponding to, say, free fields or affine algebras. One such approach to extended conformal algebras is the construction of the so-called Casimir algebras. Let g be a simple finite-dimensional Lie algebra of rank /. Then the center of the universal enveloping algebra of g is /-dimensional and is spanned by the Casimirs of g. Associated to each Casimir we can define an operator (also referred to as the Casimir with a little abuse of notation) in the universal enveloping algebra of the affinization g of g. This is a generalization of the Sugawara construction which from the quadratic Casimir obtains the Sugawara stress tensor. It turns out that these operators (except for the Sugawara tensor itself) are primary of weight equal to the order of the Casimir with respect to the Virasoro algebra generated by the Sugawara tensor. However, and except for specific values of the central charge, the operator algebra generated by the Casimirs does not close in the sense described above. For example [7], in the case of the affine algebra A^, in the OPE of the cubic Casimir with itself there appears a new primary field which only decouples for c = 2. The way to make a closed operator algebra from the Casimirs relies in a coset construction analogous to that of Goddard-Kent-Olive [8] for A*/'. For example in the case of A'^, the authors of ref. [9] obtained the W3 operator algebra by constructing a weight-three primary operator in the universal enveloping algebra of A(^ x A^ which commutes with the diagonal A(P subalgebra: hence a weight-three primary field in the coset theory
370
452
J.M. Figueroa-O'FarriU / Casimir algebras
( }
(A 2 X A^O/A^. This operator turns out to form a closed operator algebra with the coset Virasoro generator if and only if one of the A(^ factors is at level 1. The weight-three primary is constructed out of the cubic Casimirs of the two factors but also contains mixed terms which are rather mysterious. In fact, the explicit construction of the operators generating the Casimir algebras associated to other affine algebras is still lacking and the very existence of the higher Casimir algebras has not been proven except for A^, although there is certainly some evidence of it coming from character formulas for affine algebras [3]. In fact the conjecture stands that all extended conformal algebras (generated by primaries of integer weights) are indeed Casimir algebras. So far, the only supporting evidence for this claim comes from the results of ref. [3], where it is suggested that the extended conformal algebras obtained by adding just one extra primary field correspond to the Casimir algebras resulting from A, X D,, A, X A,, A 2 , B 2 , and G2 respec tively. The coset construction (or any other construction, for that matter) of these Casimir algebras is known explicitly only for the first three cases. The explicit form of the algebra (as an abstract associative algebra) is nevertheless known in all cases: ref. [10] for the case of spin 4 and ref. [11] for the case of spin 6. However, the identification of these two last algebras as Casimir algebras is still lacking. In this paper we propose a different construction of Casimir algebras than the coset one. This is a generalization of the one in ref. [12], where an explicit construction of W3 from A(p was provided. The method is founded on the result of Drinfeld and Sokolov [13] (after an observation by Reiman and Semenov-TyanShanskii) which showed that a classical version of W3 (as fundamental Poisson brackets of a Poisson manifold) arises from the symplectic reduction of the infinite-dimensional Poisson manifold defined by the dual of the affine algebra A(2} relative to the action of a unipotent subgroup. The role of the Casimirs in this construction has recently been clarified in ref. [14]. The construction of ref. [12] can be thought of as a quantization of the Drinfeld-Sokolov construction for the case of A 2 . There the cubic Casimir of A 2 also played a fundamental role. In fact, the operators which generate the W3 algebra are induced from the BRST comple tions of deformations of the Sugawara stress tensor and of the cubic Casimir by terms of lower order in the A(2} currents. Let us briefly describe the Drinfeld-Sokolov construction for an arbitrary affine algebra g. The dual space M of g has a canonical Poisson structure which is invariant under the action of the corresponding loop group. Let n + denote the nilpotent subalgebra of g generated by the elements associated to the positive roots and ft+ the corresponding affine algebra. The action of the corresponding loop group is Poisson and gives rise to a moment mapping J: M -»h*. Drinfeld and Sokolov consider the level set M0 of / corresponding to the following constraints: t AZ)
"
\0,
otherwise,
*1'1'
371
J.M. Figueroa-O'Farrill / Casimiralgebras
453
where a is a positive root, E_a the generator of g corresponding to the negative root -a, and A is a choice of simple roots. Equivariance of the moment mapping implies that M 0 is stabilized by the loop group corresponding to n + which allows us to quotient by its action and obtain a manifold M which inherits a natural Poisson structure from that on M. In order to write the fundamental Poisson brackets of M explicitly we need to coordinatize M. Since M is defined as a quotient there are no preferred coordinates. In order for M to inherit coordinates from M 0 it is necessary to exhibit it as a submanifold of M 0 , i.e. to fix a gauge. Different choices of a gauge slice will give different coordinates and, hence, different fundamental Poisson brackets. For the case of g = A„, Drinfeld and Sokolov show that there exists a choice of gauge slice in which the fundamental Poisson brackets are those of n free bosons; whereas there exists a different gauge slice in which the fundamental Poisson brackets represent the Gelfand-Dickey algebras which, for A„, is a classical version of W„ + , , the generalization of W3 due to Fateev and Lykyanov [15]. Moreover, the change of coordinates from one gauge slice to another (i.e. the corresponding gauge transformation) is nothing other than the Miura transformation of the KdV theory. This was exploited by Fateev and Lykyanov to construct the Coulomb gas representation for W„. This paper is organized as follows. Sect. 2 contains the general construction. On it we impose the Drinfeld-Sokolov constraints in the BRST formalism. We construct a BRST invariant stress tensor showing that the quantal space of the reduced theory inherits the structure of a Virasoro module and determine its central charge. We do this in detail for all simple Lie algebras. In the simply laced case and for suitable choices of the level, we recover the discrete series of the Casimir algebras. The unitary subseries agrees with the results obtained in the coset construction of ref. [7]. In sect. 3 we analyze the cohomology of the BRST operator in some more detail with the help of a free-field realization for the affine algebra. We compute the BRST cohomology of a Fock module and show that it is (as a Virasoro module) isomorphic to the Fock space of / free bosons with background charge. This allows us to prove for general g a conjecture of Bershadsky and Ooguri [16] for the case A„. The proof of the main theorem in sect. 3 requires a technical result that is discussed in appendix A. Finally, sect. 4 contains some concluding remarks.
2. The general construction Let g be a finite-dimensional simple Lie algebra of rank / and h a Cartan subalgebra which will remain fixed throughout. Let
372
454
J.M. Figueroa-O'Farrill / Casimir algebras
positive roots have higher heights. Associated to each positive root a there are generators £ ± a e g . We now consider the affine algebra g of g. Its Lie bracket is encoded in the operator product expansion (OPE) of the currents X(z) for X e g: X(z)Y(w)
k(X,Y) =-;+ (z-w)
[X,Y](w) +reg,
(2.1)
z—w
where ( , ) is a fixed symmetric invariant bilinear form on g, i.e. a multiple of the Killing form. In particular the currents {Ea(z))ae
Ea(z)Efi(w)
=
^
+reg,
(2.2)
where the coefficients map are defined by [Ea,Ep] = mapEa+p. In the universal enveloping algebra of g we find a Virasoro subalgebra generated by the Sugawara stress tensor:
where gab is the inverse of gab = {Xa,Xb) with {Xa} any basis of g; cg is the eigenvalue of the Casimir element gabXa ®Xb in the adjoint representation; and where by the normal ordered product {AB) of any two operators we mean the following: (AB)(z)=$
, dw — ~C,2TTI
A(w)B(z) \
(2.4)
w —z
The central charge of this representation of the Virasoro algebra is given by 2hd. c(g,k)^—-^, 2k + c%
(2.5)
where dg is the dimension of g. As explained in sect. 1 and following Drinfeld-Sokolov we now impose the following constraints:
These constraints close under commutators since the Lie bracket of two positive
373 J.M. Figueroa-O'Farrill / Casimir algebras
455
roots can never be a simple root. Therefore we can quantize the system a la BRST. To this effect we introduce an antighost-ghost pair (ba,ca) for each positive root a with the following OPE: ba(z)cp(w)
= j f ^ + reg,
(2.7)
and we define the BRST operator d by x
dz
d =
(2.8)
where /BUST "= ~
E c„ + £
(ca£_J + i
£
rnap(cacpba+p).
(2.9)
The closure of the constraint algebra implies that the BRST operator is square-zero: d2 = 0, whence its cohomology is defined. The operators in the reduced theory will be the BRST invariant operators in the algebra generated by the g currents and the (anti)ghost fields; two such operators inducing the same operator in the reduced theory if they are BRST cohomologous, i.e. if their difference can be written as [d, ]. Since we want the reduced theory to be a conformal field theory we want to induce in BRST cohomology the structure of a Virasoro module. In other words, we want to exhibit a BRST invariant field which obeys (at least up to BRST coboundaries) the OPE of the Virasoro algebra. This requires the constraints to be conformally covariant with respect to this Virasoro algebra. For example, under the Virasoro algebra generated by the Sugawara tensor, the currents E_a(z) are all primary of weight one. However the constraints set Ea(z) for a a simple root equal to a constant (1 in our conventions) which has zero conformal weight. Therefore the constraints corresponding to the simple roots are not conformally covariant with respect to the Sugawara stress tensor. In order to obviate this problem we can try to deform the Sugawara stress tensor in such a way that the currents corresponding to the negative simple roots are primary but of zero conformal weight. Let us define a deformed stress tensor Tde{ by adding to it the derivative of a current, r def (2) = r « ( z ) - a / i ( z ) .
(2.10)
It is clear that demanding that the currents E_a(z) be primary forces h to lie in
374
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J.M. Figueroa-O'Fanill / Casimir algebras
the Cartan subalgebra. Computing the OPE of Tde{ with E_a we find TM(z)E_a(w)
=-
/ (z-w)
°"
+
— z-w
+ reg,
(2.11)
where we have used that [h,E_a]= -a(h)E_a. Demanding that for a a simple root, E_a have zero conformal weight we get the following conditions on h: a(h) = 1 for all simple roots a. Since the simple roots span the dual h* to the Cartan subalgebra, these conditions fix h uniquely. We now determine h. The restriction of the invariant symmetric bilinear form ( , ) to the Cartan subalgebra h is non-degenerate. Under the induced isomor phism h -»h*, h gets sent to h . We shall determine h . Since the fundamental weights {A,} span h* we can expand h as h = E,MIA,- Using the fact that (A,, otj) = 5 ( ; |(a ; , ctj) and also that (h , a,) = ctj(h) = 1, we can solve for the coeffi cients /i,. Therefore h = E,(2/(a„ a,))A,. Notice that if g is simply laced then h is simply a multiple of 5, half the sum of all the positive roots. We will compute the norm of h (or equivalently that of h) for all g later on when we compute the central charges of the Casimir algebras. The upshot of all this is that T^ still satisfies a Virasoro algebra with central charge given by c^, = c(g,A:)- \2k(h,h) and that the currents E±a for a a positive root are still primary with respect to T^ with weights A ± a = 1 ± ht a. Since the BRST operator is a closed contour integral of a current, BRST invariance of the Virasoro stress tensor is equivalent to the current being primary of weight 1. This is clearly the case if we assign to the (anti)ghost pair (ba, ca) the conformal weights (1 - ht a, ht a), which corresponds to the stress tensor T*=
Z
[(hta-l)(badca)
+ hta(dbaca)],
(2.12)
which obeys the Virasoro algebra with central charge Cgh=-2 E
(6(hta)2-6hta + l).
(2.13)
Since the total stress tensor 7"tot = Tdef + T& is BRST invariant and obeys a Virasoro algebra with central charge c = c^ + cgh, the BRST cohomology Hrf(M) of any g-module M inherits the structure of a Virasoro module with central charge given by c. We now come to the calculation of the central charge for the Casimir algebra of an arbitrary finite-dimensional simple Lie algebra g. If we let 8 stand for the maximal root, the level x of the representation of the affine algebra g is given by x = 2k/\6\2. Moreover, the eigenvalue of the quadratic Casimir in the adjoint
375
J.M. Figueroa-O'FarriU / Casimir algebras
457
representation is given by cg = |0|2g*, where g* is the dual Coxeter number. The central charge c = cdef + cgh is then given by d g* ^—^ — 6JC|©| 2 |/I| 2 — 12 E
c=l
((hta)2-hta).
(2.14)
This expression is manifestly independent of the choice of invariant bilinear form ( , ), since the multiplicative factor in h is compensated by the inverse factor in h*. Therefore we choose to compute things with the Killing form K. The eigenvalue of the quadratic Casimir on the adjoint representation is identically 1 with this choice and this means that |0| 2 = l/g*. Also we notice that since h acts diagonally on g in such a way that [h, £„] = h t a £ a , its norm relative to the Killing form is just |/t|2 = 2E a e 4 ) + (hta) 2 . These remarks allow us to rewrite (2.14) as c=/ - - ^ - — x
+8
8
E a
(hta) 2 (x + g*) + 12 E
e*+
hta.
(2.15)
oG* +
Therefore the central charge of the Casimir algebra is expressed in terms of the rank, the dimension, and the dual Coxeter number of the algebra - all of which are tabulated in standard references on the subject; as well as the sums over the positive roots of the heights and their squares. These are straightforward to compute from the explicit realizations for the root systems in terms of linear combinations of the standard orthonormal basis of euclidean n-space. Such real izations are standard and can be found, for example, in ref. [17]. Table 1 summarizes the information relevant to the calculation of the central charges. With this information it is then straightforward to compute the central charge of the Casimir algebra according to eq. (2.15). For the (A,D,E) series - i.e. the simply-laced algebras - the choice x +g* =p/q e Q, where p and q are coprime TABLE 1
Parameters for the calculation of the central charges g A/ B,
c, D, E6 E7
E„ F4
G7
*
«•
£<»e*. hta
E„ e * + (hta) 2
Kl + 2) /(2/+1) /(2/+1) 1(21 - 1) 78 133 248 52 14
/+1 2/-1 /+1 2(/-l) 12 18 30 9 4
iKl + 1X/ + 2) i/(/+ 1X4/- 1) |/(/+lX4/-l) |/(/-lX2/-l) 156 399 1240 110 16
i/(/ + 1)2(/ + 2) |/(/+lX2/-lX2/+l) il(l + 1X2/ - 1X2/ + 1)
d
l/(/-l) 2 (2/-l) 936 3591 18600 702 56
376
458
J.M. Figueroa-O'FarrUl / Casimir algebras
natural numbers, corresponds to the discrete series of the Casimir algebras: cA< = ill - ( / + ! ) ( / + 2) iP~q)
I,
(2.16)
-I,
(2.17)
(P-QY C
D, =
l
l-2(/-l)(2/-l)PQ
l c
(P-QY\
E6 = 6 | l - 1 5 6 — — j ,
c c
(2.18)
^- 7 ( 1 - 3 4 2 ^r]'
(219)
E8 = 8 | l - 9 3 0 — — j .
(2.20)
In particular notice that the A, discrete series (2.16) agrees with that of the W/+1 algebras, the Virasoro algebra being W2. The unitary subseries are obtained setting p = m and q = m + l. Then for m >g* we obtain the unitary discrete series of the coset construction [7].
3. The cohomology of the BRST operator In this section we will analyze the cohomology of the BRST operator in some detail. A naive counting of degrees of freedom suggests that the reduced quantum theory (i.e. the one whose quantal space is given by the BRST cohomology at zero ghost number) has / degrees of freedom in "units" where a free boson would constitute one degree of freedom. We will make this observation precise by computing the BRST cohomology of a highly reducible module, namely the Fock space of a free-field representation for the affine algebra g. Under some assump tions we will see at the end of the section what this implies for the BRST cohomology of an irreducible g-module M. Fortunately we will not need the explicit form of the g currents in terms of free fields but only some qualitative properties of them and, of course, their existence. This last assertion is guaranteed by the work of ref. [18] which, although unable to give a general formula for the g currents, give us a method to compute it. It seems clear that there is no obstruction to their construction and that, in fact, a free-field realization exists for any g in terms of / free bosons with background charges and dim
377
J.M. Figueroa-O'Farrill / Casimir algebras
459
In this realization the Sugawara tensor decomposes into a sum of free-field tensors: T*=T; + Tly,
(3.1)
where r ; = £ ( - i t o > . - ) 2 + G,3V.-). Tj,y-
Z
(/Vr„),
(3-2) (3-3)
where the Qt are background charges. The deformed energy-momentum tensor is obtained from Tg by adding to it —dh. The general form of h in the free field representation is h = a-dv+
Z
to<*{paya).
(3.4)
To see this notice that in the free-field representation E_a = (5a + ..., where the dots correspond to terms of the form yaiya2.-.yaJa+ai + ...+an. Since [h,E_a] = - h t a E_a this fixes the coefficient in front of (Paya) in the free-field expansion of h. Therefore the deformed stress tensor in the free-field representation takes the form T*t=T9-
Z
[(hta-l)(f}adya)
+ hta(df}aya)],
(3.5)
where 7^ has the same form as T£ except for different background charges. The full BRST invariant stress tensor is thus the sum of two terms: Tv and T given by 7=
Z
[(to<*-l)((ba*ca)-(Padya))
+ hta((dbaca)-(dfiaya))].
(3.6)
The general form of the BRST current can be read off from eq. (2.9): W r =
-
Z
Ca+
Z
( 0 „ O + I
Z
'"a^CaC^fca+^ + • • • .
(3-?)
where dots stand for terms of the form y/3c coming from the y/3 terms in E_a. In particular we notice that the BRST operator is independent of tp. We now consider a Fock-space representation of the free-field algebra: sr= # ® j?
®^
.
378
460
J.M. Figueroa-O'Farrill / Casimir algebras
The BRST operator acts as the identity on J^
and hence its cohomology is
Ht,(r)sJt>99Hd(<X%r9'**)-
(3-8)
Letting C = J^y ® JPgh we will prove in this section that Hd(C) s C. The proof is a straightforward extension to the general case of the one given for g = A 2 in ref. [12] as part of the explicit construction of W3 from A^. The crux of the proof relies on the observation that the BRST operator d contains a piece d0 given by the contour integral around 0 of E ae< j, + (^„c a ) obeying d\ = 0 whose cohomology is almost trivial. In fact we have Lemma. Hdo(C) = C. Proof. We need to introduce some notation first. C is generated by the creation operators of the fields {ba,ca,fia,ya} acting on the sl2 invariant vacuum O0, which is annihilated by the following modes: (ba)p, (/3„)p for p^hta; and (ca)p, (ya)p for p > (1 - ht a). For every kind of field let us now define the following creation (a f ) and annihilation (a) operators:
Vp>(l-hta), «(/UP=
-(ya)Pl
<*Hya)P = (ya)-p
Vp^hta,
(3.9)
and the same for b and c except for the minus sign in the definitions of a(ba). With this notation and if A' is a free field, [a(X)p,a\X)q]±
= 8pq,
(3.10)
for allowed p, q. A short calculation further shows that d0=
E
{a'(Pa)pa(ba)P
+ ^(ca)pa(ya)p).
(3.11)
+ a\ya)pa{ca)p).
(3.12)
a,P allowed
Let us define the operator K as follows: *=
E a,P allowed
{a\ba)pa(fia)p
379
J.M. Figueroa-O'Farrill / Casimir algebras
461
This operator obeys {dQ, K) = N, where N is the full number operator diagonalized by the basis states n [flt(/3a)p]*-'[«t(6a)„]*i-'[flt(y(,)1,]'-'[flt(c<,)J,]/i-'-/Jo allowed
(3-13)
with eigenvalue L
(*„., + *;.„ + '„., + / ; . , ) < » ,
(3.i4)
a,P allowed
where &a p and la p take integer non-negative values and k'a p and /£ are either 0 or 1. Since N commutes with d{), the cohomology of d0 splits into a direct sum H do (C)= ©H,o(C<">),
(3.15)
where C (n) is the eigenspace of N with eigenvalue n. But since N is d0-exact, the cohomology resides in C(0); for any d0-cocycle
380
462
J.M. Figueroa-O'FarriU / Casimir algebras
is rather technical and not very illuminating and hence it is best relegated to the appendix. Hence from now on we will assume that we have graded C in such a way that the two conditions mentioned above are satisfied and, moreover, that the {Aa} are all positive integers. Under this grading the BRST operator decomposes naturally into a finite sum d = E,,, where deg dt = / and where some of the dt may be zero. Notice that since deg L 0 = 0, [dt, L0] = 0 for all i. In particular, [d0, L0] = 0 and so Hdo(C) = ©AHd(C/l). From the lemma, however, and since the sl2 invariant vacuum is annihilated by L 0 , H
381 J.M. Figueroa-O'Fanill / Casimir algebras
463
cochains £ obeying <]f = d(; would be in C, which, by definition, consists of finite linear combinations of basis elements of the type (3.13). Note also that the grading is not bounded from below. Had this been the case then each Ch would have been a bounded complex and the above theorem would have followed trivially from the lemma by a standard spectral sequence argument. As an immediate corollary of this theorem we conclude that under the isomor phism Hd(&~) = JSfv and given that T(z) induces the zero operator in cohomology, the operator induced by 7tot is precisely Tv. Therefore, as a Virasoro module, H rf (JF) is precisely the one defined by the Fock space of / free bosons with background charges. Moreover, by abstract nonsense, it follows that T(z) = {d, t(z)}, which was proven by Bershadsky and Ooguri [16] for the case of A, and A 2 and conjectured for the rest of the A„ series. Moreover, if M is a g-module embedding equivariantly in a Fock space J^ ® J^py in such a way that the embedding splits, i.e. that there is a g-module N such that Jfy ® Jfpy = M 8 N , then the above theorem implies that the BRST cohomology for non-zero ghost number vanishes: H r ° ( M ® ^ h ) = 0,
(3.16)
which means that the complex (M ® J^,, d) provides a resolution of H^(M ® JPgh) and thus allows the use of Lefschetz-trace-type formulas in order to compute the traces of operators on H^(M ® J^,) in terms of the alternating traces of their lifts to BRST invariant operators in M ® ^ h . It is not clear whether there are any interesting g-modules satisfying these properties. But even if the embedding does not split one can still take advantage of the vanishing of the BRST cohomology for the Fock module by first constructing a Fock resolution of the relevant g-module M. In the case of A ^ and A(^ (which are the only cases for which this construction has been explicitly worked out) the BRST operator intertwines between the Fock resolutions of the affine algebra and of the Casimir algebra. The resulting double complex is easy to analyze using standard techniques in homological algebra [16]. 4. Conclusions In this paper we have outlined a quantum homological construction of the Casimir (extended conformal) algebra associated to a finite-dimensional simple Lie algebra g based on the quantization of the constrained system introduced by Drinfield and Sokolov. We have found the stress tensor in the general case and have proven that, in the framework of a free field representation for the currents of the affine algebra g, it agrees with the one of / = rank g free bosons with background charges. We have computed the central charge of the Casimir algebras as a function of the level for arbitrary Lie algebra g and have found, in the simply laced case and
382
464
J.M. Figueroa-O'Farrill / Casimir algebras
for certain values of the level, their discrete series. The unitary subseries agrees with the one suggested by the proposed coset construction. For the non-simply laced algebras we do not seem to recover the coset discrete series in the same fashion. Understanding why the construction is different in this case is, in our opinion, a very interesting and important open problem. It is a pleasure to thank Peter Bouwknegt, Alvaro Diaz, Stany Schrans, Walter Troost, Toine Van Proeyen, and Dirk Verstegen for many useful conversations. I am particularly grateful to Dirk Verstegen for his ideas on how to compute the discrete series.
Appendix A THE CONSTRUCTION OF THE GRADING
In this appendix we prove the existence of the grading used in the proof of the theorem in sect. 3 by its explicit construction. Recall that the grading was defined on C = <%fpy ® JlfgYl by setting deg O0 = 0 and deg ca = deg ya = - deg ba = -deg/3„=A
Va,/3,a + / 3 e * + .
(A.l) (A.2)
The inequalities obtained from type (3) terms are already contained in (A.2) since they are of the form E,A„ > A„ + ... +a . These inequalities are to be supplemented by the requirement that deg be bounded above on C \ the eigenspace of L 0 with eigenvalue h. Ch is spanned by monomials of the form (3.13) satisfying
E P{K,P + K.P + la,P + l'a,P)=h, a,p allowed
(A.3)
383
J.M. Figueroa-O'Farrill / Casimir algebras
465
where we have used that for a primary field
(A-4)
K(-ka.p-k'a,p+la.p + l'a,,)-
allowed
Demanding that this be bounded on each Ch is clearly equivalent to the following inequality: E
[(-A„-MP)(*(,.p + *;.P) + (Aa-/i/»)(/..p + / ; . p ) ] < 0 ,
(A.5)
a,p allowed
for some ix. Since ka + k'a p and la p + l'a p can grow arbitrarily large, expression (A.5) is equivalent to the following two inequalities on the {Aa}: -\a^fip, Aa
Vp>l-hta
(A.6)
Vpsshta,
(A.7)
which can only be true if fi is positive. Now, (A.6) is equivalent to — A0 < /u.(l - ht a) and (A.7) is equivalent to A„ < /x ht a which combine together into / n ( h t a - 1) < A „ < / i h t a .
(A.8)
For convenience let us define Aa = A a //i. In terms of these new variables the system of inequalities (A.l), (A.2) and (A.8) becomes Aa>0, A„ + A p > A a + / l , hta-KA„
Vae4,
(A.9)
Va,/3,a+/3G*+,
(A.10)
Vae$+.
(A.ll)
Evidently Aa = ht a almost satisfies the second inequality. Thus it behooves us to choose the {Aa} just below ht a at a distance which decreases as the height increases so that the second inequality can be satisfied. It is then obvious that there is no problem in satisfying everything. Basically it all comes down to the fact that there is a lot of room in the interval. A possible choice of the {Aa} is the following: Aa = h t a - 4 h , a e ,
(A.12)
where e = 4 _ < M + 1 ) j ftf being the height of the maximal root. Choosing /x = 4 M + 1
384
466
J.M. Figueroa-O'Farrill / Casimir algebras
we have Aa = 4 M + 1 h t a - 4 h , ° ,
(A.13)
which is an integer satisfying the system of inequalities (A.1), (A.2) and (A.8). This proves the claim in sect. 3. References [1] A.B. Zamolodchikov, Theor. Mat. Phys. 65 (1986) 1205 [2] V.S. Dotsenko, Nucl. Phys. B235 [FS11] (1984) 54 [3] P. Bouwknegt, Phys. Lett. B207 (1988) 295; MIT Preprint CTP-1665 (December 1988), Proc. Infinite dimensional Lie algebras, CIRM, Luminy, July 1988, to be published [4] V.G. Knizhnik, Theor. Mat. Phys. 66 (1986) 68 [5] M. Bershadsky, Phys. Lett. B174 (1986) 285 [6] S.A. Apikyan, Mod. Phys. Lett. A2 (1987) 317 [7] F.A. Bais, P. Bouwknegt, K. Schoutens and M. Surridge, Nucl. Phys. B304 (1988) 348 [8] P. Goddard, A. Kent and D. Olive, Phys. Lett. B152 (1985) 88; Commun. Math. Phys. 103 (1986) 105 [9] F.A. Bais, P. Bouwknegt, K. Schoutens and M. Surridge, Nucl. Phys. B304 (1988) 371 [10] K. Hamada and M. Takao, Phys. Lett. B209 (1988) 247 [Erratum: B213 (1988) 564] [11] J.M. Figueroa-O'Farrill and S. Schrans, Phys. Lett. B245 (1990) 471 [12] A.H. Diaz and J.M. Figueroa-O'Farrill, KUL-TF-preprint 90/10 [13] V.G. DrinfeW and V.V. Sokolov, J. Sov. Math. 30 (1984) 1975 [14] J. Balog, L. Feher, P. Forgacs, L. O'Raifeartaigh and A. Wipf, Dublin IAS preprint DIAS-STP-8931 [15] V.A. Fateev and S.L. Lykyanov, Int. J. Mod. Phys. A3 (1988) 507 [16] M. Bershadsky and H. Ooguri, Commun. Math. Phys. 125 (1989) 49 [17] J.E. Humphreys, Introduction to Lie algebras and representation theory (Springer-Verlag, New York, 1972) [18] A. Gerasimov, A. Marshakov, A. Morozov, M. Olshanetsky and S. Shatashvilli, Wess-ZuminoWitten models as a theory of free fields
385
Reprinted with permission from the Proceedings of the 1991 Cargese Summer School "New Symmetry Principles in Quantum Field Theory" pp. 433-447, 1992 © 1992 Plenum Press, New York W-ALGEBRAS AND LANGLANDS-DRINFELD
CORRESPONDENCE
Edward Frenkel Department of Mathematics, Harvard University, Cambridge, MA 02138 USA
ABSTRACT The W-algebras, associated to arbitrary simple Lie algebras, are defined as the cohomologies of certain BRST complexes. This allows to prove many important facts about them, such as determinant formulas, duality and free field resolutions for generic values of the central charge. A classical limit of a W-algebra can be identified with the center of the universal enveloping algebra of the corresponding affine Kac-Moody algebra. This gives some information on the geometric Langlands-Drinfeld correspondence for complex algebraic curves.
1. I N T R O D U C T I O N The W-symmetry is one of the most interesting among the new symmetries, recently discovered in conformal field theory (CFT). Unlike other symmetries of CFT, it is not generated by a Lie algebra: the relations in the corresponding conformal algebra, which is called the W-algebra, are highly non-linear. The appropriate mathematical language for W-algebras is the theory of vertex operator algebras (VOA) [1]. The VOA of the W-algebra is its vacuum representation, in which every vector defines a linear operator, depending on a complex parameter: a local field in the holomorphic sector of the cor responding CFT. The operator product expansion (OPE) expresses the composition of two local fields in terms of other local fields. In this work I will use the definition of the W-algebra W(g), associated to a simple Lie algebra g, by means of the quantum Drinfeld-Sokolov reduction [2]. Namely, W(g) appears as the cohomology of a certain BRST complex, which involves the affine KacMoody algebra g of g and fermionic ghosts, associated to the currents to the maximal nilpotent subalgebra n of g. This approach has many advantages. First of all, it works for any simple Lie algebra g and any level. Second, the OPE of the W-algebra closes automatically. Third, we can use standard homological technique to prove important facts about the W-algebra. In particular, we can compute the Walgebra, using a spectral sequence. For generic central charge this allows us to identify the VOA of W(g) with a subalgebra of the VOA of free fields, associated to the Cartan
386
subalgebra of g, which lies in the kernel of certain vertex operators. Moreover, W() is the Oth cohomology of a certain complex, which looks like the Bernstein-GelfandGelfand (BGG) resolution of the trivial representation of g. Higher cohomologies of this complex vanish for generic central charge. When the central charge tends to infinity, the W-algebra degenerates into the Gelfand-Dikii algebra (or classical W-algebra), which is obtained by the Hamiltonian reduction (due to Drinfeld and Sokolov [3]) of the Poisson algebra of local functionals on the dual space to g. We are then able to prove that the W-algebra is a quantization of the Gelfand-Dikii algebra in the usual sense: the Fourier components of the local fields of the W-algebra are quantum deformations of elements of the Gelfand-Dikii algebra, and their Lie bracket is a quantum deformation of the Poisson bracket in the Gelfand-Dikii algebra. It means that the W-algebra is essentially finitely generated: there is a finite number of fields: Wi(z),..., Wr(z), where r is the rank of g, such that the vacuum representation is linearly generated by polynomials in their Fourier components, applied to the vacuum vector. In other words, the O P E of Wi(z) and Wj(w) can be expressed in terms of local fields, which are polynomials in Wk(w), 1 < k < r and their derivatives. The conformal dimension of W±{z) is equal to d,; + 1, where di is the ith exponent of g. For example, W(s/2) is the Virasoro algebra, and W(s/3) is the Zamolodchikov algebra [4]. For simply-laced Lie algebras W(g) have been defined by Fateev and Lukyanov [5] by means of the direct quantization of the Miura transformation (which is only possible in the simply-laced case). This gives explicit formulas for the embedding of the W-algebra into the free fields, or, in other words, for the Oth cohomology of our free field resolution. The difference is that we do not need to prove the closure of the OPE, it is insured automatically from the very beginning. Our definition of the W-algebra also gives a functor from the category of positiveenergy representations of g to a category of representations of W(g), which is studied in detail in [6]. It is possible to define minimal representations of W(g), compute their characters (as residues of the affine characters) and fusion coefficients. There are two classical limits of W(#): when the level of g tends to infinity, it de generates into the Gelfand-Dikii algebra, associated to g, and when the level of g tends to minus dual Coxeter number, which is called the critical level, it degenerates into the Gelfand-Dikii algebra, associated to the Langlands dual Lie algebra g' [2, 7]. It has been proved by Feigin and myself [2, 7], that this limit can be also identified with the center of a local completion U(g)ioc of the universal enveloping algebra of g. This result plays an important role in the recent development of the geometric Langlands correspondence, which is due to Drinfeld. The concept of Langlands correspondence (for an introduction to the Langlands Program see, e.g. [8], see also [9], where its relation to CFT was first suggested) is one of the most important and universal in mathematics. It relates local and global properties of a field k. Namely, there is a one-to-one corre spondence between the automorphic representations of an algebraic group G\ over the ring A of adeles of k and homomorphisms from the Galois group of k to the Langlands dual group G'. A representation is automorphic, if it. occurs in the decomposition of the space of functions on the coset space Gx/Gk- An unramified automorphic representa tion, which contains an invariant vector with respect to the compact subgroup K of G\, defines a function on the double coset space K\Gx/Gk. In our case k is the field of rational functions on a complex curve £, and the role of the Galois group is played by the fundamental group of £. The adele group Gx can be described as the product of the loop groups LGp,p 6 £ of G over all points of the curve £. Here LGP is the group of maps from a small circle Sv around the point p to G. The
387
compact subgroup is the product of the subgroups LG+ of LGP, where LG+ consists of the holomorphic maps from the interior of the circle Sp to G. The double coset space is then the moduli space MG{£) of stable G—bundles over £. In the geometric version of the Langlands correspondence, proposed by Drinfeld [10], the unramified representation of the adele group are replaced by certain holonomic sys tems of differential equations (or, more generally, by 2?—modules) on MG{£)There is a surjective map from the center of U(g)\oc at the critical level to the algebra of differential operators on the bundle of half-forms on MQ{£) [11]. Our description of the structure of the center implies "half" of the Langlands-Drinfeld correspondence, which looks very much like a suitably defined modular functor at the critical level. We see that the W-symmetry helps to understand a very deep algebro-geometric concept. This is yet another example of the impact that two-dimensional conformal field theory has had on modern mathematics in the last few years. The results of this paper were obtained in collaboration with Boris Feigin. 2. D E F I N I T I O N O F T H E W - A L G E B R A Let g be a complex simple Lie algebra, and g - its affine Kac-Moody algebra, which is the extension of g igi C[tf,<-1] by the central element K. It is linearly spanned by K and A(m) = A® tm, A g g,m g Z. Let k be a complex number. We denote by Uk(g) the quotient of the universal enveloping algebra of g modulo the relation K — k. We call k the level of g. Let Vk be the vacuum representation of g, generated by the vacuum vector, annihilated by g ® C[t], on which K acts by multiplication by k. The space Vjt carries the structure of vertex operator algebra (VOA) [1]: every vector of Vk defines a local field, which is a formal series in z and z~1, whose coefficients are linear operators, acting on Vk. There is an operator product expansion (OPE) for the product of two local fields (c.f. [2] for details). The Fourier coefficients of local fields form a Lie algebra, which we denote by Uk(g)ioc. It lies in a completion of Uk{g) and is linearly spanned by Fourier coefficients of the normally ordered polynomials in the basic local fields A(z) = £ A(m)z~m~l, A g g and their derivatives [2]. The Lie bracket in Uk(g)ioc is completely determined by the singular part of the OPE. Denote by n the upper-nilpotent subalgebra of g. It is spanned by the root vectors ea,a g A + , where A + is the set of positive roots of g. Put n = n ® C [ t , < - 1 ] . Let us introduce the Clifford algebra, which is generated by i/> a (m),t/'*(m),m g Z , a g A + with the standard anti-commutation relations: [ipa(n),ip"0(m)} =
6aJ)6n-m.
Denote by A its irreducible representation, generated by the vacuum vector, annihilated by tp(m),m > 0,i{>'(m),m > 0. It is Z—graded: degt/>(m) = —1, degV>*(m) = 1. The space Vk ® A has a structure of complex. The differential is given by d = dst + p. Here
dst = / ( £ or6A+
ea(z)ra(z)
- \
£
cl^l(z)r0{z)^z))dz,
a,/3,-(6A+
where c ^ are the structural constants of n, is the standard differential of Lie algebra cohomology of n, and
P= I E ra,(z)dz.
388
We have:
389
n, and x be such that x(ea) = 1, if a is a simple root, and 0, otherwise. Clearly, one always has a map from the center of U(g) to the Hecke algebra. In general, this map may well have both a kernel and a cokernel: there may be other elements in the Hecke algebra, and some of the central elements may act by zero on the space (M ® C x ) 6 for any g—module M. Kostant showed, however, [13] that in this example the Hecke algebra is isomorphic to the center of U(g). He also showed that all other cohomologies of the complex £/((?) ® Cl vanish. Our definition of the W-algebra is a generalization of this construction. Moreover, as we have shown in [2, 7], there is an affine analogue of the Kostant's result on the cohomologies of our complex, when k = —hv (cf. Sect. 4).
3. F R E E FIELD R E S O L U T I O N S In this section we will construct free field resolutions of W-algebras for generic values of the central charge. Our strategy is the following: first we will construct a resolution of the vacuum representation of the affine algebra g in terms of the Wakimoto modules for generic level. Then we will convert it into a resolution of W(g) in terms of Fock representations, using the vanishing of the cohomologies of the Wakimoto modules. The vanishing of higher cohomologies of this resolution for generic central charge c of W(g) will follow from the acyclicity of its classical limit, when c tends to infinity. Let us denote by W\tk the Wakimoto module over g of level k with highest weight A [14, 15]. There exists an explicit realization of this module in terms of r free scalar fields and |A+| ^ - s y s t e m s . We know [16] that H{(WXyk) = 0, if j ^ 0, and H^(Wx,k) = n\,k+hv, where TA,*+/IV is the Fock representation of the Heisenberg algebra of level k + /i v with highest weight A. This Heisenberg algebra is generated by u ( m ) , m (E Z , u £ h - the Cartan subalgebra of g with the standard commutation relations: [u(n), u(m)\ = (k +
hw)n(u\v)6n,-m,
where (|) denotes the invariant scalar product on h. Throughout this Section we will assume that k ^ — hv. Therefore we can normalize the Heisenberg algebra by introducing new generators u(m) = u(m)/i/, where u = \/k + /i v . Then n\rk+hv becomes itx/Vti = ■K\/v. Denote by a<, 1 < i < r, the set of simple roots of g. We have the following complex: Ck(g) = ®Ck(g), where Cite) = ©J(.)=iW.(p)-p.t, where s runs over the Weyl group S of g and p is the half-sum of the positive roots of g. Let me give explicit formulas for the differentials of this complex. Introduce the screening operators Si = / Si(z)dz, s z
ii )
-
ti{z)v-a>l»(z)'
where V^/^z) denotes the bosonic vertex operator, acting from ■K\/t/ to 5T(A+-,)/1/ (and therefore from W\,k to W\+~,tk) and e.\{z) is a certain polynomial in 01—fields, which comes from the right action of the Lie algebra n on W\
390
where 1 < t; < r, and 7 is equal to £ a<(. [«M •••■»••„] = J dzl...dznsil(z1)...sin(zn),
(1)
where T is a set of contours taken counterclockwise from the basepoint z = 1 to itself around 0 and nested according to |zi| > . . . > |z„|, as in [18]. These operators obey the Serre relations of the quantum group Uq{g), where q = exp ni/(k + hv) [18, 19]. It means that there is a well-defined linear map e, from the nilpotent quantum group Uq(n) to End(®W1
nis) = ®Fi(s),
The differential rPk : Fk(g) —* Fk(g) of this complex is given by the same formula as the differential dj of the complex Ck(g), using the operators [ i ] . . . i n ] , which are given by formula (1), where Si(z) is to be replaced by V^(z) = V_ a -/„(z). This two operators are equivalent, because they differ by a commutator with the differential of our BRST complex. The monodromy properties of the operators V^l\z) are the same as the monodromy properties of the operators s,-(z), therefore again £ ) J + 1 D J = 0. This complex is well-defined for any k. It is possible to extend this complex to the value k — 00. In order to do that we should pass to a new basis in TTA/I/, which consists of all monomials in u'(m) = u(m)/// 2 , m < 0. We should also rescale the differentials of the complex Fk(g), passing from [*»...*„] to f 2 n [i'i... t n ]. In this limit Wk(g)ioc degenerates into the Gelfand-Dikii algebra, in which the Poisson structure is given by the (k + /i v ) - 1 —linear term of the Lie bracket in W*(^)iocNow I want to explain, why higher cohomologies of this complex vanish for generic k.
391
We have a family of complexes Fk'(g). Each of them decomposes into a direct sum of finite-dimensional subcomplexes Fk(g)n, n > 0, where Fk(g)n is the eigenspace of the operator L 0 € W*(<7)ioc with the eigenvalue n. The differential Dj. decomposes into a sum of differentials Di(n) : Fk(g)n —> Fk+l(g)n. As linear spaces F£(g)n do not depend on A;. The differentials Z^(n) depend algebraically on u~2 = (k + A v ) - 1 . Therefore the dimension of the kernel of [^(n) is the same for all but finitely many values of k, where it may jump up. The dimension of the image of D{~l(n) is the same for all but finitely many values of k, where it may jump down. Thus the dimension of the j t h cohomology of the complex Fk(g)n is the same for all but finitely many of values of k, and in special points it may only jump up. In particular, if for some value of k the j t h cohomology of the complex Fk(g) vanishes, then it also vanishes for generic value of k (i.e. for all but countably many values of k). So now in order to prove the vanishing of higher cohomologies for generic ifc it is enough to prove it for some value of k. I will do it for k = oo. In fact, the vanishing of the higher cohomologies for k — oo follows from [3], Proposition 6.1. But I will give another proof, which will lead to a better understanding of the meaning of the complex
™When v i/ / V^(z)dz 2
1
—► 0, the modules w\/„ get identified with -KQ. The limit V; of the operator is equal to
where [d/du'(m),v'(n)] generating function
= (u\v)6ntm,m,n
'£Vt(l)z' /<0
=
< 0, and V;(/) are defined by the following
exPC£o'i(m)zm/m). m<0
The composition operators [ t i . . . t„] become the products V^ ... Vin. The operators VJ, 1 < i < r generate the nilpotent subalgebra n of g. It is a useful exercise to check this directly. Therefore the complex F^g) is isomorphic to Homn(Z?'((/),7ro), where Bl(g) is the BGG resolution of the trivial representation of g. Indeed, for any A the module M> is a free n—module M. Therefore the module of n—homomorphisms Hom n (M, ir0) is canonically isomorphic to TTO, namely, any non-zero homomorphism x S Hom„(Af, 7r0) defines a non-zero element in N: the image of the lowest weight vector of M . The embedding of M into itself, which is given by the singular vector P , y , induces the homomorphism from %o to TT0, which sends y g TT0 to P,y • y. Hence the differentials of the BGG resolution Bl(g) go to the differentials of the complex F^(g). It means that the cohomologies of the complex F^(g) coincide with the cohomologies of the Lie algebra n with coefficients in JTO (with respect to the action by the operators Vi). This action is "co-free" (i.e. the action on the dual module is free). In other words, we have ir0 = W<x{g) ® Mm, where M' is the dual module to the free n—module. It implies that the 0th cohomology is the space Woo(g) of invariants of 7To under the action of n, and that all higher cohomologies vanish. Therefore higher cohomologies also vanish for generic k. Recall that for any £—module M the cohomolgy H3k(M) is a module over Wk{g)iocIn particular, H3k(Vk) is the vacuum representation of Wk(g)ioc (which is also the VOA Wk(g))- So we may view the complex F£(g) as a BGG resolution of the vacuum repre sentation of Wfc(<7)ioc in terms of Fock representations. We have proved the following result.
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T h e o r e m 1 For generic k there is a resolution F£(g) = G)F£(g), where F
k(9)
=
®l{M)=j*(.(p)-p)/V,
of the vacuum representation of the W-algebra Wk(g)ioc *" terms of the Fock repre sentations, such that the Oth cohomology is the vacuum representation, and all higher cohomologies vanish. For g = 5/2 this result follows from [22]. For g = sln this result was obtained in [23] by other means. It is natural to conjecture that there is a (highly non-local) action of the (nilpotent) quantum group Uq(n) on TT0 for any k and q — expiri/(k + ftv), such that it commutes with the action of Wk(g)ioc and with respect to their action the module TTO decomposes as Wk(g) ® M" for generic k. Theorem 1 would follow from this conjecture, because if it was true, then for any k the complex F£(g) would be isomorphic to Homi^(n)(.BJ,7ro), and so its cohomologies would coincide with the cohomologies of Uq(n) with coefficients in n0. Therefore higher cohomologies would vanish for generic fc, because the action of Uq(n) on ir0 would be "co-free". It follows from Theorem 1 that for generic k the W-algebra W*() is isomorphic to the intersection of the kernels of the operators / V^>(z)dz : TTQ —+ ir_ 0l ./„. (In [2] we proved this result in a slightly different way.) Clearly, the elements of Wk(g) depend algebraically on fc, therefore they define a VOA for any fc. Note that this VOA is contained in Wt() (defined as the Oth cohomology of a BRST complex, cf. Sect. 2) even for non-generic fc, so that we have a family of algebras, depending on a complex parameter fc. It follows from our conjecture on the vanishing of cohomologies of the BRST complex, that it is isomorphic to Wk(g) for any fc. Note that the complex F£(g) is well-defined for any fc, but for special values of fc its cohomologies jump up, so that it is no longer a resolution of H°(Vk) (in other words, the action of Uq(n) is no longer "co-free"). It happens exactly when H°(Vk) is not irreducible (as it is for generic fc), but contains an extra singular vector. We then should take the quotient modulo this vector to obtain the irreducible vacuum representation in this case. The free field resolution of such module should be two-sided (as it is in the case of W^sty, which is the Virasoro algebra [24]). Such resolution was conjectured in [6, 19]. We can calculate the character (or partition function) of the W-algebra Wk(g) for generic fc. The simplest way to do that is to calculate it for fc = 00 (obviously, it will be the same for generic fc). Using the decomposition ir0 = W00(g) ® M*, we find: chW((/) = ch5r 0 -(chM*)- 1 , where chX = £ d i m Xmtm. We have: ch7r0 = rim>o(l — < m ) _ 1 - Since the operators VJ the generators of the Lie algebra n - have degree 1, chM* = rii
chw(5)= n n o-tT 1 . l«J,
This implies that the W-algebra is essentially finitely-generated: there are fundamental fields Wi(z), 1 < t < r, of conformal dimensions <£ + 1 , such that the ordered polynomials in their Fourier complonents W,(m,),m,- < -rf, constitute the (Poincare-Birkhoff-Witt) basis of Wk(g) (or, in other words, the VOA is spanned by normally ordered polynomi als in Wi(z) and their derivatives. The formula for W1(z), whose Fourier components generate the Virasoro subalgebra of the W-algebra, is given in [2] for any g.
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Explicit formulas for other generators of the W-algebra were given by Fateev and Zamolodchikov [25] for g = sl3, and by Fateev and Lukyanov [5] for sln and S02n, n > 3. Their formulas were obtained by direct quantization of the Miura transformation. It is easy to check that the corresponding fields are indeed in the kernel of the vertex operators / V^'{z)dz. Since they have the correct conformal dimensions, they generate the whole W-algebra. It is important that we do not need to prove that their operator product closes: it automatically follows from our definition of the W-algebra. For non simply laced algebras one can not directly quantize the Miura transformation, and I do not know any anzatz for the fields W{(z) in this case. From the description of the W-algebra as the kernel of vertex operators and the existence of the Poincare-Birkhoff-Witt basis the determinant formulas [26] follow, using the explicit formulas for the intertwining operators as contour integrals of vertex operators V'''(z). Further results on the representatation theory of W-algebras can be found in [5, 6]. The Lie algebra Wk(g)ioc of the Fourier components of the local fields from Wk{g) is a quantum deformation of the Gelfand-Dikii algebra W^g^o^, associated to g. Let us pass to the basis in Wjt(<7)ioc, constituted by polynomials in u'(m),u 6 h,m < 0. The 0th differential D° of the complex F£(g) (the sum of the vertex op erators / V^(z)dz) is equal to Ei>o<^(^ + hw)~j, where the constant term d% equals D^. The cohomology vanishing theorem guarantees that every A0 € Woo(jf) can be ex tended to an element A of W *,(#), which a polynomial in (k + hv)~l (this is the parameter of deformation), with constant term A0. We have: A = £,->0 Ai(k + h?)~'. The condition D°A = 0 for any k is then equivalent to the system of equations J2i+j=m ^j^i = 0, m > 0. I want to use these equations to determine Ai,i > 0. The first equation d%Ao = 0 is satisfied, since A0 belongs to W 0O (g'). The second equation reads d%A\ = —d^A0. There exists A\, which satisfies this equation. Indeed, we can also decompose the 1st diferential D\ of the complex F£(g) as X)j>o^](fc + hw)~3, where d\ is equal to D^. Since D\D° = 0, we have Z)i + j=o^J < ^ = 0,m > 0. In particular, d\d\ = -d\d°. Therefore
d°0An = - ( £
d?An_;).
(2)
If we apply d}> to the right hand side of (2), we obtain
l<j
0<j
0
Therefore dl{d%An) = 0, and there exists An, which satisfies (2). Thus, every element of W^g) can be deformed to an element of V\?k{g) for any k. Therefore any element a0 of the Gelfand-Dikii algebra Woo(g)\0c can also be deformed to an element a = a0 + (k + / i v ) _ 1 + . . . of Wit{g)xoc for any k. The Lie bracket of a and 6 from Wk(g)i0c is given by [a,b] = (k + /i v ) _ 1 {a 0 , &o} + {k + h*)~2(...), where {«o, bo} is the Poisson bracket of a 0 and &o in the Gelfand-Dikii algebra. It is known [3] that Woo((7)ioc is the Poisson algebra of local functional on the space of gauge classes of certain g—connections on the circle, which are intergrals of polynomials in W{(z), 1 <
394
i < r and their derivatives. For example, if g = sln, then the Gelfand-Dikii algebra is the space of local functionals on the differential operators on the cercle of the form dn + Wi(z)dn~2 + .. . + Wn-i(z). In this case the local field Wi(z) is precisely the quantum deformation of Wi{z). In the conclusion of this Section, I would like to mention that the complex F£(g) can be defined for an arbitrary Kac-Moody algebra g. As I have just explained, if g is a simple Lie algebra, then the cohomology of this complex gives the W-algebra, associated to g. In [27] Feigin and I have shown that if g is an affine algebra, then the cohomology of this complex gives integrals of motion in the quantum affine Toda field theory, associated to g. It is interesting, what is the meaning of this complex for non-affine Kac-Moody algebras.
4. C R I T I C A L L E V E L A N D L A N G L A N D S - D R I N F E L D C O R R E S P O N DENCE The W-algebra also has another classical limit: when k tends to — hw. It was proved in [2, 7], that in this limit W j t ^ i o c degenerates into a Poisson algebra, which is isomorphic to the Gelfand-Dikii algebra, associated to the Langlands dual Lie algebra g' (the Cartan matrix of g' is the transpose of the Cartan matrix of g). This result is the limit of the following duality of W-algebra: Wk{g) is isomorphic to W*<('), if r v (fc + /i v (p)) = (k' + fcv(<7'))_1, where r v is the maximal number of edges, connecting two vertices of the Dynkin diagram of g. It follows from the description of the W-algebra as the kernel of the vertex operators [2]. Let Uk{g)\0c be the local completion of the universal enveloping algebra of g (cf. Sect. 2). This is a Lie algebra. Denote its center by Zk(g). Let x (E 14 be a singular vector of imaginary degree. Then the operator product of the basic local fields of g with the local field x(z), corresponding to z, has no singularities. Therefore all Fourier components of x(z) belong to Zk(g). It is also possible to prove the converse statement [2]. It is known [28] that there is no singular vectors of imaginary degrees in Vk, if k ^ —Av. Therefore Zk(g) = C, if * # -h\ For k = —hw there is a precise analogue of the Kostant's theorem (cf. Sect. 2): the center Z_/,v($f) is isomorphic to W-hv{g)ioc [2, 7], Combined with the duality theorem, it gives the following result. T h e o r e m 2 The center of the local completion of the universal enveloping algebra of an affine Kac-Moody algebra g is isomorphic to the Gelfand-Dikii algebra, associated to g' the Langlands dual Lie algebra to g. In fact, there is a natural Poisson structure on Z-hv(g). as linear spaces for all k. If we have two central elements in bracket is a polynomial in (k + hw) with zero constant term. defines a Posson bracket on Z-h*(g). This Poisson structure structure on the Gelfand-Dikii algebra. Let me give you an example. Define the Sugawara field:
We can identify Uk(g)ioc U-hv(g)ioc, then their Lie The (k + Av)—linear term coincides with the Poisson
S(z)= £ S(n)*—2 = ± 5 : u?(*), n€Z
where u,- are the elements of an orthonormal basis of g with respect to the standard inner product. We have: [S(n), A(m)] = -m(k + hv)A(n + m ) ,
395
for any A £ g. Therefore S(n),n G Z belong to Z_/,v(<j). If g = s/ 2 , then the center is generated by S(z): every central element is a Fourier component of a polynomial in S(z) and its derivatives. We also have: [S(n), S(m)} = (k + 2)((n - m)S(n + m) + fc/4 • (n 3 - n)<5n,_m). Therefore the Poisson bracket of S(n) and S(m) is equal to (n — m)S(n + m) — 1/2-(n 3 — ra)£n,-m- Hence as a Poisson algebra Z_ 2 (s/ 2 ) is isomorphic to the Gelfand-Dikii algebra of 5/2, which is the space of local functionals on the dual space to the Virasoro algebra. The operators S(n) define a Poisson subalgebra of Z-hv(g) for any g. Some explicit formulas for other elements of the center can be found in [29]. They are unknown in general, although it follows from Theorem 2 that their symbols give all g— invariant local functionals on the dual space to g. Theorem 2 gives a possibility to assign #—modules at the critical level to certain geo metric data. Indeed, the Gelfand-Dikii algebra, associated to g is the algebra of functions (more precisely, local functionals) on the space C(g) of gauge classes of connections on the circle of special kind [3]. Let c be an element of C(g'). It defines a map fic from the Gelfand-Dikii algebra of g' to C: we take the value of each local functional at the point c. We can then define the module V_fcviC over g, taking the quotient of V_/,v modulo the relations u = /i c (u) for any u 6 Z-tiv(g). The module V-hy,c ^ 0, if and only if c can be holomorphically extended inside the circle, embedded into C. For example, C(sl2) is the space of second order differential operators of the form df + q(t) on the circle. An operator of this type can be extended inside the circle, if q(t) is a polynomial in t: q(t) = £m<-2 q{m)t~m~2. The module, corresponding to such operator, is the quotient of V_2 modulo its submodule, generated by the vectors (S(m) — q(m))u_2,m < —2, where u_2 is the vacuum vector of V_2. Now I want to describe briefly a "globalization" of the Theorem 2, which was recently proposed by Drinfeld. It relates holonomic systems of differential equations on the moduli space Mc(£) of stable principal G—bundles on a smooth projective algebraic curve £ over C to holomorphic G'—connections on £. This construction may be viewed as a quantization of a remarkable completely integrable hamiltonian system on the cotangent bundle to MG{£), which is due to Hitchin [30]. Let me recall his construction. Let T'MG{£) be the cotangent bundle to M.G{£)A point of T'MG{£) is a pair (P, £), where P is a principal G—bundle over £ and £ is a cotangent vector to Ma(£) at the point P € MG{£) (sometimes it is called a Higgs field). The tangent bundle to P is isomorphic to Hl(£,gp), where gp = P XQ g is the vector bundle, associated to P and the adjoint representation of G. So £ £ Hl(£,gT)m = H°(£,gp ® fl 1 ), where fi 1 is the bundle of 1-differentials on E, by the Serre duality. We can define a map
396
of algebraic functions on T*MG(£) is isomorphic to the space of polynomials C[H] on the space W, which is a commutative Poisson algebra. Now let us try to quantize this system. Quantization means that we assign to every classical hamiltonian h on T"A4G(£) a differential operator Dh, acting on a certain line bundle over MG{£)We also expect that the differential operators D/,, and D^, cor responding to two commuting hamiltonians hi and h2, will also commute. It is known that every line bundle over MG(£) is a power of the so-called determinant bundle £. In particular, the line bundle (,~2h is isomorphic to the canonical bundle (i.e the bundle of the volume forms) K over MG{£). The bundle K1'2 = (~hV is called the bundle of half-forms. It is natural to expect that the differential operators, which are the quantizations of the Hitchin's hamiltonians, would act on the bundle of half-forms. Indeed, if they acted on another bundle L ^ K1'2, then the dual operators would act on the Serre dual bundle KL-1 ^ L, and we would have two different quantizations. This would be too much to hope for! In fact, there is a deep relation between the center Zk(g) for integer k and the algebra of global differential operators, acting on the line bundle (k. The moduli space MG{£) is an open set in a double coset space of the loop group of G [32]. Indeed, let p be a point of £ and P - a small disc around this point. One can trivialize any bundle over both V and £ — V. Therefore any bundle over £ is defined by the transition function, which is an element of the loop group LG (maps from the boundary dV of V to G). The isomorphism classes of bundles are then identified with the double cosets GoutX-LG/Gin, where Gi a (G 0 ut) is the subgroup of LG, which consists of those maps, which can be extended inside (outside) of the disc V. The space M = LG/G^a is a homogeneous space of the Lie group LG. Therefore the Lie algebra Lg embeds into the Lie algebra of vector fields on it. For any k € Z one can construct a line bundle (k over M, such that the Kac-Moody algebra g of level k embeds into the Lie algebra of infinitesimal automorphisms of (k [32]. This bundle is G o u t — equivariant, and it descends down to the bundle f* over MG(£)• The local completion Uk(g)ioc of the universal enveloping algebra of g at level k will map to the algebra of differential operators, acting on the bundle £* over M. Clearly, the differential operators, acting on f*, which lie in the image of the center Zjt(), commute with the action of G o u t, and therefore they define differential operators on the bundle (k over the moduli space A 4 G ( £ ) . But we know that Zk(g) is trivial for k ^ — Av, therefore it does not produce any differential operators on the bundle £*. In fact, it was proved in [31], that the only global differential operators on the bundle (k over MG{£) for k ^ — hw are constants. On the other hand, Z_/,v() produces a big algebra Diff of global differential operators on the bundle of half-forms over MG{£)More precisely, the following is true: (1) Diff is a commutative algebra, which is isomorphic to the algebra of polynomials on the space H; (2) the map Z-hv {g) —► Diff is surjective [11]. These results follow from the existence of the injective symbol map from Diff to the space of algebraic functions on T'MG{£), Hitchin's description of this space, and Theorem 2. The first statement allows to assign to any point x € H a system of differential equations on half-forms on MG{£)Namely, the point x defines a map Diff —» C, taking D 6 Diff = C[H\ to the value of the polynomial, corresponding to D, at the point x. We then consider the system of differential equations on half-forms rj on MG{£)'■ {D ■ t) = x(D)i],D e Diff}. By (1), this system is compatible, and it is holonomic, because the dimension of 7i is equal to the dimension of the moduli space MG(£).
397
On the other hand, the statement (2) shows that H is embedded into the space of connections C(g'). Indeed, by Theorem 2, the center Z_>,v(<jr) is identified with the Gelfand-Dikii algebra of g', which is the space of functions on C(g') of certain kind. We have a surjective map from Z-\v(g) to the algebra Diff, which is the algebra of polynomial functions on "H, therefore we get an embedding of the corresponding spectra:
H^C(g'). The space C(g') is the space of certain G'—connections on the circle. The image of Ji in C(g') consists of such connections, which can be holomorphically extended from the circle dT> C £ to the whole curve £. Thus, we see that each point of Ti defines a system of differential equations on the moduli space MQ(£), and a holomorphic G'—connection on £. Such a connection gives rise to a local system on £, which defines a homomorphism from the fundamental group 7Ti of £ to G'. We have therefore established a correspondence between systems of differ ential equations on MQ(£) and homomorphisms n\ —> G'. This is exactly "half" of the Langlands-Drinfeld correspondence on £. Drinfeld conjectured [10] that there should be a one-to-one correspondence between the isomorphism classes of holonomic V—modules on MQ(£) with singular support in the "global nilpotent cone" A/" and the isomorphism classes of homomorphisms from %\ to G'. Here Af = V _ 1 (0) is the lagrangian subvariety in T'Ma(£) [33]. Theorem 2 and the Hitchin's results give a correspondence between D—modules of special kind (which are defined by systems of differential equations on half-forms) and homomorphisms iti —► G' of special kind (which are defined by some holomorphic connections on £). One can show that the space W of such homomorphisms gives a lagrangian subspace in the symplectic space of the isomorphism classes of all homomorphisms 7Ti —» G'. There is another way to relate these objects. Any element c e C(g') defines the module V-hv,c over g. We can then take its coinvariants with respect to the Lie algebra gout of the Lie group G ou t- This defines a certain modular functor on the £—modules at the critical level. It is known, that for positive integer level this functor, applied to the irreducible quotient of Vjt, gives the space of conformal blocks in the WZW model [34]. For the critical level this functor, applied to VL/,viC, gives 0, if c can not be holomorphically extended to £, and it gives the space of solutions of the corresponding system of differential equations on Ma(£), if it can be extended to a holomorphic connection on £. This construction can also be generalized to the moduli spaces of bundles over the curve £ with punctures. Hopefully, it will allow to establish the Landlands-Drinfeld correspondence in general.
Acknowledgements I would like to thank the organizers of the Cargese Summer School for financial support, excellent weather conditions, and the opportunity to present this work.
References [l] I.Frenkel, J.Lepowsky, A.Meurman, Vertex Operator Algebras and the Monster, Aca demic Press 1988 [2] B.Feigin, E.Frenkel, Affine Kac-Moody algebras at the critical level and Gelfand-Dikii algebras, Preprint MSRI 04029-91, RIMS-796, to appear in Proceedings of RIMS-91 Program
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[3] V.Drinfeld, V.Sokolov, Sov. J. Math. 30 (1985) 1975 [4] A.Zamolodchikov, Teor. Math. Phys. 65 (1985) 1205 [5] V.Fateev, S.Lukyanov, Int. J. of Mod. Phys. A3 (1988) 507 [6] E.Frenkel, V.Kac, M.Wakimoto, Characters and fusion quantized Drinfeld-Sokolov reduction, Preprint, 1991
rules for W-algebras via
[7] E.Frenkel, Affine Kac-Moody algebras at the critical level and quantum Sokolov reduction, Ph.D. Thesis, Harvard University, 1991
Drinfeld-
[8] S.Gelbart, Bull. Amer. Math. Soc. 10 (1984) 177 [9] E.Witten, Comm. Math. Phys. 113 (1988) 529 [10] V.Drinfeld, private communications; A.Beilinson, Affine algebras on the critical level and geometric Langlands correspon dence (after V.Drinfeld), handwritten manuscript, and talks given at RIMS and MIT,1991 (11] A.Beilinson, V.Drinfeld, B.Feigin, V.Ginzburg, A commutative operators on the moduli of G-bundles, to appear
ring of differential
[12] B.Kostant, S.Sternberg, Ann. Phys. 176 (1987) 49 [13] B.Kostant, Invent. Math. 48 (1978) 101 [14] M.Wakimoto, Comm. Math. Phys. 104 (1986) 604 [15] B.Feigin, E.Frenkel, Russ. Math. Surv. 39, N5 (1988) 221 [16] B.Feigin, E.Frenkel, Comm. Math. Phys. 128 (1990) 161 [17] B.Feigin, E.Frenkel, in Physics and Mathematics of Strings, V.G.Knizhnik Memorial Volume, eds. L.Brink, e.a., 271-316, World Scientific 1990 [18] P.Bouwknegt, J.McCarthy, K.Pilch, Progr. Theor. Phys. Suppl. 102 (1990) 67 [19] P.Bouwknegt, J.McCarthy, K.Pilch, Preprint CERN, to appear in Proceedings of Stony Brook Conference, 1991 [20] C.De Concini, V.Kac, Progress in Math. 92, eds. A.Connes e.a., 471-506 (1990) [21] J.Bernstein, I.Gelfand, S.Gelfand, in Representations 21-64, Wiley 1975
of Lie groups, ed. I.Gelfand,
[22] B.Feigin, D.Fuchs, in Representations of Lie groups and related topics, A.M.Vershik and D.P.Zhelobenko, 465-554, Gordon and Breach 1990 [23] M.Niedermaier, Irrational free field resolutions for W(sl(n)) construction, Preprint, 1991
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[24] G.Felder, Nucl. Phys. B324 (1989) 548 [25] V.Fateev, A.Zamolodchikov, Nucl. Phys. B280 [FS18] (1987) 644
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[28] V.Kac, D.Kazhdan, Adv. Math. 34 (1979) 97 [29] T.Hayashi, Invent. Math. 94 (1988) 13 R.Goodman, N.Wallach, Trans. Amer. Math. Soc. 315 (1989) 1 [30] N.Hitchin, Comm. Math. Phys. 131 (1990) 347 [31] A.Beilinson, D.Kazhdan, Projectively flat connections, Harvard Preprint, 1990 [32] A.Pressley, G.Segal, Loop Groups, Cambridge University Press 1988 [33] G.Laumon, Duke Math. Journ. 57 (1988) 647 [34] A.Tsuchiya, K.Ueno, Y.Yamada, Adv. Stud, in Pure Math. 19, 459-565, World Scientific 1989
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Reprinted with permission from Communications in Mathematical Physics Vol. 147, pp. 295-328,1992 01992 Springer-Verlag
Characters and Fusion Rules for W-Algebras via Quantized Drinfeld Sokolov Reduction Edward Frenkel1*, Victor Kac2** and Minoru Wakimoto3*** 1 1 3
Department of Mathematics, Harvard University, Cambridge, MA 02138, USA Department of Mathematics, M.I.T., Cambridge, MA 02139, USA Department of Mathematics, Mie University, Tsu 514, Japan
Received November 8, 1991
Abstract Using the cohomological approach to IP-algebras, we calculate charac ters and fusion coefficients for their representations obtained from modular in variant representations of affine algebras by the quantized Drinfeld-Sokolov reduction. 0. Introduction The study of extended conformal algebras has been playing an increasingly impor tant role in the recent development of conformal field theory. Among them the Walgebras have attracted much attention in the past few years. The first example of a IP-algebra was discovered by Zamolodchikov [37] in an attempt to classify extended conformal algebras with two generatingfields.(Further classification of IP-algebras generated by two or three fields may be found in [8,9].) There have been developed several approaches since then to the construction of a general IP-algebra. In the series of papers [15-17, 31] Fateev, Zamolodchikov and Lukyanov defined If-algebras associated to simplefinite-dimensionalLie algebras g of type At and Dt by explicitly quantizing the corresponding Miura transformations and derived some results on their "minimal" representations. They put results in a form suitable for an arbitrary simply laced g. At the same time Bilal and Gervais studied IP-algebras as the algebras of symmetries of Toda theories [7]. In [2,9,11] the If-algebras appeared as the chiral algebras in coset models. In [34,1] they also appeared in an attempt to generalize the Sugawara construction to higher degree Casimirs. All these constructions are closely related to the invariants of the Weyl group W of g, hence the name IP-algebra. We adopt the point of view of the paper [21] by Feigin and one of the authors of the present paper, where the IP-algebra IP(g), associated to any simple * Supported in part by Junior Fellowship from Harvard Society of Fellows ** Supported in part by NSF grants DMS-8802489 and DMS-9103792 *** Supported in part by RIMS-91 Project
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finite-dimensional Lie algebra g, naturally appears as a result of quantization of the (classical) Drinfeld-Sokolov reduction [14]. Namely, W(g) is realized as the cohomology of a BRST complex involving the universal enveloping algebra U (g) of the affine algebra g associated to g and the ghosts associated to the currents of a maximal nilpotent subalgebra ft of g. For (classical) simply laced algebras this construction gives the same result as in [16, 17]. This approach allows one not only to define the ff-algebras, but also to construct a functor F from the category of positive energy representations of the affine algebra g to the category of positive energy representations of the algebra W(Q). Namely, the W(g)-modu\e corresponding to a g-module M is the cohomology of a BRST complex associated to M. The most important representations of affine algebras to which we apply this functor are the admissible (conjecturally = all modular invariant) representations of g of fractional levels k, discovered and classified in [26-28] by two of the authors of the present paper. In the particular case g = sT2 all modular invariant representations of level different from - 2 have level k = — 2 + p/p' [26], and it was shown in [6, 19] that the functor F sends these representations either to zero or to the irreducible representations of the Virasoro algebra from the (p, p')-minimal model [3]. This makes us to believe that F sends a modular invariant representation of an arbitrary affine algebra g either to zero or to an irreducible "minimal" representation of W(g). This irreducibility is our basic conjecture. We use the functor F to evaluate the characters of the W(g)-modules thus obtained as residues of affine characters. Our results completely agree with the results and conjectures of [7,9, 16]. The fact that the characters of the minimal series of the Virasoro algebra are residues of affine sT2-characters wasfirstobserved in [32]. The functor F gives a simple explanation of this phenomenon. Our calculations give much information about the conformal field theory with W(g)-symmetry which as yet has not beenrigorouslydefined. In particular, we can apply the Verlinde formula [35] to the modular transformation of W(g)-characters (found in [17,28]) to describe the fusion algebra of the (conjectured) minimal W(g)-models (in the simply-laced case). It is interesting that if we apply Verlinde's argument to the affine characters at a fractional level, then the fusion coefficients may be negative. However, the functor F corrects the situation. It sends some different g-modules to the same W(Q)modules and "erases" some of the g-modules, so that the resulting fusion coeffi cients for the ff-algebra are positive integers. Note that the characters of W(g)-modules computed by means of the quantum Drinfeld-Sokolov reduction coincide with those of the gi ® g*'/9i+*- coset model in the case of a simply-laced g. The connection between the quantum Drinfeld-Sokolov reduction and the coset models still remains a mystery. Below we describe the contents of the paper. In Sects. 1.1 and 1.2 we recall the necessary information about an affine Kac-Moody algebra g, its affine Weyl group W and especially the "enlarged" affine Weyl group W = W+ x W, where W+ is a group of symmetries of the Dynkin diagram of g isomorphic to the center of the simply connected group corresponding to g. In Sects. 1.3-1.5 we recall the defini tion and properties of the principal admissible weights Pr* [26, 27]. Here k stands for the level; it has the form k = — h v -I- p/p', where h v is the dual Coxeter number and p, p' are relatively prime positive integers such that p ^ h v . We also recall [27] the definition of the subset N*_ of " — "-nondegenerate weights, and the map
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/,., = (P'+-*,xP?''-*)/tf\. where P + (respectively PJ m ) is the set of dominant integral weights (resp. coweights) for g of level m. The map
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1. Principal Admissible Highest Weight Representations of Affine Algebras /./. Preliminaries on g. Let g be a simple finite-dimensional Lie algebra over C of rank t. Choose a Cartan subalgebra h of g and let A v e r) and A c h* be the sets of coroots and roots respectively. Let Q v c r) be the^coroot lattice and let 2 * c 5 be the dual to the root lattice. One knows that Q* => Q v and that the group Q*/Q v is isomorphic to the center of the simply connected Lie group correspond ing to g. Choose a subset of positive roots A + c A and let A I be the corresponding subset of positive coroots in J v ._Let g = r i - © 5 ©n+_be the corresponding triangular decomposition of g. Let /7 = {a 1 ; . . . , a,} and /7 v = {a, v , . . . , a / } be the sets of simple roots and simple coroots respectively. Let — a 0 = Yfi=i a '*> e ^+ and — dto = YJi= i ai *? e ^+ be the highest root and the corresponding coroot respectively, and let a0 = a© = 1- The numbers t
h=
YJ
t a
i
an
d
hv = Y, ai
i=0
i=0
are called the Coxeter number and the dual Coxeter number respectively. Let J be a jubset of the set {0, 1,. . . , t} consisting of those i for which a, = 1. One has: \QVQV\_=\J\Let ^ e h * (resp. A? eh), i = 1, „ . , /, be the fundamental weights (resp. coweights), i.e. (A,, a / > = 50- (resp.
foraeJ,
(1.1.1)
i= 0,...y.
(1.1.2)
It follows that (/ljlaj) = a?/a((i = 1, . . . , /), hence A^e Q* if i e J. Thus, we have {A~i)i*j is a set of representatives of Q* mod Q v .
(1.1.3)
All possible values of the ratio a,/afv are 1 if g is of type A(, D{ or E{, 1 and 2 if g is of type Be, C( or F 4 , and 1 and 3 if g is of type G 2 . We let r v = ma.xi(ai/a>'). The case r v = 1 (resp. r v > 1) is called simply-laced (resp. non-simply-laced). Let W a GL(rj) be the Weyl group of g. We denote by W+ the subgroup of elements of W that map the set {a0,_oci, .. . .a,} into itself. Notethat the set {a 0 ,. . . ,a,}\{a,} is a root basis of A if and only if jeJ. Since W acts simply transitively on root bases, we conclude that for each je J there exists a unique Wj g W+ such that a, = w,<x0, and that W+ = {wj}j€j . Proposition 1.1. e(w,) = ( -
(1.1.4)
\fW'\
Proof. Let a = £ , m,<Xi e A +. Then, for j e J we have: either m, = 0, then wj~'a e J + or rrij = 1, then wj"'ae — J + . Hence we have: | w ; ' A + n - A +1 = Y (al/Tj) = 2(^1^).
□
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299
1.2. Affine Algebra g and the Groups W and W (see [24] for details). Let g =
[K, g ] = 0 ,
(1.2.1)
m
where a, b e g, m, n e Z and aim) stands for t ® a. Let h = j) +
(1.2.2)
v
It turns out that A = W(77 ) is invariant with respect to a larger group W:= tpxiW, which will play an important role in our considerations. Let W+ = {w e W\ w(77v) = 77 v } . Since W acts simply transitively on root bases, we have: W=fV+xW.
(1.2.3)
Using (1.1.3 and 4), the group W+ can be described explicitly as follows: ^ + = {wj}jej,
where
w} = t^Wj.
(1.2.4)
we have canonical isomorphisms W+ Z- W+ =* Q*/Qv ,
(1.2.5)
which are induced by the canonical homomorphism W-* f u s i n g (1.2.3) and the definition of W. Proposition 1.2. (see e.g. [25]). The group W+ is a unique normal subgroup of the group Aut 77 v that satisfies the following two properties: Aut77 v = Aut fivxW+
and W+~Q*/QV.
Let / l 0 e h * be defined by A0\!) = Q, (A0,K} weights (resp. coweights) by
□
= 1. Define the fundamental
A, = At + a? A0 (resp. /l, v = A? + atA0),
i = 0, . . . , i .
One has wj(ag) = « / A
Let p = Yfi=o hP
v
and Wj(A0) = A} = AJ
if j e J .
(1.2.6)
v Then
=H=o^i (p,K)
= hv,
(p\K) = h.
(1.2.7)
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Let P = Xi^^i and P v = £,2/1^ be the sets of integral weights and coweights andletP + = £,Z + /ljand PI = £ l Z + /4iv be the sets of dominant integral weights and coweights. Let P \ P + etc. be the subsets of level k weights. Note that the bilinear form (.|.) on h is W-invariant, but there is no non-trivial Pf-invariant bilinear form on h*. The situation can befixed,however, as follows. One enlarges b by a one-dimensional space
(1.2.8)
We identify b* with the subspace of linear functions on f) which vanish on d. This subspace is not IP-invariant, as we can see from £a(A) = A+<>l,X>a-«>l,a>+i(a|a)
Aer}*,
(1.2.9)
where S is defined by <5|„ = 0, <M> = 1As the bilinear form (.|.) is non-degenerate on rj, it induces one on r>* which extends that on rj* by (r)*|
(1.2.10)
Let A" = A+ u {a + m5|a e A, n e N} be the set of positive real roots. 1.3. Principal Admissible Weights. Given A e h*, let RA = {a e A v re|
for all a e J r c ,
(1.3.1)
vre
(1.3.2)
1
K' is isomorphic to A
.
Note that all dominant integral weights are principal admissible. Recall the description of all principal admissible weights [27]. Let u € N and let RM = Av+ u {a + nuK\<x eAv,ne N}. One has (cf. (1.2.6)): tuA.WjRiu] <= RM for jeJ.
(1.3.3)
Given y e W, denote by PMi,, the set of all principal admissible A such that R\ = y(RM), and by Pj,,, the subset of Puy of weights of level k. Denote by Prk the set of all principal admissible weights of level k. A rational number k with the denominator u e N is called principal admissible if U(/C + / I V ) ^ / I V
Letting
and ( u , r v ) = l .
p = ii(fc + fcv),
(1.3.4)
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301
conditions (1.3.4) can be rewritten as p,ueK,
p*h\
(p,u)=l,
(u,rv)=l.
(1.3.5)
Recall the shifted action of W: w. A = w(A + p) — p. Theorem 13 [27]. (a) Pj ,, is non-empty if and only if the following two conditions hold: k is a principal admissible number with the denominator u , y(Rw)cAX".
(1.3.6) (1.3.7)
(b) If(k, u, y) and (k, u, yi) are two triples satisfying (1.3.6) and (1.3.7) then the following statements are equivalent: (i) (ii) (iii) (iv)
P^,, and P*,„ have a non-empty intersection, Ply and Pki,yi coincide, y(RlU]) = yi(RM), >>! = yt^wjfor some j e J. (c) //(1.3.6) and (1.3.7) hold, then Pj,, = {>-.(/1 0 -(u-l)(* + /! v )/lo)|,4 0 eP? + *->-*"}.
(d) Pr* is nonempty if and only ifk is principal admissible. (e) Prk = \JyPl y, where u e N is the denominator of k and ye W satisfies (1.3.7). D Lemma 13. Let y = t^y. Then condition (1.3.7) is equivalent to each of the following two conditions: (y-lP\<*n^0
fori = l,...,r,
0^ -(jr^lajgu
(y-lP\«o)^u-
forallaeA+.
(1-3.8) (1.3.9)
Proof, is straightforward. Remarks 1.3. (a) We have a bijective map Av i-» A0 between Pj y and pU(k + k-)-h- d e f i n e d by A = y.(A°-(ul)(k + h )A0). (b) Note that k e Z+ is principal admissible and in this case, Pr* = P +. (c) If k is principal admissible, then kA0 e Pjl, i <= Prk. This is called the vacuum weight of Pr*. 7.-/. The Maps Transpose andf. In this section we consider some important maps on the set Pr11 of all principal admissible weights._The_firstmap isthe transpose A >-*'A defined in [28] as follows. Let RA = RA n Av, RA+ = RA n J J, and let W^ be the subgroup of Wgenerated by reflections in the elements ofR*. The group WA contains a unique element, denoted by wA, such that wAR\ = — R +. In particular, w°^1 X = - A J. Note that (wA)2 = 1. Define wA e Aut h by w» = - w»
if v e 5, w"(K) = X .
(1.4.1)
Then 'A is defined by M + p = wA(A + p).
(1.4.2)
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E. Frenkel, V. Kac and M. Wakimoto
In particular, one has: 'A = w°{A) UAeP+ .
(1.4.3)
Furthermore, we have: 'Pjjfj) = Pk,ty, where for y = t^y we let
(1.4.4)
Explicitly, for A = (tfiy).(A° - (« - 1)(* + >>vMo)e PS,, we have 'A = (t ./jO-CM 0 ) - (u - l)(/c + h" Mo) e P*,,,.
(1.4.5)
It is clear that the transpose is an involutive map of Pi* into itself which fixes the vacuum weight kA0. It will appear in the calculation of the fusion algebra. We turn now to the definition of the second map / : Pi* -* Pi*, which will link two quantum reductions considered in the next sections. For this we need the following lemma. Lemma 1.4. ([27], Lemma 3.4a). Given (IeQ*, there exists a unique yeQ" and a unique yeW such that (tfi+ayy)RM c A I". □ Given u e N, we first define a map y H* y' of W into itself. Let_y = tfy; by Lemma 1.4, there exists a unique yeQv and a unique y' e W such that (tll_r+uyy1)Rlu]^AVt.^clet
P' = P-r+uy,
/ = *,./•
Using (1.3.3), it is clear that if y is replaced by y^ = yt^Wj, then its image y' gets replaced by y\ = y't^Wj. It follows that the element y:=y'y-le
W
remains unchanged if y is replaced by^yt^Wj. Now, for A e Pi* there exists ye W such that A e Pku_y and we let/(/l) = y.A. Due to the above argument and Theorem 1.3,/is a well-defined bijective map on Prk, such that/(PS,,,) = Pku
(1.4.6)
Then, by definition, A':=f('A) = (tfy').('(A0) - (u - l)(fc + /i v M 0 ). We need to show that/('/I') = A. Applying the above argument Jo ft' and y' in place of P and y, there exists a unique / e 6 v and a unique y" s\V such that *,»?" KM <= J T", where /T = - /T - p v + uy'.
(1.4.7)
But P" = 0 + u(y' - y) (see (1.4.6)). Hence, comparing (1.4.7) with tfiyRM <= A V and using uniqueness in Lemma 1.4, we conclude that y" = y andft"= /?. Hence, f('A'):= (try").{A° - (u - 1)(* + /ivMo) = * proving (a).
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303
Noting that t_^.R M <= A +re if u ^ h, we have under the assumption that u ^ h: f(kA0) = t_r.(kA0) = kA0 - (k + hv)p\ proving (b). D /.5. 77ie Maps (p * and f/ze Corresponding Sets of Non-Degenerate Weights Nk±. The proof of the following lemma is straightforward (cf. Lemma 1.3): Lemma 13. Let A be a principal admissible weight, A e P|jf y, where y = tfy. Then the following conditions are equivalent: <4<x>#Z forall<xeAv y(Rlu]) C Al\Al (y-lP\*n<0
fori = \,...J;
0 < -(y~lP\a)
,
(1.5.1)
,
(1.5.2) (y~iP\^)
foralltxeA+,
(j?|a)#0modu / o r a H a e J .
(1.5.3) (1.5.4)
D
(1.5.5)
In particular, all elements of Pk y either satisfy (1.5.1-5) or all do not. Given ye W, let Mu,9 = {fie 6*|0 < - (y'lP\<x) < u for all a e A + } , p* =
M
p* .
Nl = \J P 9k ye * •
(Elements of the last set are called non-degenerate weights in [28]). Each set P* admits the following nice parametrisation: Proposition 1.5.1. [28] (a) Let AePk. Then there exists a unique /J(e M M ) such that A e Pj, ,t9. We let 99-(A)
=
(A°,uA0-y-HP)-pv)-
This is a bijective map (here, as before, p = u(k + h v )):
,
the converse map being iJ,f(X,n) = y.X-?-y{H + p*) + ?-A0. u u In particular, P* + 0 if and only if k is principal admissible and u^h
.
(1.5.6)
(b) Let k satisfy (1.5.6) and let y,yt e W. Then \f/9 (X, n) = ^~ (A,, fi^jfarid only ify~l9i. — wjfor some jeJ and p~ (X — Wj.Xi) = u~1(n — Wj.^i) = Aj. (c) Pk9_and P*, are either disjoint or coincide and they coincide if and only if 1 y~ y1eW+. □
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Given relatively prime integers p^hv
ip,p. =
and p' ^ h, consider the set
{p\-k*xpy-h)iw+
(where w(A, p) = (wk, wfi), w e W+). Let
It is easy to see, using Proposition 1.5.1b, that the map q>~ is well defined. As we shall see, the map
for all a e A.
(1.5.7)
k
(b) The map cp is defined on A e P*,^ <= N + as follows. By Lemma 1.4, there exists a unique y' eWand a unique yeM such that tp_r + uyy'Rlu] c AX". Then cp + (A) = (A°,uA0 - y'~l(p - p" + uy) - p v ) m o d W+ .
(1.5.8)
Equivalently, the weight uA0 — y~1(P — pv) is cointegral regular, hence there exists a unique wfyeW and a unique pePl"~h such that p. + p v l = w(uA0 - y~ (P - p-")); then cp+(A) = (A°,n)mod W+. (c) / /
l)(fc + hv)A0)e
wy(RM) a A\\J+
Nk-, where y = tfye W. Then, due to for any we
W.
Hence by Theorem 1.3 and Lemma 1.5, (wy). (A - (u - l)(k + h v )A0) e Nl . But wy = tifi(wy), hence by definition of
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Here is a somewhat different description of the maps
The map
=* Pr",
where fV+ acts on both factors as defined in 1.2. Let now A = tf>(i, 0) e Pr", where (A, 0) e ( P V *" x (C*/wQ v )) mod W+. Then A e TV + if and only if (i — p v is regular with respect to the group Wx uM. In this case we have: cp + (A) = (k, (u - AMo + fi) mod W>+ , l
w
where / i e P + ''~' is such that p + p Furthermore, we have:
v
and P — p
a(A) =
(1.5.9) v
lie on the same JFxuQ -orbit.
+ 2p").
(1-5.10)
/.6. Characters and Normalized Characters of an Affine Algebra. Let Af be a gmodule. It is called a level k module if K = kIM. It is called a restricted module if for any x e g and any t> e Af there exists n 0 such that x(n)v = 0 for n > n0. If M is a restricted g-module of level k 4= — hv one defines the Su^awara operators on Af by
where {HJ} and {«'} are bases of g such that (M;\ui) = <5y. Recall that these operators define a representation of the Virasoro algebra with central charge kjdim g) (L62) C =
* TT^-
A restricted g-module Af of level k +" — h v is called a positive energy module if S 0 is a diagonalizable operator on Af with a discrete spectrum bounded below and each eigenspace of S0 is a g-module from the category <S. (Recall that a g-module is said to be in the category 6 if it is finitely generated ^-diagonalizable and n+-finite.) The most important examples of positive energy g-modules are irreducible highest weight modules L(A), where A eh* is of level k 4= — hv, defined by the property that there exists a non-zero vector vA such that [24] ("+ \
+
Z t * g ) ^ = 0, hvA = (A,h}vA k>o
for he h .
/
Let q = e2*", where T e ^f+, the upper half-plane. Consider the domain Y = Jf+ x fj x
(t,
x,t)eY.
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E. Frenkel, V. Kac and M. Wakimoto
This series converges to a holomorphic function in the following domain in Y [24, Chap. 11]: Im(x|a) > 0 for a e J +
and
Im(<Xo |x) < I m t ,
(1.6.3)
and can be analytically extended to a meromorphic function in Y analytic outside the hyperplanes (x\a) = n for a e J + , n e Z . If AePk+, then XA converges to a holomorphic function on the whole domain Y [24, Chap. 10]. Given A e h* of level k one defines the normalized character %A of the g-module L(A) by the formula: XA(T,x,t)
q-°'l2*chL(A)tz,x,t).
=
We shall identify Y with a domain in i) by letting (T,
x, t) = 2ni( - xd + x + tK) .
In the case A e P* ,lf, the meromorphic function %A(i, x, t) in Y is given by the following formula [27, 28]: ,
A
X t) =
AA, + P(m, xy~l(P) + y~lM,u-l(t
*^ '
+ (x\p) +
JT|/?|2))
A^U)
.....
•
(L6 4)
-
Here, for X e P +, s € IN, we let Ax = qw'l2s
X £(w)ewU>. weW
Recall the following simple (but useful) identity for A £ P + and \i £ h* such that
(
I-|2\
^ identity: "T/Z'TW= Recall also Macdonald's
sm|w(A)
»il2
^ £(W)9
'
(1 6-5)
'
Recall also Macdonald's identity:
7.7. Modular Transformations of Normalized Characters. The most interesting from the conformal field theory point of view are the modular invariant representa tions, which are defined as follows. Recall the action of the group SL 2 (Z) on Y: a b\ , (ax + b x c{x\x) s 1 ( t , x , t ) = — , — — : , ( c dj ' \CT 4d' ex + d' 2(CT + d)J ' x and its right action on functions on Y: f(x,x,t)\B=f(B-(x,x,t)),
BsSL2(Z).
The representation L(A) is called modular invariant if XA is invariant with respect to a congruence subgroup of SL2(2). It was proved in [26] that L{A) is modular invariant if A is admissible, i.e. (1.3.1) holds, and <5}RA = Q^dvre (it was also conjectured there that there is no other modular invariant L(A) of level + — hv). According to the classification of
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Fusion Rules for W-Algebras
admissible A given in [27], they can be described in terms of the principal admissible weights (in the type A case all admissible weights are principal admis sible). The normalized characters of the principal admissible representations have remarkable transformation properties. Let
«-C-i)'-(iOTheorem 1.7. ([27, Theorem 3.6]). Let A e Pj,,,, where y = tfiy. Then XA\S =
2^
SAXX* >
A'ePr*
where SAA. = iiJ-iM-'(fc + / i v ) - ' / 2 | M * / M | - 1 / 2 £ ( ^ ' ) xe-2*nu°
WE
(Here A' ePlt?,y' ant. D
e(w)e~^r^lwiA
+ P\tr)-n*° + P\i>) + (i< + i<-mr)) y
+P)
If
= tpy'.) In particular the space Y^AZP^^XA
Recall also that the matrix (SAA)AAeP^ Proposition 4.3]).
+P)M
is SL2(Z)-invari-
is a unitary symmetric matrix ([28,
1.8. The Residue of Affine Characters. Let F(x, X, t) be a meromorphic function on Y. Define the residue of F by the following formula: Resx=0F(T,
X, t) = lim F(r, ex, t) f ]
0 -
e
~~ 2 K ' < "" ) ) •
This is a meromorphic function in (T, t) e Jt?+ x
«»*.„(*) = * ( * ) " ' £ e ( w ) q l
/i + p"! 2
P
P' I ,
weW
where >/(T) = q1/24I~[i.eN(l — ") is the Dedekind ^-function. This is a holomorphic function in T e ^f+ . Proposition 1.8. Let A e P*,,y be a principal admissible weight. (a) There are two possibilities: (i) A $ N*_; in this case ResJt=0(X/i(T» *> 0) = 0; (ii) A e TV _; in this case we let (A, p) =
-P)).
. (1.7.1)
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E. Frenkel, V. Kac and M. Wakimoto
Then: ,ai«*-/ ( T ) ( _ i)'M + w>Hi.i R e S x = o X / ) ( T ) _%r
+x,t|p v | 2 /2) = ^. | 1 (t).
Proo/ We use the explicit formula (1.6.4) for XA and identities (1.6.6) and (1.6.5). Since (a) was proved in [28, Proposition 4.2], we check here (b). The proof of (i) of (b) is the same as that of (a). In the case (ii) of (b) we have, using (1.6.4) and (1.6.6): Res^oLtfo - * p v +x,t|p v | 2 /2) = ^,("T,Tr^-pV'^
v | 2
) ( - i)IJ-'
i |,/2 <w > i+ , i« /»v""' " n. .(i-9")'n. i.(n«.(i-«"" * ")n-Si o 9 s e Using (1.6.5), and the formulas
n(i-
-«"")
n +a
= (_ iy-iq-^-Di2
Yl {\-q»)\
aeN,
|p|2/2/iv = dim g/24 ("strange formula"), £
v
(1.8.2) (1.8.3)
/zta = 2(p|p ),
£ (taz) 2 =
(1.8.1)
fcvIPvl2,
IE J .
(1.8.4)
the previous formula gives the result. Note that (1.8.4) follows from X (x\*)(y\aL) = h"(x\y\
□
IE J*
(1.8.5)
2. Two Quantum Reductions 2.1. Two Classical Drinfeld-Sokolov Reductions. Let g = ii- © rj ©n+ be the tri angular decomposition of the Lie algebra g. Choose bases of n+ (resp. n_) consisting of root vectors {e„} (resp. {«-«}), a e A + , such that (e„\e-a) = 1. Con sider the following two subalgebras of the affine algebra g: n± = C [ t , r 1 ] ® n ± . Vectorsex(m)(resp. e-„(m)), otel+.meZ,form a basis of n+ (resp. n_)and we let e„ (m)* (resp. e - „ (m)*) be the dual basis of the space n X (resp. n *) of linear functions on n+ (resp. n_) which vanish on all but finitely many vectors of the basis. Using the bilinear form (.|.) on g we may identify n^ with nT so that e±„(m)* gets identified with ef
06/7
Note that p+ (resp. p_) is a character of n+ (resp. n_).
(2.1.1)
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Fusion Rules for W-Algebras
309
Let n± be the restriction map from the dual of 9 to the dual of n ± . Denote by &± (g) the algebra of local functionals on % ±l (p ±) invariant under n ± . These two algebras have canonical structures of Poisson algebras induced from the canonical Poisson structure on the dual of g. These Poisson algebras are called the classical W-algebras. Drinfeld and Sokolov used them to write equations of KdV type as Hamiltonian systems [14]. For example, &±(slH) is the Gelfand-Dikii algebra, which can be identified with the Poisson algebra of local functionals on the space of differential operators of the form d" + a2(x)dn~2 + . . . + an(x) on the circle. According to [30], the Poisson algebra JF± (g) can be obtained as the cohomo logy of the complex which is the "local completion" of (
Z el/®
a
where a, /?, y are roots of n ± . Indeed, the space OF± of functions on nli(p±) can be identified with the 0th cohomology of the Koszul complex C[g*] ® ^(n ± ) with respect to the differential <*i = 2>a® {>?,•} + I P(ea)®{q>*,-} . a
a
The space of n±-invariant functionals on nll(p±) is the 0th cohomology of the standard cohomology complex &± ® A*(n\) of the Lie algebra n ± . The differen tial of this complex is equal to d
2 = Z {*„ • } ®
C
2.0®{
*• a, 0,y
«
Therefore, the space ^±(g) is the 0th cohomology of the double complex £[9*] <8)A(n± © n\) with respect to the differential d^ + d2 = d. Remark 2.1. This construction can be generalized as follows. Let ft t be an ideal in ft = ft+, and p e n * be such that its stabilizer in n is ftj. Let n = C [(, t~i ] ® ft, n! = C [t, t ~*] ® fii. Let us define a linear functional p e n* by p(x(n)) = <5„, -ip(x), so that p restricted to nj defines its one-dimensional repres entation Cp. Let N and TV*! be Lie groups corresponding to Lie algebras n and n t . We can apply Jthe Hamiltonian^ reduction to the orbit Op of p e n*, which is isomorphic to N = N/N^. Here N is a Lie group, because TV 1 is a normal subgroup of N. The Poisson algebra of local functionals on the reduced Hamiltonian space n~i(@p)/N coincides then with the 0th cohomology of the local completion of the complex C[g*]®/l*(n©n*)®C[0p], with respect to the differential da = < ^e.®^*-l a
Z cl,®ipr
)
1 + Z 1 ® {«»?.•} ®e*x
Here C [0 P ] is the space of polynomial functions on 0P, and the Lie algebra n acts on it as on the coinduced module Homt/(ni)((/(n), Cp). If n! = n and p = p+, then
415
310
E. Frenkel, V. Kac and M. Wakimoto
Op = p+ and we have the Drinfeld-Sokolov reduction. Some other cases were considered in [29, 33, and 12]. 2.2. Quantization of Drinfeld-Sokolov Reductions. As usual, the quantization pro cedure consists of replacing the Poisson algebra SC(Q*) by the corresponding universal enveloping algebra and the Grassmann algebra by the Clifford algebra. This is explained below. We shall view the space a 1 ± : = n ± © n , £ ( = n + © n - ) a s a n odd commutative Lie superalgebra with the bilinear form (.|.) restricted from g. We define a Lie superalgebra 6 ± to be the orthogonal direct sum of the even Lie superalgebra o ± : = 9 with the bilinear form (. |.) and the odd Lie superalgebra a' with the bilinear form (.|.). (Of course, the superalgebras o+ and 5_ are naturally isomorphia) We consider the central extension a± = C r j , r 1 ] ( g > a ± © C K © C A : ' of the loop super-algebra €[*, t~'] ® a ± by letting the even and odd part com mute, the bracket on the even part given by (1.2.1) and on the odd part by la(m),b(n)-\ = dmt.n(a\b)K',
(2.2.1) m
where a,bea±,m, neZ and, as before, a(m) stands for t (&a. Its even part o°± = 9 ©
(2.2.2)
Given IteC, let Uk{a±) = U'(a±)/(K — k) with the induced Z-gradation (in other words, we fix the value of the affine central charge to be equal k). Let z be an indeterminate. For an element a e g + ft ± (resp. e ft|) of a ± we let Aa = 1 (resp. = 0), and define the elementary field a(z) of conformal dimension Aa as the series a(z)= £
a(m)z-m~A-.
meZ
Arbitrary fields are obtained from these by taking derivatives in z and normally ordered products a finite number of times. (Recall that one defines the derivative d 3/4(z) of a field A(z) of conformal dimension A to be the field — A(z) of conformal dz dimension A + 1, and the normally ordered product of fields A(z) and Ai(z) of conformal dimensions A and A t to be the field
416
Fusion Rules for FP-Algebras
311
of conformal dimension A + A x. Here, as usual, A.(z)=
£
A{n)z--A,
A + (*)= Z
A(n)z —
\
n> - A
» S - J
and the sign + (resp. —) is taken if at most one (resp. both) of the fields is odd.) Let Uk(a±)loc denote the C-span of the coefficients of all fields (in a certain completion of Uk(a±)). It is well-known that it is closed under the Lie (super) bracket. Also, it inherits Z-gradation (2.2.2) from Uk(a±). ([4(a ± ) loc consists of the series whose symbols are local functionals on a* [20]. One also knows that the associative envelope of Uk(a±)toc is its universal enveloping algebra [20].) Denote by
Z_ cl,,
where [_ea, e„~] = Zyc«/>er Let d„ e Uk(a±)loc be the coefficient of z 'in d„ (z). It is easy to check that the singular part of the OPE d£(z)d5(w) is 0 (see Sect. 3.1 for a digression on OPE). Hence^if) 2 = 0. The operator d,t (resp. d,7) is the standard differential of n+ (resp. n_)-cohomology. We let as before
p+ = Z ??(i), p- = Z
ueUk(a±)loe,
equipes the Z-graded Lie super-algebra l/*(a±)loc with the structure of a differential graded Lie superalgebra. The corresponding cohomology is again a Lie superalgebra. Note that the complexes (Uk(a+)loc,D+) and (Uk(a-)loe,D-) are naturally isomorphic. Indeed, let w° be the involutive automorphism of g that maps ft+ to n_ and induces the element w° e W, and consider the element w = w°t _ r . We have: w(/lo) = ^o + P v - i l p v | 2 < 5 ,
(2.2.3)
w(a) = - 'a + (hta)5 if a e A, where 'a = - w°(a),
(2.2.4)
w(x) = w°(x) + (p v \x)K
(2.2.5)
ifxefj,
w(e„{n)) = e-,a{n + htct), w((p„(n)) = ><«(" + /««), *(??(«)) =
(2.2.6)
417
312
E. Frenkel, V. Kac and M Wakimoto
Using these formulas, we see that w maps p+ to p _ , n ± to n T and induces an isomorphism of l/*(a + ) and l/ t (a_) which maps d+ to d-. Hence the cohomology of complexes (l/*( a + )ioc, D+) and (Uk(a _),„,., D_) are isomorphic. It was conjectured in [20] (and proved in [23] for generic k) that the i'h cohomology of these complexes vanishes if i =f= 0. The 0th cohomology is a Lie algebra which is called the W-algebra associated to g and is denoted by W* (g). This is a natural quantization of the classical W-algebra. Namely, it was shown in [23] that Wf (g) is a quantum deformation of the classical W-algebra. Its proper ties are described in Sect. 3.3. 2.3. The Functors F'±. Let A± be the module of semi-infinite forms over the algebra W(a' ± ), i.e. the irreducible module with the cyclic vector v± satisfying the following conditions (a e A +): (p*(m)v- = 0 if m ^ 0,
(pa(m)v- = 0 if m > 0 ,
<pa(m)u+ = 0 if m ^ 0 .
Letting deg v± = 0, A± inherits Z-gradation from <#y(aT±) (given by (2.2.2)): /1± = I
A\ .
(2.3.1)
me Z
Given a restricted g-module M, let C±(M) = M®A±
= X CJ±(M),
where
C J ± (M) = M ® / 1 J ± .
;eZ
The Lie superalgebra t/»(a±)|OC acts on C±(M). In particular, the element d± acts on C ± (Af) shifting the Z-degree by 1. Let / / ± (M) = 0 ) E z # 4 (M) be the cohomol ogy of the complex (C±(M),d±). The representation of t/ k (a ± ) loc on C ± (M) induces a representation of the Lie algebra W* (g) on each space H^ (M). Thus, we get functors, which we denote by FJ±, from the category of positive energy g-modules to the category of W£(g)-modules, that send M to HJ±(M). In order to prove a vanishing theorem, we need the following standard lemma. Lemma 2.3. Let (C, d) be a complex, i.e. d(CJ) a Cj+1 and d2 = 0. Let 3: C -> C be such that 3(CJ) c C'~' and dd + 3d = A is an invertible operator on C. Then the cohomology of the complex (C, d) is zero. Proof. First, note that dA = dbd = Ad. Given coeC such that dco = 0, let
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Fusion Rules for ^-Algebras
313
Remark 2.3. We can also quantize the generalized Drinfeld-Sokolov reduction, described in Remark 2.1. The quantum BRST complex tfien is t/t(5)ioc> where 5 = (g 0 nfe © (n © n*)j where ft = n/tti. The differential D is the supercommutator with du, and the action of n on 14(5) is twisted by p. Let us denote the 0lh cohomology of this algebra by W^(g, n 1( p). We also have functors from the category of positive-energy modules over g to the category of Wk(Q, nlt p)-modules, sending a g-module M to HJ(n, M
d2p"(z)+Tsh(z),
where S(z) is the Sugawara field (cf. Sect. 1.6):
and T#[z) is the ghost field: T*(z) = X (htoi: dq>a{z)cp*{z): + (1 - htct): d
(3.1.1)
In order to avoid lengthy calculations, we use some well known field-theoretic techniques that we now recall. Given two fields A(z) and Av(z) of conformal dimensions A and A t, we may write their operator product expansion (OPE): A(z)A1(w)=
X a
Cj(w)(z-Wy,
-A-A,
where Cj{z) are somefields.The sum of terms with ;' < 0, the singular part of the OPE, determines the (super) bracket of Fourier coefficients. One says thatfieldsdo not interact if the singular part of the OPE is 0 (in this case the Fourier coefficients (super) commute). The regular part of the OPE is unimportant for calculation of (super) commutators and is usually dropped. One calls a field t(z) of conformal dimension 2 an energy-momentumfieldwith central charge c if t(z)t(w) = , ,4 + , \2 + — — , where ceC. (z — w) (z — w) z — w This OPE is equivalent to the property that t(z) = £ n e l tHz~"~2 and the t„ obey the commutation relations of the Virasoro algebra with central charge c.
419
314
E. Frenkel, V. Kac and M. Wakimoto
A field A(z) is called primary of conformal dimension A with respect to t(z) if ..At^ AA(w) dA(w) t(z)A(w) = ^ + —!-i. (z — w) z—w In order to prove (3.1.1) we use the following simple lemma. Lemma 3.1.1. If A(z) = X n ^ n Z " ' is a primary field of conformal dimension 1 with respect to an energy-momentum field t(z), then [r(z), A0~\ = 0 . □ Let us recall some of the OPE's: Lemma 3.1.2. (a) S(z) is an energy-momentum field with central charge ck (given by (1.6.2)). (b) The field T%,":= X: d
- 12A2 + 1 2 A - 2 .
(c) Elementary fields a(z), a e g, are primary with respect to S(z) of conformal dimension 1. (d) Elementary fields (p„(z) and (p*(z) are primary with respect to Tgi," of con formal dimension X and 1 — X respectively. (e) One has the following OPE between elementary fields: a(z)b(w) = z—w
+ -j, (z — w)z
(p„(z)
a,beq,
□
The following lemma is immediate by Lemma 3.1.2, using the usual Wick formula for free fermionic fields. Lemma 3.13. (a) T+(z) is an energy-momentum field with central charge c(k) = ck-
12fc|pv | 2 - 2 X (6(hta)2 - 6ht<x + 1),
(3.1.2)
cte J .
where ck is given by (1.6.2). (b) The field d+(z) = d£(z) + X06/j
2
+ 24(P\PV)-
U(k + h")\pv\2-
(3-1.3)
We have the following explicit formula for L$: U = S 0 - p v +L 0 + , g h ,
(3.1.4)
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Fusion Rules for W-Algebras
315
where L
o,gh= Z ( Z (m-hta)(pa(-m)(p*(m)+
£ (m + faa)(p*( - m)q>M)) m£0
aei. \m>0
= z (zo(ro<5 -
/
a\A0 + pv)
ate J+ \ m > '
+ Z M + «Mo + PW)
(3.1.5)
Applying the automorphism vv (see formulas (2.2.3H22.6)) we get a formula for LE = w(L0+): i o = So - i ( * + /»V)IPV I2 + ( p l p v ) + W
>
(3.1.6)
where ^o,«h= Z_ ( Z CEEJ.
m(
P'( ~m)(p*(m) + Z "»«»?( - m)(pa(m) j .
Xn^O
m > 0
(3.1.7)
/
(In this calculation we use (1.8.3 and 4) along with the formula Q So
-2(k +
hn~Ao'
where Q is the affine Casimir [24, Chapter 2].) 3.2. A Calculation of the Euler Character of the Wf-Module H±(M). Define the Euler character of a direct sum of W* (g)-modules V = @JeZ Vj by the formula chr=£(-l)>tr,,y*. In this definition we assume that ch V converges, by which we mean that L$ is diagonalizable on V withfinite-dimensionaleigenspaces. Let now M be a positive energy g-module. By trie Euler-Poincare principle we have: chtf ± (M) = chC ± (M) if the right-hand side converges. Unfortunately, it does not converge. To get around this difficulty, introduce a Z2-gradation of C±(M) in such a way that degds* = (1,0) and degp ± = (0,1). It follows that the cohomology of the complex (C±(M),d±) may be calculated as follows. First, we calculate the co homology E±(M) of the complex (C±(M),d„). Then we consider the spectral sequence (£±(Af)U), (*•>), j ' ^ 1, where £±(M)(1) = £±(M) and d(1) = p±. This spectral sequence converges, which is ensured by the following facts. The complex C±(M) decomposes into a direct sum of subcomplexes C±(M)X which are Xeigenspaces of Lfi . Furthermore, C±{M)X = (Bi+j=PC'iJ(M)x, where j is bounded from above for any k and p. Thus we have: H±(M)=
lim E±(M)U). ]-<X>
In order to proceed, we need the following
(3.2.1)
421
E. Frenkel, V. Kac and M. Wakimoto
316 Lemma 3.2. For x e b, let
x(z) = x(z) + X (*l«):
(3-2.2)
cte J .
77ien
(a) [
-j— .
(z - w) 2
Froo/ One checks (a) directly, using Wick's theorem and the fact that clfi 4= 0 only, if y = a + /?, that the singular part of the OPE d£ (z)Jc(w) is zero, (b) follows from (1.8.5). □ By Lemma 3.2b, the Fourier coefficients of the fields x(z), x e rj, form an oscillator algebra of level k + h", which we denote by T(g). By Lemma 3.2a, T(g) acts on E+(M). Proposition 3.2.1 [20]. The action of the W-algebra WJ[(Q) on £ + (M) can be expressed via the action o/U(r(g)) l o c . In particular, one has
where ut is an orthonormal basis of%.
□
Fix now x e 5 such that (a|x) < 0 in the " + " case (resp. > 0 in the " — " case) for all a. e 77, and fix e > 0. Then all eigenspaces of the operator L$ + ex in C + (M), (resp. LQ + ew(x)) are finite-dimensional. Here
x = x+ £
£ (x\a):
is the coefficient of z" 1 of x(z). Thus, by the Euler-Poincare principle we have a rigorous formula: I
( - l)'trcAM,9tt + rf = I ( - l) J tr £AM) g L ° + <*.
jeZ
(3.2.3+)
;EZ
Letting = — S0 we extend any positive energy g-module M to an rj-module (cf. Sect. 1.2) which decomposes into a direct sum of finite-dimensional weight spaces: M = ®x€p(M)Mx, where P{M) <= 5* is the set of weights of M (note that weight spaces with respect to b and to S0 may be infinite-dimensional). A weight p e P(M) is called maximal if (p\pv) is maximal. Fixing a maximal weight p., we may define the height of Ae P(M) by ht^k) = (p - X\pv)eZ + . Recall that the oscillator algebra T(g) acts on £+(Af), the semi-infinite cohomology of n+, with coefficients in M. Since k + hv 4= 0, it follows from repres entation theory of oscillator algebras [24, Chap. 9], that for each p. e h* of level k there exists a unique irreducible T(g)-module 7t„ which admits a non-zero vector Vp (vacuum vector) such that xintfVft = 0 for m > 0 and
x(0)i>„ = p{x)vll for x e rj,
and that E+ (M) viewed as a T(g)-module decomposes into a direct sum of modules n„. Using the formula for T(z) given by Proposition 3.2.1, we obtain
tr.q* = qrwf[
(1-«")-',
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Fusion Rules for W-Algebras
317
where I/J + P l 2 - I p l 2 yh 2(k + hv) ^ ' In particular, all eigenspaces of LQ in n^ are finite-dimensional. Now we are in a position to prove the following important proposition. Proposition 322. For any positive energy Q-module M all eigenspaces of LQ on £ ± (M) are finite-dimensional. lw
Proof. We give the proof in the " + " case, the proof in the " — " case being similar. Let fx be a maximal weight of M. Denote by 0„ the category of positive energy modules M' such that all irreducible subquotients of M' are of the form L(w. ft), where we W, and ht^X)eZ+ if XeP(M'). We may assume using results of [13], that M is a module from the category 6„. We shall prove by induction on n the following: Claim (n): the multiplicity of nx in a g-module from the category 0M is finite if ht„{X) ^ n and it is non-zero only if X = w. fx. We shall repeatedly use the (obvious) fact that if ht„(X) > 0 for all maximal weights A of a g-module M' (in this case we write: P(M') < ii), then 7r„ does not occur in £+(Af'). Let B(n) be a Wakimoto module [18]; by its definition, E°+(B(ii)) = n„ and EJ+ (B(n)) = 0 if j 4= 0. We have an exact sequence: 0-»I/0I)->B(JI)->B(AI)-0,
where U(fi) is a quotient of M(fi) and P(B(LI)) < \i. From the long exact sequence for semi-infinite cohomology, we conclude that the multiplicity of nx in E+ (U(^)) is equal to that in E+(B((i)). Hence, Claim (0) holds for U(n) and, applying the inductive assumption for n to B(n), we derive Claim (n + 1) for U(LI). Thus, we have proved the claim for U(LI). The same argument applied to the exact sequence 0 - M(n) -> M(n) - U(fj) - 0 proves the claim for the Verma module M(n). Similarly we prove the claim for any quotient of M(//). Finally, let filt. . . , n„ be all maximal weights of M (with their multiplicities). Consider the exact sequence O-0,M(/ii)->M-M-O, where M(ni) are some quotients of Verma modules. Applying the above argument to this exact sequence we prove the claim for M. Proposition now follows since for any positive integer N there exists n such that P(w./z)>7Vif
(3.2.4+)
)eZ
Similarly, under the same assumption on M we have chtf _(M) = lim X ( - iytr c .i ( V ) ^ + «w». i|0
We can prove now
jeZ
(3.2.4.)
423
318
E. Frenkel, V. Kac and M. Wakimoto
Proposition 3.23. Let M be a positive energy q-module of level k. Then: (a) chH.(M) = ^(c(*»-Ck,>;(T)di,I,8-'Resx=ochM(T,x,0). (b) chfl + (Af) = ( - l) 2W '" ) + |J - l ^ (c(,I) - o -^(T) dimS - / Res x . 0 ch M (T ) -Tp v + x, v 2 t|p | /2). Proof. Using (3.1.5) and (3.1.7), it is straightforward to derive the following for mulas:
K - i y t r ^ 1 * " * * - " - fl (l-^--'*-»'«), £ ( - \)i\zAjqL~<> + + c*{i-x) = n Jel
(1 - qiA°-'*°MM) .
(3.2.5 + ) (3.2.5.)
«sit"
Since C±(Af) is a tensor product of M and A±, and since the operator LQ + ex (resp. LQ + ew(x)) acts on Af as S0 — p v + x (resp. S0 — i(/c +/i v )|p v |2 + (P~IPV) + ew(x)), and on /1+ (resp. /1_) as Lo,gh + e(x —x) (resp. as Lo.gj, + e*(x — X))J (a) aQ d (b) follow from (3.2.5 _) and (3.2.5 + ) respectively. □ Comparing Proposition 3.2.3 with Proposition 1.8 (and its proof), we obtain Theorem 3.2. Let A e P* tf9 be a principal admissible weight. (a) If A e Nk. and (p~(A) = (A, p), then q-'(k),2*chH-(L(A)) = ^ ( T ) . (b) IfAe Nk+, q>+ (A) = (A, /i) and w is rne element of W defined in Proposition 1.8b(ii), f/ien q-<wchH+(L(A))
= «(*)?*».
D
5.5. Some Properties of W-Algebras. In order to state some properties of JF-algebras define the Harish-Chandra homomorphism n: C/t(a±)loc-» l/(f>). For this note that (4(a ± ) loc is a direct sum of subspaces t/(t>) and n_ ^(ai.),^. + l/k(o±)locn+ + a± ^(Oi),,,,.. We let n be the projection on the first summand. Let dx = 2 < d2 ^ . . . < dt = h be the degrees of fundamental Winvariants in S(f)). It was shown in [21,23] that the W-algebra W»+(g) contains Fourier coef ficients of i fundamental fields W$(z) = T(z), WS2{z), ...,Wl (z), with the follow ing properties: (Wl) The Lie algebra W£ (g) is the linear span of the Fourier components of all fields obtained from the WJ (z) by taking finitely many times normally ordered products and derivatives. (W2) Wj{z) has conformal dimension;': »?(*) = I
W/(m)z--',
[^/(m),L 0 + ] = m ^ ; ( m ) .
mcZ
(W3) The highest degree terms of n(rVj(0)), j = dl,...,d(, generate the algebra of invariants S(rj)*. (W4) IWtiO), iVjm = Yi,,mCij(s,m)W;i(m1)lv;i(m2) ..., where m, g m2 We let WJ{m) = w-1(Wj(m)).
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Fusion Rules for W-Algebras
319
Proposition 33. (a) Let Pj(X) = n(WJ{Q))(X + p), A e Jj*. Then the polynomials Pj generate the algebra S(fj)*. (b) cy(s, 0) = Ofor all i, je {dt d(},s = (sl3s2, . ■ . )■ Proof. In view of (W3), in order to prove (a) it suffices to show that P} is W-invariant. Let rtbe the reflection with respect to<x((i = 1 , . . . , t\ Let n e N and let A be a generic element in the hyperplane = n in h* of level k. Consider the Wakimoto module B(X). Then we have either the exact sequence 0-L(A)-B(A)-L(r,.A)^0, or the same sequence with arrows reversed. Recall that H _ (L(A)) = 0 by Theorem 2.3. Note also that £ - (fl(A)) = H-(B(X)) and that Lfri.X) = M(rt.X) - B(r,.X). From the d_-cohomology long exact se quence we now obtain that H0-(L(rt. A)) — nx. Since the vector of maximal weight of the W± (g>module H _ (Hfi. X)) is v,t. x <8> f -, we deduce that «(WJ (0))(r,. A) = B( JK7 (0))(A) for all i. This completes the proof of (a). We prove (b) by induction i which we may assume to be ^ j . For i = 2, (b) follows from (W2). By Proposition 3.2.3a, the vector v"x = vx(&v- spans the eigenspace corresponding to the minimal eigenvalue of LZ in H° (M(A)). Since all W," (0) commute with LQ »we obtain that JfY (0)0^ = P,(X — p)vx for all A e h*. In particular, [Wf (0), ^ " ( 0 ) ] ^ = 0, hence (Xcy(s, 0) IF" (0) W- (0). . . )vx = 0
or aU A .
Since, by the inductive assumption all factors in the above sum commute (see (W4)), we deduce that c,j(s, 0) = 0. □ 3.4. Positive Energy Modules Over W-Algebras. A W* (<j)-module is called a posit ive energy module if L$ ( = W* (0)) is diagonalizable with finite-dimensional eigenspaces and has a real discrete spectrum bounded below. Note that by Proposi tion 3.2.2, FJ± are functors from the category of positive energy g-modules to the category of positive energy W* (g)-modules (see Sect. 2.3). Lemma 3.4. Let M (resp. M') be a quotient of a Verma module M(X) (resp. M(w.X) for some w e W) over g and let v (resp. v') denote its highest weight vector. Then the eigenspace corresponding to the minimal eigenvalue ofLo in F%(M) (resp. F°± (AT)) is \-dimensional and Wf (0)-invariant. Furthermore the eigenvalues of Wf (0) in these eigenspaces are equal. Proof. The first claim of the lemma is clear and the second one follows from Proposition 3.3a. □ Let now V be an irreducible positive energy W* (g>module. It is clear by Proposition 3.3b that the eigenspace of LQ corresponding to the minimal eigen value is 1-dimensional. The (-tuple of eigenvalues (cu...,c,) of ^ , ( 0 ) , . . . , ff£(0) in this space is called the highest weight of V. Clearly, it determines V uniquely; moreover, there exists a unique irreducible positive energy module over Wf (g) with a given highest weight.
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Conjecture 3.4-. Let AeNk be a non-degenerate principal admissible weight. Then (a) F°-(L(A)) is an irreducible W± (g)-module. (b) Fi(L(A)) = 0ifj*0. Conjecture 3.4 _ a together with Propositions 1.5.3 and 3.3a and Theorem 3.2a imply Proposition 3.4. (a) A and A' eNk- are such that q>~ (A) = q>~(A') if and only if Fl(L(A)) and F°.(L(A')) are equivalent W;{o)-modules. Thus, W;(Q)-modules obtained by applying the functor F l to the set of q-modules {L(A)\A eJV-} is parametrized by the set Ip „■ via the map (p~, where p' is the denominator of k and p = p'(k + h"). (b) Let A e Nk- and let (A, n) = q>~{A). Then: Remark 3.4. (a) Formulas (3.1.3) for k = — hv + p/p' can be rewritten as follows: c(k) = t -
™v
r PP
, where (p,p') = 1, p ^ h\p' ^ h ,
which in the simply laced case becomes (cf. [7, 9, 17]):
c(k) = A\ - W + WP - P')2\
w h e r e (p)
p')=i,p^h,p'^h.
(b) Let hXll denote the lowest eigenvalue of Lo in a W * (#)-module labeled by {X, (i) e 7pp.. Then hklk = ^« + c(fe), where hXl, is the exponent of the leading term of q>xn- Using this one easily derives the formula (cf. [9]): hx, = 2pp ~(\P'(* + P)~ P(H + Pv)l2 - \P'P ~ PPV\2) ■ (c) Let g be a simply laced simple Lie algebra of type different from At. Then for each s such that a, > 1 one has a family of non-principal admissible g-modules L(A) parameterized by a finite set of /l's which we denote by Pj. The set of all non-principal admissible g-modules is a union of these sets [27]. The sets Pk are explicitly described in [27, Theorem 2.3]. Here we only recall that P{ + 0 if and only if k + h = p/p', where p and p' are relatively prime positive integers such that p^max(M,...),
(3.4.1)
where h,h, . . . are Coxeter numbers of Lie algebras g, g, . . . whose Dynkin diagrams are connected components of the Dynkin diagram of g with the s,h node deleted. In some cases (described in [27]), (3.4.1) should be a strict inequality. Furthermore, consider the set of coroots
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Then all possible (A, n) =
neP'i~h) (3.4.2)
v
Let now TV} = {A e P ,\(A, a> e Z for all a e J } be the set of non-degenerate weights from P£. Due to Theorem 2.3, given A e P,, we have ff _ (L(A)) = 0 unless A e Nj. The set Nj is non-empty if p' satisfies the same inequality (3.4.1) as p. In the case A e Nj we have, using Theorem 3.2a and [27, (3.4)]: q-<™2*chH-(L(A)) = q>it(*)
©
BsA,
'tM - i th
and that all of its cohomologies but 0 vanish, and the 0th cohomology is isomorphic to L(A). Here ttA(s) denotes £t{s), where s is the image of se WA in W under their isomorphism. The existence of this resolution has been proved for any integrable representa tion over arbitrary g [18] and for any modular invariant representation over A\l> [4, 18]. Resolutions of this kind were extensively studied in [10]. If we apply our functor F+ to this resolution, then we get the complex of modules RA over the FF-algebra, such that £!.= ©
K.M,
se W"
because F + (B„) = 0, i * 0, F°+ (BM) = ?tM. By definition, the ilh cohomology of the complex RA coincides with F + (L(A)). Conjecture 3.5.2. RA is a resolution of an irreducible module F + (L(A)) over the Walgebra: all of its cohomologies but St(w)th (where w is the element, defined in
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Proposition 1.8b(ii)) vanish, and the /f(w)lh cohomology is isomorphic to an irreducible module (with character
( - l)''tr«<7L'°,
( - r i
by the Euler-Poincare principle. This is equal to ( - l)"(w' I
( - lfMtr^AqLi
= ( - l)"(w) £
(-
lY'Mqn-Vriix)-'.
We get the same formula as the one obtained by means of the residue calculation. Now Conjecture 3.4+ follows from Conjectures 3.5.1 and 3.5.2. Note that the lowest eigenvalue of LQ on RA is equal to P(w.A), where w is the element of WA, which corresponds to the element w under the isomorphism W ~ WA, and that the corresponding eigenspace is the span of the vacuum vector of n*.A. Therefore this vector represents a cohomology class in F'l{w)(L(A)), which is the highest weight vector of F+(L(A)). It is natural to assume that the Pfn(g)-modules which are the images of L(A), Ae Nk+ under the functor F+ form a minimal model of the corresponding conformal field theory in the sense of [3]. In the next section we will prove that the linear span of characters of these modules form a representation of SL 2 (Z) and we will use the information on the action of this group to deduce the fusion algebra of this theory by means of the Verlinde argument.
4. Fusion Rules for W-Algebras in the Simply Laced Case Throughout this section we will assume that g is simply laced (i.e. of type Af, D( or £,); equivalently: ax = a(v for all i (i.e. r v = 1). 4.1. Some Properties of the Group W+^ We use here results and notation of Sect. 1.1. Let Q be the root lattice and P the weight lattice of g. Note that Q* = P, Hence by (1.1.3) we have for any keZ
Cv = 6 •
(4.1.1)
relatively prime to \J\:
{kA~i}iej is a set of representatives of P mod Q .
(4.1.2)
Lemma 4.1.1. Let k e N be relatively prime to\J\. Then for any X e Pk there exists a unique w e W+ such that w(X) e Q. Proof By (4.1.2), there exists a unique; e J such that X = kAj mod Q. Since (for any JEEZ)
WJ(X) = Wj(X) + kAj and w(X) = X mod Q if w e W, the lemma follows.
(4.1.3) □
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By (4.1.2), there exists a unique s e J such that A,-peQ. Of course, s = 0 if p e Q. In all other cases s is listed below: s = i (/ + 1) if g is of type A(, t odd, s= 1 if g is of type De, { = 2 or 3 mod 4, s=6
if g is of type £ 7 .
Note the following properties of s: 2J.ee,
ws2 = l .
(4.1.4)
Lemma 4.L2. Given j e J, let ieJbe_ defined by vv, = v/Jl (i.e. Wi(A}) = A0). (a) wt(A}) + A{ = 0, /zence /1( + /l^ = 0 mod Q. (b) IfXeP\,then + hv)Aj = Wj(w,(A) + p).
X+ p-{k
Proof, (a) (resp. (b)) follows from (4.1.3) where we let; = i and replace A by Aj (resp. by A + p - (k + hv)AJy which has level 0). □ Lemma 4.12a immediately implies Lemma 4.13. Let ji,j2>J3 zJ ond let ajtl = a^, t = 1, 2, 3. Then (a) Ah + A_h + A_h e Q iff Ah +_Ai2 +_Ah eQ. (b) Ah + Ah + Ah + peQ iff Ah + Ah + Ai3 + peQ. 4.2. A Transformation Formula for Functions ep^Cr). Recall that
(4.2.1)
where w(A, p) = (wA, wp). The following transformation formula follows from Theorem 1.7 and Proposition 1.8a (see [28, proof of Theorem 4.4]): Let p and p' be relatively prime integers greater than or equal to h and let (A, A') e Ipp-. Then
Z
Sa>r)>(Mi(,-)
(4.2.2)
where
Sa.
A-)(M. „•> =
(pp')" ' / 2 1JI"' / 2 e 2 *'"^ ""+ w + {X'+ m v
/ .
£
, e
x Z (> )
- ^ ( J ' + P W + P)) ^
p
+m ,
,
£ w e
Z ( )
- ^ ( J + P X / J + P))
p
(4-2-3)
Note also a special case of Theorem 1.7 when A e Pk+,keZ+ (and g is simply laced): Xx\s= Z Si.,&.
(4.2.4)
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E. Frenkel, V. Kac and M. Wakimoto
where Si., = i^(k +
fc)-"Vr»'2
£
e (w)e"*^*
M
PW + W
.
(4.2.5)
Recall also the following important fact [25]: SwX,v = e-^wA"^SKll
if w e W+ .
(4.2.6)
Our objective is to express the S(A>i.)>((,fM', in terms of the SA>(t. We shall assume that p' and | J | are relatively prime. Then we may choose (andfix)positive integers a and a' such that ap' = 1 mod p\J\,
a'p = 1 mod p', a' = 1 mod | J | .
(4.2.7)
Note that a' and p'\J\ are relatively prime, hence we can find a positive integer V such that: a'b' = 1 m o d p V I -
(4.2.8)
Lemma 4.2.1. Suppose that X e Q. 77ien (a) X:= a(p'(X + p) - p(X_+ p)) = X+ p - pA, mod pQ. (b) Y:=a'[p(X + p)-_p'(X + p)) _ f A' + p — p'A modp'Q if peQ or p is even ~~ \X + p — p'(X + p) modp'Q if piQ and p is odd . Proof By (4.2.7), ap'(X + p) = X+_p mod Q, hence X s l + p - app mod pQ. If p e g , (a) follows. In the case p$ Q, p' is odd since | J | is even (see Sect. 4.1), hence a is odd. Hence app = p mod pQ since 2peQ and (a) follows from the definition of A, in Sect. 4.1. The proof of (b) is similar. □ Lemma 4.2.2. Let i i e N d c relatively prime to p\J\ (resp. p'|J|). Let XePp+~h (resp.ePp+~h). Define the map
l)hA0 = w(4>b(X) + p),
weW;
e»(A) = e(w). Then the map
(4-2.9)
then y = 1. Note that k:= p/fe — h is a principal admissible rational number with denominator b. Dividing both sides of (4.2.9) by b we get: X + p-(b-
1)(* + /»v)/lo = y(A, +p-(b-
1)(* +
hv)A0).
So A:=X + p-{bl)(k + hv)A0 and /^ := At + p - (b - l)(fc + hv)A0 are principal admissible weights such that_ RA = RA' = Rlb] and A = yAx. Hence yRm = R[b], therefore there exists t„w e W+ such that y = t^w. Since b and | J | are relatively prime and ba. e M, we deduce that a e M, hence a = 0 and w = 1 (see Sect. 1.2). Thus, y = 1. □ Given A e P\~h (resp. A' e P<"*X we let Xb =
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Fusion Rules for W-Algebras
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Proposition 42. Let (X, X') and (fi, n') be elements ofP"+~h x P"+~h such that X' e Q. We define j eJ by letting 'X mod Q if peQ or p is even (case 1) \ X + p mod Q otherwise (case 2) ,
1
and let w( = w]'1. Then VA',.<M.M-) = ( - l) |J ' l Ul 1/2 e(w J )e(^)e p .(/i)£;.(/i')
Proof We rewrite (4.2.3) using the following calculations: ye*
= I
ye*
e(y)e
, „ „
^
p
(by (4.28))
. .
- ^ ( a ' ( p ( X ' + P)-p'('T+p)|>'(/ii+p)))
= e'b.(fi') X s t ^ e " yt W
= ei.(|i')e(wy) X £(-V)e
p
(by Lemmas 4.2.1b and 4.1.2b). Similarly, we have: ^ r + M + v £ e ( w ) C " ? ? ( r + " W l ' + ')) W£
*
= X e{w)e " we *
= ep.(^)e(wJ) 2, e(w)e
'
we*
by Lemma 4.1.1a. Substituting in (4.2.3) and using (4.2.5) gives the result.
□
4.3. A Calculation of the Fusion Rules. First, recall Verlinde's formula for fusion rules [35]. Suppose that we have a finite set / of representations of a "chiral algebra" such that (i) the vacuum representation, labeled by 0, lies in / ; (ii) the linear span of normalized characters {xx}xei *s SL 2 (Z)-invariant and the action of S e SL2(Z) is given by a matrix (SAM)i>)(e/. Then the fusion coefficients NXltv are given by the following formula:
^V=I^4^. ael
(4.3.1)
^Oa
If, in addition, an involutive map X t-» 'X of / into itself is given, one defines the fusion algebra as an algebra over C with basis {xx}xei and the following multiplica tion: Xx * X„ = Z
WA«'VXV .
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E. Frenkel, V. Kac and M. Wakimoto
In the case when the chiral algebra is the affine algebra g and the set of its representations is L(k), XePI, the vacuum representation is L(mA0) and one knows an explicit expression for the fusion coefficients N A(JV (A,/i, v e P + ) [24, Exercise 13.35]. Let now k be a principal admissible rational number with the denominator p' and let p = p'(k + h). Note that p £ h and (p, p') = 1. Recall that Nk± * 0 if and only if p' k h (Proposition 1.5a). We consider the set of representations of the W-algebra rVk{q) obtained from the principal admissible representations of g by a quantum Drinfeld-Sokolov reduction. Recall that (by Proposition 3.4) these representations are parametrized by the set IPiP=(Pp+'kxPp+''')/W+, that the vacuum representation is labeled by ((p — h)A0, (p' — h)A0) and that a representa tion labeled by the pair (A, /z) has normalized character q>x,^)Theorem 43. Let p and p' be integers such that p,p'^h and (p, p') =_(p', \J\) = 1. In A(i) e Ip p- (i = 1,2, 3) choose a representative (Af, A'f) such that X\ e Q (see Lemma 4.1.1). Then AUn-Ww = Nx^,NliiM , (4.3.2) where Nx XlX and NX'XiXi are fusion coefficients for g. (Similar result holds in the case when(p,\J\)=l.) First, note the following lemma, which follows immediately from (4.2.6) and (4.3.1): Lemma 43.1. Let i t , i2, i 3 e_J and A,, A2, A3 € P +, k e N. Then (a) IfA_h + Ah + 4 J 3 e Q, then NWiMilWiMAwiMi) = NXiXjXr (b) IfAtl + Ai2 + A,t + peQ, then NWI„IMIXWIMI),WIMS) = NXiXiX}.
D
A special case of Lemma 4.3.1a is Lemma 43.2. Let A,, A2, A3 e P\. Then Nli:WMiiwMi) = A^,*,,^. Proof of Theorem 4.3. Let k0 = (p- h)A0, A'0 = (p' - h)A0. For each t = 0, 1, 2 or 3, define j(t) e J by letting (cf. Proposition 4.2): -
_ ( A, mod Q in case 1 [X, + p mod Q in i r\.f | y n i v u ^ i n case wuov 2 ^ .•
J< —
"
and define i(t) by by w wi(() = wf^. wf^. In In particular, particular, i(() = w Now, using Verlinde's formula (4.3.1), ^ifo) formula (4.2.6), case 1,Proposition and = w, in4.2 case and 2. no) = 1 in Lemma weVerlinde's obtain theformula following(4.3.1), formula: Now,4.2.2 using formula (4.2.6), Proposition 4.2 and Lemma 4.2.2 we obtain the following formula: ^U.^mA),
=
^^.^.i^^uWl"imWl«iaMi)
>
(4-3.3)
where £ = e(wj(1))e(Wji2))e(Wjm)E(,, and e0 = 1 in case 1, e0 = e(w5) in case 2. Furthermore, it follows, for example, from the explicit formula in the affine case [24] that Nililit * 0 implies X1+X2 + X3eQ.
(4.3.4)
In case 1, we may assume, due to (4.3.4), that AJ(l) + Aj(2) + AJ(3) e Q, hence ^((D + ^t(2> + Ai(3) e Q by Lemma 4.1.3a. It follows that e = 1 and, by Lemma 4.3.1 a, that NWioMil WimWX WiiiMi) = A ^ , proving the theorem._ In case 2 we similarly have Aj{1) + AH2) + AJi3) + peQ, hence /l i ( 1 ) + Ai(2) + ^«3) + p e 6 by Lemma 4.1.3b. It follows that £ = 1 and, by Lemma 4.3.1b, that
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Fusion Rules for JF-Algebras
327
One has the following involutive automorphism of the set Ip,p'. '((A, X) mod W+) = ('X, 'k') mod W+ , where 'X is defined by (1.4.3). Since w° is the unique longest element in W, w° commutes with fV+, hence this map is well-defined. Theorem 4.3 may be refor mulated as follows. Theorem 43'. Let p and p' be relatively prime integers such that p, p' ^ h, and assume that {p, | J\) = 1 (resp. (p', \J\) = 1). Let st"'"' be the fusion algebra for the Walgebra Wk($), where k = p/p' — h. Given meZ+ let s/m denote the fusion algebra for the affine algebra g with K = m (and the index set P +) and let s/" denote its subalgebra spanned by the Xx with Xe Q. Then: tfp-p' = ^ - * ® jar'-* (resp. = st"'"® stf-") . Remark 4.3. If | J | is a power of a prime number, then either p or p' is relatively prime to \J\. Thus, Theorem 4.3 describes fusion rules completely in all (simply laced) cases except for g of type AH, n not a power or a prime. The following result takes care of all cases (but it is not as nice as Theorem 4.3). Its proof is the same as that of Theorem 4.3. Proposition 43. Let p and p' be relatively prime integers greater than or equal to h. Choose integers b and b' such that (p — b'p', \J\)= 1 and (p' — bp,\J\)= 1. Let a = w„ (resp. = \)ifb is even {resp. odd) and o' = w, (resp. = 1) ifb' is even (resp. odd). Given A({) e IPtP; i = 1,2, \ choose their representatives (A(, Aj|(resp. (Af, A?')) such that b(X~t + p)'- (X\ + p)eQ (resp. b'(k~? + p) - (I? + p)e Q). Then
References 1. Bais, F.A., Bouwknegt, P., Schoutens, K., Surridge, M.: Extensions of the Virasoro algebra constructed from Kac-Moody algebras using higher order Casimir invariants. Nucl. Phys. B304, 348-370 (1988) 2. Bais, F.A., Bouwknegt, P., Schoutens, K., Surridge, M.: Coset construction for extended Virasoro algebras. Nucl. Phys. B304, 371-391 (1988) 3. Belavin, A., Polyakov, A., Zamolodchikov, A.B.: Infinite conformal symmetry in two dimen sional quantum field theory. Nucl. Phys. B241, 333-380 (1984) 4. Bernard, D., Felder, G.: Fock representations and BRST cohomology in SL(2) current algebra. Commun. Math. Phys. 127, 145-168 (1990) 5. Bershadsky, M.: Conformal field theory via Hamiltonian reduction. Preprint IASSNS-HEP90144, 1990 6. Bershadsky, M, Ooguri, H.: Hidden SL(n)-symmetry in conformal field theory. Commun. Math. Phys. 126, 49-84 (1989) 7. Bilal, A., Gervais, J.-L.: Conformal theories with non-linearly extended Virasoro symmetries and Lie algebra classification. In: Adv. Ser. Math. Phys. vol. 7, pp. 483-526. Singapore: World Scientific 1989. See also Phys. Lett. B206, 412 (1988); Nucl. Phys. B314, 646 (1989); Nucl. Phys. B318, 579 (1989) 8. Blumenhagen, R., Flohr, M., Kleim, A., Nahm, W., Rechnagel, A., Varnhagen, R.: W-algebras with two and three generators. Nucl. Phys. B354, 255-289 (1991) 9. Bouwknegt, P.: Extended conformal algebras from Kac-Moody algebras. In: Advanced Ser. Math. Phys. vol. 7, pp. 527-555. Singapore: World Scientific 1989 10. Bouwknegt, P., McCarthy, J., Pilch, K.: Free field approach to 2-dimensional conformal field theory. Progr. Theor. Phys. Suppl. 102, 67 (1990) 11. Bowcock, P., Goddard, P.: Coset constructions and extended conformal algebras. Nucl. Phys. B305, 685 (1988)
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12. Burroughs, N.J., de Groot, M.F., Hollowood, T.J., Miramontes, J.L.: Generalized DrinfeldSokolov hierarchies II: The Hamiltonian structures. Preprint IASSNS-HEP-91142, 1991 13. Deodhar, V.V., Gabber, O., Kac, V.G.: Structure of some categories of representations of infinite-dimensional Lie algebras. Adv. Math. 45, 92-116 (1982) 14. Drinfeld, V.G., Sokolov, V.V.: Lie algebra and the KdV type equations. Soviet J. Math. 30, 1975-2036 (1985) 15. Fateev, V.A., Zamolodchikov, A.B.: Conformal quantum field theory models in two dimen sions having Z 3 symmetry. Nucl. Phys. B280 [FS18], 644-660 (1987) 16. Fateev, V.A., Lukyanov, S.L.: The models of two-dimensional conformal quantum field theory with Z. symmetry. Int. J. Mod. Phys. A3, 507 (1988) 17. Fateev, V.A., Lukyanov, S.L.: Additional symmetries and exactly soluble models of twodimensional conformal field theory. Kiev preprints, ITF-87-74, 75, 76 (1988) 18. Feigin, B., Frenkel, E.: Affine Kac-Moody algebras and semi-infinite flag manifolds. Commun. Math. Phys. 128, 161-189 (1990) 19. Feigin, B., Frenkel, E.: Affine Kac-Moody algebras, bosonization and resolutions. Phys. Lett. 19, 307-317 (1990) 20. Feigin, B., Frenkel, E.: Affine Kac-Moody algebras at the critical level and Gelfand-Dikii algebras, preprint RIMS 796, 1991 (to appear in Proceedings of RIMS-91 Program) 21. Feigin, B., Frenkel, E.: Quantization of the Drinfeld-Sokolov reduction. Phys. Letts. B 246, 75-81 (1990) 22. Felder, G.: BRST approach to minimal models. Nucl. Phys. B317, 215-236 (1989) 23. Frenkel, E.: ff-algebras and Langlands-Drinfeld correspondence, to appear in Proceedings of Cargese Summer School, 1991 24. Kac, V.G.: Infinite-dimensional Lie algebras. 3-d edition, Cambridge: Cambridge University Press 1990 25. Kac, V.G., Wakimoto, M.: Modular and conformal invariance constraints in representation theory of affine algebras. Adv. Math. 70, 156-236 (1988) 26. Kac, V.G., Wakimoto, M.: Modular invariant representations of infinite-dimensional Lie algebras and superalgebras. Proc. Natl. Sci. USA 85, 4956-4960 (1988) 27. Kac, V.G., Wakimoto, M.: Classification of modular invariant representations of affine algebras, in: Adv. Ser. Math. Phys. vol. 7, pp. 138-177. Singapore: World Scientific 1989 28. Kac, V.G., Wakimoto, M.: Branching functions for winding subalgebras and tensor products. Acta Applicandae Math. 21, 3-39 (1990) 29. Khovanova, T.: Super KdV equation related to the Neveu-Schwartz-2 Lie superalgebra of string theory. Teor. Mat. Phys. 72, 306-312 (1987) 30. Kostant, B., Sternberg, S.: Symplectic reduction, BRS cohomology, and infinite-dimensional Clifford algebras. Ann. Phys. 176, 49-113 (1987) 31. Lukyanov, S.L.: Quantization of the Gelfand Dikii algebra. Funct. Anal. Appl. 22:4, 1-10 (1988) 32. Mukhi, S., Panda, S.: Fractional level current algebras and the classification of characters. TIFR preprint, 1989 33. Polyakov, A.: Gauge transformations and diffeomorphisms. Int. J. Mod. Phys. A5, 833 (1990) 34. Thierry-Mieg, J.: Generalizations of the Sugawara construction. Proceedings of Cargese Summer School, 1987 35. Verlinde, E.: Fusion rules and modular transformations in 2D conformal field theory. Nucl. Phys. B300, 360-375 (1988) 36. Watts, G.T.M.: If-algebras and coset models. Phys. Lett. B245, 65-71 (1990) 37. Zamolodchikov, A.B.: Infinite additional symmetries in 2-dimensional conformal quantum field theory. Teor. Mat. Phys. 65, 1205-1213 (1985) Communicated by A. Jaffe Note added in proof. Two of the authors of the present paper have shown recently that the quantum reduction applied to modular invariant representations of affine superalgebras osp(l, 2n)<1) (resp. sl(l, 2n)(1)) gives the "minimal" series of representation of certain W-superalgebras. In particular, for n = 1 one recovers all "minimal" representations of N = 1 (resp. N = 2) superconformal algebras.
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Reprinted with permission from Nuclear Physics B Vol. 379, pp. 63-95,1992 © 1992 Hsevier Science Publishers B. V. (North-Holland)
On the classification of quantum W-algebras P. Bowcock
12
Enrico Fermi Institute, University of Chicago, Chicago, IL 60637, USA
G.M.T. Watts 3 Department of Mathematical Sciences, University of Durham, South Road, Durham, DH1 3LE, UK Received 5 December 1991 Accepted for publication 27 February 1992
In this paper we consider the structure of general quantum W-algebras. We introduce the notions of deformability, positive-definiteness, and reductivity of a W-algebra. We show that one can associate a reductive finite Lie algebra to each reductive W-algebra. The finite Lie algebra is also endowed with a preferred sl(2) subalgebra, which gives the conformal weights of the W-algebra. We extend this to cover W-algebras containing both bosonic and fermionic fields, and illustrate our ideas with the Poisson bracket algebras of generalised Drinfeld-Sokolov hamiltonian systems. We then discuss the possibilities of classifying deformable W-algebras which fall outside this class in the context of automorphisms of Lie algebras. In conclusion wc list the cases in which the W-algebra has no weight-one fields, and further, those in which it has only one weight-two field.
1. Introduction In the last few years remarkable progress has been made in the understanding of two-dimensional field theories that are conformally invariant. A key to complet ing this program is the classification of extended conformal algebras, or W-alge bras. The first examples of W-algebras were the conformal algebra, various superconformal algebras and Kac-Moody algebras [1]. Later it was realised that a wider variety of algebras could be constructed from GKO coset theories [2-5]. Interest then moved to Toda theories, which provided many examples of W-alge bras [6]; later these were re-incorporated into the Drinfeld-Sokolov scheme of hamiltonian reductions [7-10]. Most recently it has been shown that the gener alised Drinfeld-Sokolov reduction of WZW models can be used to produce a new 1 2 3
[email protected] Supported by US DOE grant DEFG02-90-ER-40560 and NSF grant PHY900036. E-mail [email protected]
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class of algebras. In this construction one gauges a WZW model associated with a Lie algebra g by the currents associated with some nilpotent subalgebra. For bosonic W-algebras with fields of integer conformal weight, the nilpotent subalge bra can be labelled by an (integral) su(l, 1) embedding in g [11]. This latter model has the advantage that the properties of the algebra obtained are easily related to the finite Lie algebraic ingredients of the construction, while the corresponding relationship in the GKO case is much more mysterious for the present. However illuminating the examples cited above may be, we cannot hope to obtain a classification scheme for W-algebras if we tie ourselves to any one construction. It is this that motivates us to adopt a more general standpoint in this paper. The study of W-algebras is hampered by their infinite-dimensional nature. Worse still, their commutation relations are generally non-linear in the generating fields. Some progress has been made by looking for examples using algebraic computing techniques [12,13], but the calculations involved are complex, and so the searches are restricted to examples containing two or three fields of low conformal weight. In this paper we shall restrict our attention to "deformable" algebras. By deformable we mean that the algebra satisfies the Jacobi identify for a continuous range of values of the central charge c. In general the structure constants of the algebra are allowed to be functions of c. The algebras excluded by this restriction are a very complicated set of objects, which in principle include, for example, a large number of W-algebras which can be constructed from lattices using vertex operators [14,15]. There is some hope that these algebras are extensions of deformable algebras, occurring when a generically non-integer weighted primary field becomes integer weighted for particular values of c. The main result of our paper is contained in sect. 2, where we demonstrate the existence of a finite subalgebra associated with each classical W-algebra. Perhaps of more importance is that we can extend this result to the quantum case if we demand that the quantum algebra have a "good classical limit". After discussing what precisely this means, we demonstrate the existence of a similar finite subalgebra in the limit that the central charge c -»». This provides us with an easily computable characteristic for W-algebras. A special role is played by an su(l, 1) subalgebra of this finite algebra, which corresponds to the modes L,, L0, L_, of the Virasoro algebra which generate Mobius transformations. The characteristic we have derived is a finite-dimensional Lie algebra, and an su(l, 1) embedding. This is precisely the data used in the generalised DrinfeldSokolov reduction method. In sects. 3 and 4 we clarify this connection. After a review of the generalised Drinfeld-Sokolov construction of W-algebras, we calcu late the structure constants of the W-algebra obtained by this method up to linear order in the fields, and use this to demonstrate that in this case the finite subalgebra is simply the Lie algebra g associated with the WZW model that we are reducing and that, further, the su(l, 1) embedding is the same as that used in the
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P. Bowcock, GMT. Watts / Quantum W-algebras
65
construction. This provides us with a proof of the existence of the classical W-algebras associated with each finite Lie algebra g, and su(l, 1) embedding. Armed with these results we discuss certain features of the W-algebras that are constructed in this way in sect. 5. In particular we give a complete list of such algebras which have no Kac-Moody components, and those with only one spin-2 field. We also comment on the possible use of automorphisms of the finite Lie algebra to generate homomorphisms of the W-algebra. The resulting algebras will be deformable, but will not have a good classical limit. Finally, we conclude with some comments on the relevance of our approach to the classification of deformable W-algebras.
2. Finite algebras from W-algebras If we want to classify extended conformal symmetries, or W-algebras, we should like to attribute to them some easily computable characteristics which specify the algebra completely. In this section we shall construct a finite Lie algebra associated with classical W-algebras and their quantum counterparts. Although we do not prove that this specifies the W-algebra, it does reveal something of its structure, and may ultimately form part of some classification scheme. To start with we shall consider the relationship between a general quantum W-algebra and its classical counterpart. After discussing the "vacuum preserving algebra" (vpa) for both types of algebra, we show that in the classical case this contains a finite subalgebra if we define a "linearised" Poisson bracket. We then extend this result to the quantum case by showing that the corresponding finite algebra decouples in the limit that the central charge goes to infinity. Let us begin by discussing the relationship between quantum W-algebras and their classical counterparts. A quantum W-algebra comprises a set of modes W£ of some simple fields W{z), a notion of normal ordering, and a Lie bracket. W-algebras are usually presented in the form of an operator product expansion, which we may represent schematically as
W(z)Wb(z') = *" f c (z-z')- 4 °- 4 * c
+ Lf&Uz-zY+*d-A°-*h[:wc{z')wd(z'):
+...]
c,d
+
...\z\>\z'\.
(2.1)
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Here we have arranged the right-hand side according to degree in W. Since we are interested in conformal field theories, we assume that the algebra contains the Virasoro algebra L{z)L{z')
= \c{z-z')~A
+ 2 L ( z ' ) ( z - z ' ) ~ 2 + dL(z')(z
-z')~l
+ 0(1), (2.2)
as a subaigebra. We also assume that the algebra is generated by a finite number of primary fields W(z) which obey L(z)Wa(z')
= AaW(z')(z
-z')~2
-z')~l
+ dW(z')(z
+ O(l), (2.3)
where A" is the weight of W. The commutation relations of the modes W£ which are given by W(z) = Y.W£z~A°~m can be deduced in the standard manner from the operator product expansion by a double contour integral. These take the form fc
Kb] =g°bP{K,
A„, 0, m, n) +f{\hcP{Aa,
+f&dP{Aa,
Ab, Ac, m, n)W^+n
Ah, Ac + Ad, m, n):W<Wd:m+n
+ ...,
(2.4)
where P is some known polynomial. In terms of modes eq. (2.3) becomes [Lm,W:]=[(Aa-\)m-n]w:+n.
(2.5)
Any field that obeys eq. (2.5) for all m is called primary, and any field that obeys it for m = - 1 , 0, 1 is called quasi-primary. The modes of a quasi-primary field <9'm form an indecomposable representation of the su(l, 1) algebra generated by L_v L(), L,. One can use the representation theory of su(l, 1) to show that the quasi-primary fields and their derivatives span the space of fields in the algebra, and that the polynomials P are related to Clebsch-Gordan coefficients. We define the hermitian conjugate by
m*
= W°_m,
(2.6)
and this induces a natural inner product on the states of the quantum theory. The requirement that this inner product be positive definite and the representation theory of the Virasoro algebra requires that the central charge c > 0 and that the fields all have positive-definite weight. This then implies that the metric gab is only non-vanishing on fields of equal weight, that it is positive-definite, and that a basis of fields satisfying (2.6) can be chosen for which the metric is diagonal. We
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P. Bowcock, C.M.T. Watts / Quantum W-algebras
67
call such a W-algebra positive-definite. With this choice of basis, the algebra (2.4) takes the form [w:,Wnh]=(c/(2Aa-l)lAa)8°bm(m2-l)...(m2-(da-l)2)8m+n<0 +
f&P{Aa,Ab,Ac,m,n)W^n
+ f&dP(*a,
K, K + 4 , , m, n):W<Wdlm+n
+ ...
(2.7)
where / are constants, and we have used that P(Aa, Aa, 0, m, n) = m(m2 1).. .(m2 - (Aa - D 2 )5 m + n 0 - We do not as yet require that the algebra be defined for more than one value of c. Examples of algebras which are not positive-definite include Kac-Moody algebras based on non-compact groups, and algebras includ ing "ghost" fields with strange statistics, such as the bosonic N = 2 superalgebra recently considered in ref. [16]. We should remark on the definition of normal ordering ° " which we use here. In meromorphic conformal field theory, we assign a field uniquely to each state by
(2.8)
We can define the normal-ordered field *<£$'* by :^'>^_^'_^|0>.
(2.9)
However, this is not the only possible normal ordering. Following Nahm [13,17], we have introduced the normal ordering 11, by
:w.=&w*,
(2.io)
where & is the projector onto su(l, 1) highest weight fields so that the resulting composite fields are quasi-primary. Further ambiguities arise when we try to normal order more than two fields, since this product is not associative. One can, for example, decide to order the fields by conformal weight and index a, and then always nest the normal orderings from the left. However, there are many choices of basis. We shall call a particular choice of basis a presentation of the W-algebra as a commutator algebra. The underlying structure, which is that of a meromorphic conformal field theory, is the same for each presentation, but the structure constants will be different. The point that we should like to stress is that the classical limit of different presentations are identical. This is a consequence of the observation that the difference in two orderings can be written as a commutator, and thus must be an Oifi) term which vanishes in the classical limit. (In fact, the projection operator & does not simply amount to a reordering, but the difference
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between the two normal orderings can be seen to be the Virasoro descendents of commutators, so that the result is true in this case too.) Let us now consider classical W-algebras. This is a Poisson bracket algebra of fields W(x) of one variable which closes on (differential) polynomials and central terms. We can represent the Poisson bracket schematically as {W(x),
Wb{y)}=gabdA-+A"-'i8{x
-y)
+ E/ ( lU^ + 4 ^- 1 8(x-y)^(v) c
+g°c» dA°+A"-AC-28{x-y)dWc{y)
+ ...]
+ Lf(£d^+Ab-AC-Ad-l8(x-y)[\VC(y)W<>(y)
+
...}
c,d
+ ...,
(2.11)
where the right-hand side has been ordered according to degree in W, and /("£. z may be functions of the central charge c. Alternatively, if we take the space on which the fields are defined to be the unit complex circle, we can expand the fields in modes exactly as in the quantum case. Identical mode algebras are generated if, in eqs. (2.1) and (2.11) we use the correspondence (z - z ' ) ' N - * (-l)N~12mSN-l(z
- z ' ) / { N - 1)!,
(2.12)
although if we use identical structure constants we do not expect that both quantum and classical commutator algebras satisfy the Jacobi identity if they are non-linear. We shall assume that the classical algebras have a number of proper ties that they would inherit automatically as the classical limit of the quantum algebras. They contain a classical version of the Virasoro algebra
^-{L(x),L(y)}
=
-±c8'"(x-y)-2L(y)8'(x-y)+dL(y)8(x-y),
LIT
(2.13) and the generating fields obey the classical version of eq. (2.5). Further, the only terms in the Poisson bracket algebra which are independent of W are taken to be of the form m{m2 - 1).. .(m 2 - (Aa - l)2)8m+nfi8ab. By analogy, we refer to such algebras as positive-definite classical algebras. We now discuss the relationship between a classical W-algebra and its quantised version. We shall see that an extremely important criterion for a quantum algebra to have a classical limit is that it is well-defined for all values of the central charge
440
P. Bowcock, G.M.T. Watts / Quantum W-algebras
69
c, with the exception perhaps of a few isolated values or closed intervals. By this we mean that that there is an operator product algebra for a set of fields W(z) of fixed conformal weights Aa, with structure constants / ( l ) which are continuous functions of c, which is associative for a continuous range of c-values. We call such algebras deformable. We shall see that deformability is, however, not sufficient for a quantum algebra to have a classical limit. As an example let us first consider the classical Virasoro algebra, eq. (2.13). Quantising this algebra yields [L'n, L'n] = ±tic'm(m2
- l)Sm+nfl
+ (m - n)hL'm+n,
(2.14)
where the prime indicates that we have the normalisation inherited from the classical Poisson bracket structure. To recover the standard normalisation we must substitute L' = hL,
c' = hc.
(2.15)
Similarly, for a general quantum W-algebra, we can re-introduce h by the substitu tions L^L'/h,
c^c'/h,
W^W"/ha°,
(2.16)
where the constants aa are to be determined. The classical limit is given by the usual correspondence [W,
Wb) = lim ~\W'a, A-.O in
W'b\.
(2.17)
For this limit to make sense we require that the quantum operator product algebra remain associative as h -* 0, or equivalently, as c -* oo. This is why the W-algebra must be deformable. Substituting (2.16) into (2.7) we obtain schematically [WJ, W^]^c'h2a'-18+fwWc'ha'+a^a'+f(2^WJW/:ha'+a>'-af-a'
+
0(Wi). (2.18)
For this to be the quantisation of a classical W-algebra, we require that the right-hand side be CKh). The h dependence comes both explicitly from IV-* W'h", but also implicitly, from f(i)(c) -*f^c'/ti). If we have /("xc,)-0( *"<■•**'■»)
asft^O,
(2.19)
and all the fields l(W)pl are (XI), then we must impose that for each term in the singular part of the operator product algebra expansion of W and Wb min ly*+ aa + ab-
£ac.
> 1.
(2.20)
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P. Bowcock, GMT. Watts / Quantum W-algebras
If it is not possible to find such constants aa, then we say that the W-algebra has no classical limit. The restriction (2.20) only restricts the couplings to fields which appear in the commutation relation, or equivalently to fields in the singular part of the operator product of W and Wb. It is obvious that we have no restriction on the regular terms since a b a
w (z)w {z') = ... + :w (z')w\z'): +...,
(2.21)
where the coupling to I W"Wbl is CXD. If the classical limit of a W-algebra is positive-definite, we call the quantum algebra reductive. To examine what restrictions this implies, we must consider the central terms in eq. (2.18). Fixing the behaviour of the central term we require a a = l,
for all a.
(2.22)
For this choice of aa the requirement (2.20) becomes, for each term which appears in the singular part of the operator product expansion. / (/) = 0 ( c ' - ' )
as c - o o .
(2.23)
If it is not possible to impose eq. (2.20), then the only possibility of recovering a classical W-algebra is that the normal-ordered products are no longer O(l). Generically for a W-algebra which comes from the quantisation of a classical algebra we have :Wa(x)Wb{y): = W(x)Wb(y) + 0(h).
(2.24)
It is possible for the first term to vanish if the bosonic fields W", Wb can be written as composite fermionic fields, W = d(x)f(x),
Wb = d(x)e(x),
(2.25)
where classically d(x)d(x) = 0, and quantum mechanically ld(x)d(y)l = O(h). A simple example of this possibility may be seen by considering the first two W(4, 6) algebras of ref. [12]. The coupling constants of these algebras do not meet the requirements in eq. (2.23) or even eq. (2.20). In fact, one of these two algebras can be constructed as the bosonic 'reduction' of a fermionic W-algebra [18], the N = 1 superconformal algebra. This yields a W-algebra with fields of spins 4 and 6, with zero central charge classically. We shall discuss such reductions further in sect. 5. Let us now turn to the question of constructing the advertised finite Lie algebra from classical and quantum W-algebras. Although the full set of modes of a quasi-primary operator ' only form an indecomposable representation of su(l, 1), the subset of modes
{^m.\m\
(2.26)
442
P. Bowcock, GMT
Watts / Quantum W-algebras
71
form an irreducible representation of su(l, 1). The set of all such modes for a W-algebra forms a closed subalgebra. We call this the vacuum-preserving algebra (vpa), since in the quantum case these are precisely the modes which annihilate both the right and left su(l, 1) invariant vacua. Although this algebra involves only a finite number of modes of each field, for a non-linear algebra it will only close on the modes associated with an infinite number of such quasi-primary fields, so that it is not a finite Lie algebra. For the linear Virasoro algebra the vpa is the set {L,, L 0 , L _ J which form the algebra su(l, l) = sl(2, U); for the superconformal algebra, the vpa is the algebra osp(l, 2). These subalgebras give useful information about the structure constants of fields in conformally invariant and superconformally invariant theories, respectively, and we would like to define a similar finite Lie algebra associated to a general W-algebra. Let us consider first a classical W-algebra. The assumption of positive-definiteness says that the algebra takes the form {W°,Wnb) = (c/{{2 Aa-\)\
Aa)m{m2-\)...(m2-{A-\f)8ab8m+n
+ f&P(Aa,
Ab> Ac, m, n)W^„ + ....
(2.27)
If we restrict attention to the vpa, we see immediately that the central terms are absent. We can now consider a new bracket {.,.}P on the modes in the vpa, which consists simply of the linear term in (2.27). We can easily check that the Jacobi identity is satisfied by this new bracket when we restrict to the vpa. This is because for | m | < A", P(Aa, Ab, 0, m, n) = 0 and consequently
(wZ,I,lVnb+pWL\ = E / , 1 f (4 fl , Abt Ad, m, n + p)W*+n+pWip *■
p
'
P
+ ff)dP{Aa, Ac,Ad,m,
-p)W*_pWn\p
+ 0(W3),
(2.28)
so that in the classical case the contributions to the Jacobi identity from the quadratic and higher order terms which we have neglected do not contribute, and so the restricted bracket {»£. W„b}r=f&P(A.,
4 6 , Ac, m, n)W^+n.
(2.29)
is a closed Lie algebra, g. Since we have, by assumption, included the modes L ± „ L0 in the vpa, we see that we automatically have an su(l, 1) embedding su(l, l ) c g given by a classical W-algebra. In the case of the Zamolodchikov algebra WA 2 , we have the modes {Q±2, Q±\, Qo, L±x, L0} forming the algebra sl(3) with su(l, 1) in the maximal regular embedding.
443
72
P. Bowcock, GMT. Walls / Quantum W-algebras
We should like to attempt the extension of this argument to the quantum case. In the classical case, the contribution from composite terms to the linear terms in the double commutator vanished for the vpa because the only possible 'contrac tion' from three fields to one arose from the central term which decoupled precisely for these modes. However, in the quantum case there are other contribu tions to this term which arise from the need to normal order composite fields. As an illustrative example we return to the Zamolodchikov algebra WA2, this time in its quantised version. The quantum commutation relations are [Lm,Q„) = {2m-n)Qm+n,
(2.30)
c m{m2 - \)(m2 - 4)
+ {m
n) 2m2 30
(
'
m n + 2 2
" ~ *)Lm + n+P{rn-n)Am+n,
(2.31)
where /3=
16 22T5^'
MZ)
(2.32)
= :T(Z)T(Z):.
The only non-trivial double commutators are [Lp[Qm, (?„]], [Qp[Qm, Qn]] and the only composite field appearing in the intermediate channel is A, so we need only consider the linear terms in [Lp, Am+„], [Qp, Am+n]. These are [Lp,pAm+n}=— [Qp,pAm+n]=[i[4(5pi-5p2(m
16
p(p2-\) 'Lm+n+p+..., 3j + n) + 3p(m + n)2-(m
+ 9(m+n))]/35Qp+m+n+....
(2.33) +
n)3-np (2.34)
The first of these commutators vanishes when we take p = - 1, 0, 1. In the second commutator there is a contribution from the A term in [Q, Q] which does not vanish even when we restrict to the vpa, and a more careful consideration of this term shows that it arises from the need to normal-order composite fields. Instead we can ensure that this term does not violate the consistency of the 'linearised' Jacobi identity by taking the limit c -» °°. In this case /3 -> 0 and the vpa linearises, again to give sl(3, R). Note that we need to combine the limit c -* °° and the restriction to the vpa to ensure that both commutators vanish. We are now in a position to prove this feature, namely that the vpa linearises to give a finite Lie algebra as c -» », assuming that the W-algebra is reductive. Let us
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P. Bowcock, G.M.T. Watts / Quantum W-algebras
73
denote a generic composite field composed of i basic fields as l(W)'l. The contribution to the Jacobi identity from the coupling through such terms in [W, [Wb, Wc}} is K°,
K " , Kc]\ = E K a , f$P(Ab,
4 C , A0), n, p)l(Wy:n+p].
(2.35)
i
Let us also write the linear part of the contribution from the commutator of W with W(i\ K°> :(H0':„] =8%P(Aa> Ao> A<> m' n)W^+n.
(2.36)
At this point we must split our argument into two cases, depending on whether l(W)'l appears in the singular or regular part of the operator product expansion of W with W. If l(W)'l appears in the singular part of the operator product expansion then we can calculate the order of g(l) by taking the three-point function
cabi = <ww<:(wy:).
(2.37)
This can be written in two ways. We have that ca6,=/(l)'<:(^'::(^)':> = o(c), using eq. (2.23) and evaluating the leading contribution (0\(W)'Aii(.Wy_AJ0). We also obtain Cabl = g0){WaW<)~g%c,
(2.38) in c to (2.39)
using eqs. (2.7) and (2.36), and suppressing non-zero constants. Thus we see that g") = (XD and so the contribution to the Jacobi identity of three basic fields [W, [Wb, Wc]] to the field We from the term in [Wb, Wc] of the form KWYl is Oig("f^) = 0(c}-i), if the field :(W)'I appears in the singular part of the operator product expansion of W with W. However, if the field °(WO'I does not, then we cannot apply eq. (2.23) to deduce the order of the coupling g"Y In this case we have that \{W)'\ has conformal weight A(i)^Aa+Ae. However, the polynomials P(Aa, 4 ( 0 , Ae, m, n) vanish identically if \m\ oo, then all contributions to linear terms from composite fields in the intermediate channel drop out. Since the commutator algebra is a Lie algebra for all c values by the assumption of deformability, the only obstruction to the vpa algebra restricted to the generating fields satisfying the Jacobi identity was
445
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from such contributions. Thus, this algebra in the c -* °o limit of a reductive W-algebra is a finite Lie algebra. We have now shown how to recover finite Lie algebras from positive-definite classical W-algebras and reductive quantum W-algebras. We shall call this the linearised vpa algebra. By the Levi-Malcev theorem, the most general form for a finite Lie algebra would be the semidirect product of a semi-simple Lie algebra with its radical, which is its maximal solvable ideal. However, we can use the positive-definiteness of the classical algebra to show that the maximal solvable ideal of the finite Lie algebra we have constructed is in fact its centre, or, in other words, that the linearised vpa is the direct sum of a semi-simple Lie algebra with an abelian Lie algebra (For results on the structure of Lie algebras used here, see e.g. ref. [20]). To do this, let us consider the maximal solvable ideal a of the linearised vpa of a reductive W-algebra. Let us suppose that a particular mode W£ e a. The modes L±l, L0 are always in the linearised vpa, and we know the commutation relations of W£ with Lm to be of the form [Lm,Wn°]=((Aa-l)m-n)WZ+n.
(2.40)
Since a is an ideal, eq. (2.40) implies that M ^ e a ^ ^ ' e a for all \n\
= (c/A)(z-z')~2/i'
+ 2L(z')(z-z')~2*-
+2
+ .... (2.41)
Using the Virasoro Ward identities, (see e.g. appendix B of ref. [21]), we can deduce the coefficients of all the terms d'L(z') in this operator product and we can deduce that [W£_xt W?_A] = 12(4 - l)/(A(2A
- 1))L 0 + ....
(2.42)
For Aa > 1 this is non-zero, and so, for Aa > 1 we have L0 e a. If L0 e a, then we immediately we get that L0, L ± , e a, which is a contradiction since a solvable ideal cannot contain a semi-simple algebra. So, if W£ e a, where a is a solvable ideal, then 4 a < 1. If Aa<\ then it contributes no modes to the vpa; if Aa = 1 then m = 0, and we can thus denote the elements of a as £/0', the zero modes of a set of weight one fields U'(z). These zero modes UQ form a solvable Lie algebra. However, it has been known for a long time (see e.g. ref. [22]) that the requirement that the inner product on the primary fields of weight one is positive-definite forces them to have a Kac-Moody algebra based on a compact semi-simple Lie algebra plus some u(l)" current algebra. Thus the zero modes of weight one fields in eft form a finite-dimensional Lie algebra which is the direct product of a semisimple Lie algebra with an abelian algebra, and we see that the ideal a is abelian.
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P. Bowcock, GMT. Watts / Quantum W-algebras
75
The only possibility left open to us now is that the linearised vpa has the structure of a semi-simple Lie algebra semidirect product with an abelian algebra. Suppose that U0 e a. Then [U0, W°] e a for all W£ in the vpa. If [U0, W£] = Xm, then the operator product expansion of U(z) with W(z) must be of the form U(z)W(z')
= ...+X(z')(z-z')~l
+ 0(1),
(2.43)
since UQ = / dz/(2vi)U(z). However, from eq. (2.43) we see that the field X must have conformal weight equal to that of W. Since Xm e a, we see that X must have weight one, and so W must have weight one. We already know that a commutes with the zero modes of the spin-one fields, so in fact a is the centre of the vpa. This completes the proof that the linearised vpa of the classical limit of a reductive W-algebra is the direct sum of a semi-simple Lie algebra with an abelian algebra. The above discussion has been for a purely bosonic W-algebra. If we wish to include fermions then we must also consider Lie superalgebras, since the vpa of fermionic fields will contain anti-commutators of the modes of fermionic fields. We shall use the notation of ref. [23] for Lie superalgebras, with the algebra decomposition g = go®8T.
(2-44)
where the bosonic generators are in gg and the fermionic in g^. We define the grade of a generator X to be g(A')=/ if X^gy The (super) Lie bracket then takes the form [X, Y]=XY-(-l)*ix)slY)YX
(2.45)
The bosonic fields have modes in g0 and the fermionic fields have modes in g^ It will also be the case that the bosonic fields will have integral conformal weight and the fermionic fields half-integral conformal weight, for unitarity. A fermionic field of weight A will have mode decomposition *(*)-
E
(2-46)
neZ+l/2
As for bosonic fields, the vpa contains the modes of the fermionic fields *M:|m|'<4.
(2.47)
We see that for a free fermionic field of conformal weight | , there are no modes in the vpa. Thus analysis of the vpa will yield no information on the free fermion content of a theory. However, this is not an obstacle since free fermions have
447
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already been shown to factorise from the Hilbert space by Goddard and Schwimmer [24]. Since the fermionic fields will have half-integer modes, the su(l, 1) decomposi tion must be compatible in the sense that the decomposition takes the form 8o=®>ez^,
gl=^i6Z
+ i/2Dj
(2.48)
where D ; is the representation of dimension 2j + 1. We can also prove that the superalgebra consists of the direct sum of simple (super)-algebras and an abelian Lie algebra in an analogous manner to that above for purely bosonic W-algebra vpa's. This means that the field content of any positive-definite W-algebra which is defined for all c-values must comprise a set of free fermion fields of weight one-half (which do not contribute to the vpa; such fields have already been shown to factorise [24]), a set of bosonic free fields of weight one (u(l)" current algebra) and a set of fields whose weights are given by an sl(2) embedding in a semi-simple Lie superalgebra which is compatible with the grading of the superalgebra as in eq. (2.48). For a purely bosonic W-algebra, the field content will comprise a set of weight one fields and a set of bosonic fields whose conformal spins are given by an integral su(2) embedding in a semi-simple Lie algebra. We shall now go on to show that this is indeed the case for the generalised Drinfeld-Sokolov constructions mentioned earlier, and then to consider various cases of particular interest. The rest of this paper will be concerned only with the case of bosonic algebras for simplicity.
3. Hamiltonian systems and co-adjoint orbits The analysis of the previous section showed that to each reductive W-algebra one could associate a finite Lie algebra with some su(l, 1) embedding specified. This is reminiscent of the data that is required for a generalisation of the Drinfeld-Sokolov construction of hamiltonian structures that have been studied recently [11,25,26]. In sect. 4 we shall show that this data is recovered as the finite Lie algebra we constructed. This provides us with an existence proof for the classical W-algebras associated with each Lie algebra and su(l, 1) embedding. In this section we give a brief review of this construction. The classical hamiltonian systems of Drinfeld and Sokolov [8] are based on a Poisson bracket structure of g*, the dual to the Lie algebra g, and the extension of this to g, the centrally-extended Kac-Moody algebra related to g. An element of g consists of a pair, (j(z),c),
(3.1)
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P. Bowcock, G.M.T. Watts / Quantum W-algebras
77
where c is a number and / is a field on S1 values in g. The coordinate on S1, we denote by z, with 0 < z < 2n. With this definition, the Lie bracket of two elements of g is given by [(;>(*), c 1 ), ( ; 2 ( z ) , c 2 )] = ([y»(z), j\z)),kJTr{d}\z)j\z)}
dz), (3.2)
where the second term corresponds to the cocycle of g. An element of g* is given by a pair (q, A), where q is a g-valued field on S1 and A is a number. The action of this element on (/, c) in g is given by ((q, A ) , ( ; , c ) ) = /Tr{ 9 y}dz + cA.
(3.3)
With this, we may identify g and g*, and we obtain a canonical action of g on g*, the co-adjoint action ad*. If (q, A) e g*, (/', c') e g, then we have ad* l i c V (q, A)[(; 2 , c 2 )] = (q, A)[ad ( / , c V (; 2 , c 2 )]
-((«.A),([Aj a ],*/Tr{(;>)>})) = /tr{[ < ?,y 1 ]y 2 + ^ y V 2 } . Thus we obtain ad ( *. V ) -(9,A) = ( [ 9 + *Aa,y I ],0). This is simply an infinitesimal gauge transformation of q. This phase space also has a canonical action of G, the co-adjoint action Ad*, given by Ad*- 9 (/ l )= 9 (Ad [ / -/z), Ad*,-(, X) = (U-lqU + k\U-ldU, A).
(3.4) (3.5)
There is a canonical Poisson bracket structure on g*, the Berezin-KirilovKostant-Lie-Poisson bracket. If U, V are two functional on g*, then their Poisson bracket is also a functional on g*. When evaluated on q e g * it is explicitly given by {U,V}g=(q,[dqU,d(lV]KM),
(3.6)
449
78
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Watts / Quantum W-algebras
where djU, d ; K are any elements of g, such that for all 8j e g*, U(j + Sj) = U(j) + (djU, Sj) + 0(8j2).
(3.7)
We shall usually suppress the ;' suffix if it is clear from context. We may accordingly evaluate the Poisson brackets of the components of g*. If {T1} form a basis of the generators of g with Tr{TT y } =g'', then we can define the functional T'(x), e on (q, A) e g* by fi(x)[(q,\)]=Tr{T'q(z)},
e[(q,\)]=\.
(3.8)
de = (0, 1).
(3.9)
We have dr(x)
= (T'8(x-y),0),
Thus we evaluate the Poisson brackets of these functionals {r(x),f>(y)}(tlX)
=
fdzTr{q[r8(x-z),r8(y-z)} + k\ dz(P8(x
-z))TJ8(y
-z)}.
Thus we see that {r(x),f'(y)),qJi)=rkfk(y)8(x-y)-keg^8'(x-y).
(3.10)
This is the Kac-Moody algebra g. In particular we shall often denote the zero-grade subalgebra functional J' by j ' and e by 1, with the Poisson brackets {j'(x),j'(y)}=f'kjk(y)8(x-y)-^k8,'8'(x-y).
(3.11)
The method of hamiltonian reduction involves constraining currents associated with nilpotent elements of the algebra. In the traditional reduction associated with Toda theory or the standard KdV hierarchy one gauged the maximal nilpotent algebra associated with, say, all the positive roots of g. It was then realised that one could generalise this construction by gauging some smaller set of currents, and moreover, that this set could be succinctly labelled by some su(l, 1) embedding. Since we are interested in bosonic positive-definite W-algebras, we may assume that the su(l, 1) embedding is integral. Non-integral embeddings result in bosonic fields of half-integral weight and the resulting W-algebras are not positive-definite. Let us consider some modified Cartan-Weyl basis for g, g= g eheg+.
(3.12)
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P. Bowcock, G.M.T. Walts / Quantum W-algebras
79
Here g±=®C£±a,
h=®CHi,
(3.13)
with the commutation relations [Ea, E~a] = (2/a2)a'H',
[//'', EP]=^EP.
(3.14)
One can always conjugate any su(l, 1) subalgebra of g so that 7 + e g+, I0 e h , 7_e g~ where I+, I_, J0 are the usual raising, lowering and diagonal basis of su(l, 1). We may write I0 = pvH. If we use the standard normalisation for the su(l, 1) algebra, [/0,/±]=±/±,
[ / + , / _ ] = V2/ 0 ,
(3.15)
then we may define the characteristic of the su(l, 1) embedding to be ( p v e , p v - e i ) , where e; are the simple roots of g. It is a fact that the entries of the characteristic are 0, \, 1. For integral embeddings they must either be 0 or 1. The standard reduction is associated with the principal embedding whose characteristic contains all ones. We may grade g with respect to the p v • H eigenvalue as 8=® m g m -
(3.16)
The elements of g which are highest weight states for this su(l, 1) action form a commuting subalgebra of g. We denote these highest weights by E(ei\ and the corresponding lowest weights by E(~e,\ The highest weights are annihilated by / + and the lowest weights by /_. We denote the subalgebra © n > 0 g n by p + and the subalgebra © n>0 g„ by n + c g + . Similarly for p~, n". For the standard reduction associated with the principal reduction, n * = g *. Since G acts on g*, we may perform a classical hamiltonian reduction [27] with respect to the subgroup N~, where N" is the subgroup of G which has the nilpotent subalgebra n~ as its Lie algebra. In this procedure one chooses an image of the momentum map TT and the phase space consists of equivalence classes under the residual symmetry of the inverse image of n. Here rr is essentially the projection map g->n + . We can choose the image of TT in such a way that the inverse image consists of elements of g* of the form (b(z)+I+,l),
(3.17)
where M z j e p " . We call this space M. The action of N~ is now an equivalence relation on M. From the form of M, we may choose coordinates on this space to be gauge invariant differential polynomi-
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als of the entries in the matrices b(z). In particular, there is a unique gauge transformation Ad£ = exp(ad*) with n e fi~ which gives N~1(b + I+)N + kN-ldN = I++ J^W„Eln\
(3-18)
n
where Ein) span the kernel of /_. To show this gauge transformation is unique, take components in gm. As a result, the entries of n are uniquely determined polynomials in the entries of b(z). The Poisson bracket structure on gauge invariant functionals
{^ *},-<«. ft*. V U > '
(3-19)
where ; = VQ
(3.20)
for all q e M. Thus VQ<j> is determined up to an element of n"; one such choice is Vq<j> = dq
+ /+,l)~{^.(g0)},
(3.21)
where N-\gQ
+1 +)N + kN~l dN = I++ X X £ < n ) .
(3.22)
n
Since this gauge transformation is unique, the polynomials Wn{gQ) are a choice of coordinates on the manifold M = M/N ~. It can also be shown [8] that the Poisson bracket structure on g and M are compatible in the sense that {/x*0, M *^}=^*{^, * } ,
(3.23)
where fi*
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P. Bowcock, G.M.T. Watts / Quantum W-algebras
81
4. Linearised Poisson brackets for classical W-algebras We are now in a position to calculate the Poisson brackets of the W-algebra given by the Drinfeld-Sokolov reduction associated with some Lie algebra g and a particular integral su(l, 1) embedding. The purpose of this section is to show that the finite subalgebra and su(l, 1) embedding of sect. 2 associated with this W-algebra coincide with those chosen to specify the reduction. This will demon strate the existence of the classical W-algebra associated to each such pair. We can check this in this case by using the expressions we deduced in the previous section for the W-algebra Poisson brackets. The finite subalgebra is simply the 'linearised' vpa for the generating fields, so we will only need to calculate the Poisson brackets to linear order in the fields. This is the feature which makes the calculation tractable. We need to calculate the Poisson brackets of the functionals &, ^=j^Lf"{z)W{z),
(4.1)
where W is a W-algebra field and now z is a complex coordinate. If we denote the W-algebra fields of weight 4 a = a + 1 by W, then the modes W£ are given by ^ for f(z) = zm+a. We shall not differentiate between fields of equal conformal weight, to avoid proliferation of indices. From (3.18) we know that the gauge-in variant fields correspond to the lowest weights of the sl(2) embedding. If we wish to identify a particular field of a given weight, then we shall use the notation W[^], where X is a generator g which is a lowest weight of the sl(2). The results of the last section tell us that the Poisson bracket algebra is given by fc
^ } = / ^ T r ( ; ( z ) [ d ^ , d ^ ] ) + A : / ^ T r ( d ^ ( d ^ ) ' ) . (4.2)
If we are interested in the term in this Poisson bracket which is linear in the fields W, then we clearly only need to calculate d\V£ to linear order in thefieldsW. Consider the arbitrary element of the space M to be of the form j = b(z)+I+.
(4.3)
We may decompose g with respect to the sl(2) subalgebra to find the highest weights of this sl(2) which we shall denote by E". Then bases for g, g~ and n~ are given by g=® a «, 2 -o + 1 C£'' a ,
(4.4)
g--e < ,ef_ + 0 ! CE , -- >
(4.5)
n~ = e a 0f_ o C£'' a .
(4.6)
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P. Bowcock, GMT. Watts / Quantum W-algebras
where £,'-° = ad , '(/ + )o£ a .
(4.7)
Then we may write a
E/''-fl(z)£*'••.
] = I+ + Jo = I++L
(4.8)
a 1=0
We shall now consider a gauge transformation of the form /' = exp(ad(/))» (; + **),
(4.9)
where / is some current in n". If / is the transformation which puts j into the highest weight gauge, then / is defined implicitly as a polynomial function in the components of ; 0 and their derivatives, by j'=jw
= I++'£lVaEa.
(4.10)
a
An important step in the argument is to decompose / into components which are homogeneous in the components of j 0 , and further into components of E',a:
/=E/°'\
(4.11)
j
' = E E Zl'UaE--\ j
a
(4.12)
i=0
where l"^rb is homogeneous in ; 0 of degree p. If we decompose the gauge invariant functionals W into homogeneous pieces Wp]a of degree p, then upon substituting (4.12) into eq. (4.10), we obtain W , i"=; 0 - fl -jfc(/ 1 l 0 ")', w,2|« = T r J £ 2..«[ / ( i),
(4.13)
(;0+i[/<»,/ + ])])-*(/2l°«)',
(4.14)
where a
/'"•°= P
/2"'-,-« =
{-kd)p-i-xj'>a,
£ «i +
fl
E(A:a)''-''(-l),'[Tr(£2"-''-a[/(,>,(/o
P-1
(4.15)
I
+ M ' ( , ) . ^ ] ) ] ) ] - ( 4 - 16 )
454
P. Bowcock, G.M.T. Watts / Quantum W-algebras
83
We have chosen a normalisation for the sl(2) highest weight vectors Tr(£ 2fl,fl £ 0 - a ) = l,
(4.17)
For simplicity we have used notation which assumes that there is a unique field of each weight, but the generalisation is straightforward. The normalisation (4.17) means that the generators I±, [I+, I_] obey su(l, 1) commutation relations with nonstandard normalisation factors. We can now deduce df? for %? = / W(z)f(z)dz/2iri. This will in general be a function of the entries j " , and since we are interested in the Poisson brackets of gauge-invariant quantities, we may simply substitute j by j w , after we have evaluated dW. This makes the evaluation of dW very easy since l'u" = 0, j ' a = 8'0W. We can thus identify the terms which will contribute to d ^ where & = ffWa. Using the notation {aj
b
j } =Tr[E>°[Ekb,
k
E'n),
(4-18)
we have
(kd)pfdjia
cur-/ E
+jaLLbL
E ikay-'-llw<(-k9)'f]l2a_
b a
i)dr*. (4.19)
Using Trij djia)=jia, we can easily see that d / " = (-0'£ 2fl ~' ,fl . We are really only interested in the case f = za+m where & = W^, and so finally we obtain a
<^m= E ( a + w ) , ( - ^ ) ^ m + f l " ' £ ' 2 a _ ' , f l i-0
+ E °E C£ b,c i = 0 Q-0
xlbn [0
„a . 2a -i
E*(-1),+>5>-'(wtyz"*') j - \
c
m)
\E2'-i-i*ki+i-x
+ 0(W2),
(4.20)
where we denote (b)(b-l)...(b-c
+
l)by(b)e.
(4.21)
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84
P. Bowcock, GMT. Watts / Quantum W-algebras
We are now in a position to evaluate the Poisson brackets of the modes W£ to linear order in the fields. We shall decompose AW into its homogeneous pieces, as dW° = d ^ ( 0 ) + d ^ ( 1 ) + 0 ( W2).
(4.22)
Using eq. (4.2) we see that the terms which contribute to the linear piece of the Poisson bracket are
fc ^ = * / ^ T r ( d P ^ ^ ^ + */^Tr(d^'>(d^<0))')
+ kj^Yx^W^dW^) + 0(W2).
(4.23)
O'Raifeartaigh et al. [11,25] have shown that L =aW[I_] + ZaP"W[Ua]2 is a Virasoro algebra for the system we have described, where W[I _] is the field corresponding to the representation of the embedded sl(2) itself, and W[Ua] are fields corresponding to the singlets in the decomposition of g with respect to the embedded sl(2). The fields Pf[£ 0,a ] transform as primary fields of weight a + 1 w.r.t. this Virasoro algebra. The central term in the Virasoro algebra is generated purely by the field W[/_], since we have already shown that there are no central terms in the Poisson brackets of composite fields. In the case W=W[I_], eq. (4.20) becomes exact, dW[I_]m=zm
+i
[l+, [/ + , /_]] - * ( m + l ) z " [ / + , / _ ] .
(4.24)
We can now evaluate the Poisson bracket [ni-]m^U-]n}=k\(m-n)lV[I_]m+n
+ k3m(m2-l)Sm+n,
(4.25)
which corresponds to a rescaled Virasoro algebra. In eq. (4.25) A is defined by [/+,[/+,/_]]=A/+.
(4.26)
Thus, if we re-scale W^/.] to return (4.25) to the standard normalisation, we recover c = 12&/A2 = 6k(p v ) 2 where p v defines the su(l, 1) embedding. Thus the Poisson brackets (4.23) represent a W-algebra. To establish that this is a positive-definite W-algebra, note that the first term in eq. (4.23) corresponds to the central term and is easy to compute; /J T ^ E L(a+m)i(b 2iri ,._„,._„ x1x{E2"-i'aE2b-i-b).
+ n)u+1i-k)i+'
+
l m+ +a+l
z "
'-^-i
456 P. Bowcock, GMT. Watts / Quantum W-algebras
85
The trace in this term gives 8ab8f8b{- l)a and so we get now = JfT^8ab(a+m)a(a+n)a
+
+ 1z'»
''-lk2<'
+
\-l)a
LTTl
= -k2°+lm(m2-l)...(m2-a2)8°b8m+nfl.
(4.27)
Thus the algebra (4.24) is a positive-definite W-algebra since the central term is non-degenerate. Following the theoretical framework we laid out before, we can now restrict our attention to the algebra of the modes of the vpa. For the vpa the central term vanishes and the second term in eq. (4.24) is now easy to compute.
f^:T(iw(z)[iW«»,iW»])
•ftiT'[{^Z)E-) a
X
b
£ (a +m)i(-k)izm+a-'E2a-i-a,
£ (b+
i-o
y-o
= E^
+
„ t
c
E (a + m)i(b + n)j(-k)i+i
n)j(-k)Jzn+b-iE2"-i-b
Tr(£<[£ 2 <-'*,
*'+/
E2b~^])ki+\
i-0j-0 min(a+b,b + c)
= Y,Wm+n c
x/C
L
(a + m)(fl+6_A)(fe + «) (A _ c)
A — max(i>,c)
^
Wa+6_c
°
\0 a-b + k 2b + c-\j remembering that the trace gives a delta function 8(c + a + b, 2a + 2b -j - i). The third term is more complicated,
Ti-kJ-^TTidW^dWWJ) = / ^ r E ^ + m - / ( « + m) / (-l) /
¥(-i)p+i3i(w'(z)diz>+b)
xLE E d,c i-0
X
(o
p-0
2b-i
j - \ C ] 2 2 i p jTr(E ''-'-'E ^-^)k ^'
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86
P. Bowcock, GMT. Watts / Quantum Walgebras
The last trace gives us 8(1, a), 8(a, c), 8(j, c-p) and so we now get 7 - 3 - / ^ T E E ' ' E C - ! ) " * " 9->(Wd(z) 'z'+fc) J
llTl
{t
d i-0
p-0
a
2b-i
p}^-'(a+m)m
= / T ^ E E"E(-I)"(*"-^")(^,'+*)»"'(^ J
2 m
d ,--o p - o
x{o 26*-,■ ;}*' + a -'(«+«o. H2
6-1a-1
/ ^ - E E E(-i)' 3 2ir
'_m +p —a +p + b — i
' ,--o p-o
x(a+m)a(m)(a-p)(n+b)U)Wd(z){d0
6 2£>
_j.
*}/c i+2a —n
This last term in curly braces represents a trace, which gives us 8(i, b+p -d - c), and so we get, with A = 2b + d - p, 2b + d d
A=6+d+l
y/rf s
\0
A
^
a-fc + A 2b +
\ka
+ b-d
d-\)
b+d+n
= EW» + » d
E
(a+m) (a+fc _ A) (fc + n ) ( W )
A=fc+d+l
*{o , - J + A
»+*
(428
>
where we used the fact that for A > b + d + n the second of the two Pochhammer symbols vanishes. By similar reasoning we can evaluate the fourth term of eq. (4.24) and when we put them all together we obtain for the vpa terms {W£, \m\
{w:,Wnb}=Z,W^+n c
*(n
E
(«+m)(. +fc -A)(6 + n)cA-d
A = max(c,6 —m)
1
.
,..
&
vU
a+6
"c + 0(^2).
(4.29)
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P. Bowcock, G.M.T. Watts / Quantum W-algebras
87
This establishes the linearised vpa commutation relations. We can now compare them with the commutation relations of g in a particular basis. We know that W[I_]±l0 form the sl(2) embedded inside g, and so it is convenient for us to take the modes of the (quasi-)primary fields W£ to correspond to the representation of sl(2) with highest weight E". If we take the correlation to be W^ = E"-m-ttf{a,m)
(4.30)
where f(a, m) are some constants, then the fact that W[I_]±, sl(2) tells us that /(a, m) is given by f(a,m)=»(a)(-k\)"+m(a
0
are the embedded
+ m)\/(2a)\,
(4.31)
where A is defined in eq. (4.26). We may now evaluate the commutator of two of these elements of g, and we find that we recover the commutation relations (4.29) exactly for /x(a) = (2a)!, and so WZ = Ea-m'a(-kk)a+m(a
+ m)\
(4.32)
completes the identification of the vacuum preserving modes of the W-algebra with the algebra g itself, up to quadratic terms in the fields W. Moreover, the modes Lu L 0 , L_, are clearly associated to / + , / 0 , /_. If one examines the commutation relations more carefully and normalises the algebra correctly accord ing to eq. (2.7), one sees that indeed the couplings f°b are CXI) in the central charge, thus bearing out our expectations for a classical W-algebra. This clarifies the relationship between the linearised vpa and the generalised Drinfeld-Sokolov reduction. It follows that there exists at least one classical W-algebra for every g and every integral su(l, 1) embedding. If this W-algebra is unique, then the Drinfeld-Sokolov reductions completely saturate the possibilities for bosonic integrally weighted W-algebras. We return to this point in the conclu sion.
5. Lie algebras and si (2) embeddings In this section, we shall use the theory of finite Lie algebras and their three-dimensional subalgebras together with what we have learnt in the preceding sections to look at various aspects of reductive W-algebras. We briefly comment on a possible relation between automorphisms of the linearised vpa and homomorphisms of the W-algebra. Then we give a complete list of positive-definite W-alge bras without Kac-Moody components by classifying all su(2) embeddings of semi-simple Lie algebras with trivial centre. We enumerate the algebras which, in addition, contain no generating spin-2 fields besides the Virasoro algebra.
459
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P. Bowcock, GMT.
Watts / Quantum W-algebras
First, let us consider the case where the su(l, 1) is not a maximal subalgebra of g; that is there exists some algebra h such that su(2) c h c g. In the limit that c -* oo we expect that some subalgebra of generating fields which includes the Virasoro algebra closes. This, however, does not imply that these generating fields generate some W-algebra associated with su(2) c h, which is a subalgebra of the W-algebra associated with su(2)cg. As an example we can consider the algebra WA3 associated with the principal su(2) embedding in A 3 which is generated by fields of weight 2, 3, and 4. However, we can write su(2) c B 2 c A , in this case, where the spin-2, 4 fields are associated with the first embedding. An inspection of the operator product expansion of the spin-4 field with itself reveals that it contains a term which is the composite field associated with the square of the spin-3 field. The coupling to this term vanishes in the limit that c -»oo, but the spin-2, 4 algebra does not close on itself for finite central charge, and is distinct from WB2 which we would associate with the first embedding. However, we suspect that a weaker statement is true. If T is an automorphism of g for which h is the stable subalgebra, this gives an automorphism of the vacuum preserving modes in the limit that c->°o. Since T(L) = L it defines some homomorphism which maps a generating primary field to some linear combination of primary fields of the same weight. We shall assume that this can be used to define a homomorphism on the Verma module of the W-algebra associated with g. The subalgebra which is stable under this homomorphism will contain only those generating fields associated with h, but will in general require additional generators which will be composites in all the generating fields of the algebra. In the example above, if we choose the simple roots of A 3 to be e, - e2, e2 - e3, e3 - e4 then the automorphism which preserves its B2 subalgebra is given by ex -» -e4,
e2-> - e 3 ,
and the induced homorphism on the W A 3 algebra is simply spin-3 -> -spin-3. The subalgebra which is stable under this homomorphism is the smallest closed algebra containing the spin-2, 4 fields. If it is the case that the resulting W-algebra does not have a good classical limit, which we know to be true in the case that we reduce a super W-algebra in this way, then this sort of consideration may provide a powerful tool for constructing deformable algebras which do not have a good classical limit. As a second topic of interest, we shall now give a complete list of the possibilities for bosonic W-algebras with good classical limit which have no Kac-Moody components. If we want there to be no spin-1 fields in the fields in the W-algebra we require that there are no singlets in the decomposition of the adjoint representation of g under su(l, 1). Alternatively, if we decompose g w.r.t. the / 0 member of the preferred sl(2), we may express this by saying that dim gj = dim g0, or by saying that the centraliser of su(l, 1) in g is zero. We classify all the examples of su(l, 1) embeddings where this is so.
460
P. Bowcock, G.M.T. Walls / Quantum W-algebras
89
First we need to borrow some notation from Dynkin [28]. For ease of exposition we shall revert to the real compact form of the Lie algebras, since the form of the algebra is not important for the argument. A regular subalgebra of g is a subalgebra whose root system is simply a subset of the root system of g. A subalgebra of g is called an R-subalgebra if it is contained in some proper regular subalgebra of g. Otherwise it is called an S-subalgebra. S-subalgebras have the properties that (i) they are integral; (ii) dim g, = dim g0. Thus the condition that an su(2) subalgebra by an S-subalgebra is sufficient for producing a W-algebra without Kac-Moody components, but as it turns out it is not necessary. In the other cases there must exist some proper regular subalgebra of g which contains su(2) and moreover its rank must be equal to that of g, since otherwise it is easy to prove that some member of the Cartan subalgebra will commute with it. The classification of all su(2) subalgebras of the exceptional Lie algebras whose centraliser vanishes has been given in ref. [28]. We reproduce these results in table 1. The algebra g is given in the first column. The second and third column give the index and characteristic specifying the su(2) embedding while the fourth summarises the weights (with degeneracies in parentheses) of the generat ing fields of the corresponding W-algebra. The next column gives the minimal subalgebra(s) of g which contain the su(2). A P in the final column indicates that the embedding is principal. We now deal with the remaining classical examples. (i) su(«). The only su(2) S-subalgebra of A„ is given by the principal embed ding. Any other candidate is a subalgebra of one of the maximal regular subalge bras of su(rc) and hence we can write su(2)csu(p) © su(<7) © u(l)csu(/i). Fur thermore it is clear that su(2) csu(p)© su() so that the u(l) factor commutes with it. Thus no other algebra has zero centraliser. (ii) sp(n). Again the only su(2) S-subalgebra of sp(«) is the principal subalgebra. For the other subalgebras we may write su(2)cc(/?,)®c(p2)cc(rt),
Pl+p2
= n.
(5.1)
If the copy of the su(2) is not principal in one of the c(/J,) we can decompose this further until we have su(2)cc(/>1)®-"®c(/>,.)cc(").
LPj = n,
(5.2)
i
where the copies of su(2) in each c(p,) are principal. We can decompose the adjoint representation of c(«) with respect to this direct sum of dpt) within which the su(2) are principal. We find that adj c(n) = (adj c(p,) ® 1 ® ... ® 1) © ... © (1 ® ... ® 1 ® adj c(p,)) © M l ® ... 1 ® 2pj ® 1... 1 ® 2pk ® 1... ® 1,
461
P Bowcock, GMT
90
Watts / Quantum W-algebras TABLE 1
The classification of all su(2) subalgebras of the exceptional Lie algebras whose centraliser vanishes (see ref. [28]) g
Cha racteristic
Index
E8
40
0
C)
0
1
E8
88
1
0
0
0
E8
120
0
I
0
0
Eg
160
1
0
0
E8
184
0
0
0
E8
232
1
I
0
0
E8
280
1
()
1
0
E8
400
1
1
0
E8
520
1
0
1
E8
760
1
1
1
E8
1240
1
1
1
E7
39
0
0
E7
63
0
0
E7
111
1
0
E7
159
0
1
E7
231
1
E7
399
1
E6
36
1
E6
84
1
E6
156
1
F4 F4 F4 F4 G2 G2
12 36 60 156 4 28
0 0 1 1
1 1 1 1 0 0 1 1 1 1 1 1 1 1
Spins
h
Spin-2
0 0 1 0 1 0 1 0 1 0 1 0 1 0 1 0 0 1 0 1 1 1 1 0 1 0 1 0 0 1 0
0
0
2(10), 3(10), 4(10), 5(6), 6(4)
A^© A^
0
0
0
0
E6® A 2 B 4 ®B 3 B 5 ®B 2
0
0
0
1
0
1
0
1
0
1
1
1
1
1
1
1
2(4), 3(4), 4(5), 5(3), 6(6) 7(2), 8(3), 9 2(3), 3, 4(5), 5(3), 6(3) 7(3), 8(3), 9, 10(2) 2(4), 3,4(2), 5(3), 6(3) 8(3), 9(3), 10(2), 12 2(3), 3, 4, 5, 6(4), 7(2) 8(3), 9, 10, 11, 12(2) 2(2), 3, 4(2), 6(3), 7 8(2), 9(2), 10, 11,12(2), 14 2, 3, 4, 5, 6(2), 8(3) 9, 10(2), 12(2), 14, 15 2(2), 5, 6(2), 8, 9, 10(2) 12, 14(2), 15, 18 2, 4, 6, 8, 9, 10, 12(2) 14, 15, 18, 20 2, 6, 8,10, 12, 14, 15, 18 20,24 2, 8, 12, 14, 17, 20, 24, 30
0
0
2(6), 3(4), 4(5), 5(3), 6(3)
0
1
0
1
1
1
1
1
1
1
1
2(4), 3(2), 4(3), 5(2), 6(4) 7,8 2(2), 3, 4(2), 5, 6(3) 8(2), 9, 10 2(2), 4,5, 6(2), 8(2) 9, 10, 12 2, 4, 6(2), 8,9, 10 12,14 2, 6, 8,10, 12,14, 18
1
0
1
2(3), 3(3), 4(2), 5(2), 6(2)
A5®A,
0
1
1
2, 3,4,5,6(2), 8, 9
C4,G2
V*
1
1
1
2,5, 6, 8, 9, 12
F,
t^P
*■
0 1 1 1
1 1
5. *
0 1
2(6), 3(4), 4(2) 2(3), 3,4, 5, 6(2) 2, 3, 4, 6(2), 8 2, 6, 8,12 2(3), 3 2,6
A j© A | ^.3© A j
> >
0 0 0 1
*■
E7® Aj
B 6 ®A, E7®A, B7
V
E7®A, E8
V
E8
*
Eg
f ?
A5®A2 D 6 ®A, D6®A, D 6 ©A, F 4 ®A, E7
f
E7
*?
B4 F4 A,®A, G2
V
*? *?
462
P. Bowcock, G.M.T. Watts / Quantum W-algebras
91
where we have denoted the 2p dimensional representation of c(p,) by 2p,. The adjoint representation of c(p,) contains no singlets when decomposed with respect to a principal su(2). The 2p, representations decomposes into a single irreducible representation of this su(2) and so the tensor product . . . 2p, ® ... 2 p y . . . decom poses with respect to the diagonal su(2) to give \2pl - 2pf | © . . . © 2pl-.+ 2pj. From this we can see that adj c(n) contains a trivial representation of the diagonal su(2) subalgebra if and only if Pj=pk for some ;' # k. (iii) so(n). The argument in this case is a little more involved. b„ again possesses no other su(2) S-subalgebras other than its principal. d„ possesses int[j(« - 2)] S-subalgebras, but in fact none of these are maximal (not even the principal) and they correspond to the embeddings su(2) c s o ( p ) © so(^)cso(2«) where p + q = 2n and p, q are both odd. For our purposes it will be convenient to think of so(4) as simple. Its principal subalgebra is maximal. Now starting with any su(2) embedding in so(«) it is straightforward to show that su(2) cso(/>[) ©so(/? 2 ) © ••• ® so(p,) c s o ( n ) ,
(5.3)
where pt = 3, 4, 5, 7, 9 , . . . and the copy of su(2) in each simple ideal is principal. For ffiy so(Pj) to be maximal in so(«) and hence to have trivial centraliser we need that n — T.jPj > 2. Again we can decompose the adjoint representation of so(«) with respect to this direct product of principal su(2) subalgebras and we find that adj so(n) = © 1 ® 1 ® . . . ® adj so( />,) ® 1 ® . . . ® 1 ®jkl ® . . . 1 ®pj ® 1 . . . 1 ®pk ® 1 . . . ® 1, where we have denoted the Pj dimensional representation of so(/?;) by pr Again this will have a trivial representation with respect to the diagonal su(2) if and only if Pj=pk for some / # k. Notice that if one of the p ; = 4, the associated embed ding is non-integral. This is the only example of a W-algebra with no Kac-Moody components which is not positive-definite and can be obtained in this way. The results for su(2) embeddings in classical algebras are summarised in table 2. It is also straightforward to extend the above analysis to search for W-algebras with no Kac-Moody components and no other spin-2 fields than that associated with the Virasoro algebra. If there exists some algebra h such that su(2) c h c g, h is not simple, and su(2) is embedded diagonally in more than one of the simple ideals of h then there exists more than one spin-2 field. This is because the decomposition of the direct product of N copies of su(2) with respect to its diagonal subalgebra contains N spin-1 representations. The cases where no such h exist are easy to read off from the tables, and are marked with a check-mark in
463
92
P. Bowcock, G.M. T. Watts / Quantum W-algebras TABLE 2
Results for su(2) embeddings in classical algebras Index
g
/i(/i + l)(/i + 2) A„
6 n(n + \)(2n + \)
B„
3 n(2n + l ) ( 2 n - l )
c„
3 *(/i-l)(2/i-l)
D„
c„
3 «,(2n, + l ) ( 2 n , - l ) ^
h
Spins 2,3,4,. ..,n + l
A„
2,4,6,. ...In
B„
2,4,6,. ...2n
c,
2,4,6,. . . , 2 / i - 2 , /i
B„
E2,- ..,2n, +
3
Ek -
®/Cni
E/i, = n, n, # n •
+«;+l fly 1 + 1,..,/!, -
i>>
so(AO
/.,(/>,.-l)(n,. + l) ~
E2,.
12
i
I
+ E 2 rn, - 4
i
Eik
/i,-l
"'
2 1
-flyl + 1,...,«,- + «y + 1
■ >;
E 12 +
©, so(n,)
I«,
= /I, /I — 1, /I, ^ fly
i
/I; S 3 , 4,5,7,...
table 1. For the classical algebras, it is clear that only the principal embeddings result in only one spin-2 field. 6. Conclusions In this paper we have found a connection between a general class of W-algebras and finite Lie algebras. A crucial role in our arguments was played by the vacuum-preserving-algebra (vpa) which is the closed subalgebra of modes which annihilate both right and left vacua. For "linear" W-algebras one finds that the vpa contains a finite subalgebra which provides a useful tool for studying the properties of theories invariant under these W-algebras. To extend this idea to more general non-linear quantum W-algebras, it became necessary to consider deformable W-algebras which are defined for a range of c-values in the classical limit c -»oo, and the subclass of algebras which behave 'well' under this limit. A natural criterion which arises is that of positive-definitness of the W-algebra, which essentially ensures that all the fields are important to the structure of the algebra. Reductive algebras are algebras which have positive-definite classical limits. As a result we were able to assign to each reductive W-algebra a finite Lie (super-)algebra and an embedding of su(l, 1). The field content of the W-algebra is encoded in this embedding, with each representation of su(l, 1) in the decomposition of the Lie algebra being associated to one of the Virasoro primary fields; the weight of
464
P. Bowcock, G.M.T. Watts / Quantum W-algebras
93
that field being equal to \{\ + the dimension). By considering the structure of the commutation relations of the W-algebra, combined with the Virasoro Ward identities, we were also able to show that this finite algebra was restricted to be of the form of a direct sum of a semi-simple algebra and an abelian algebra, namely a reductive Lie algebra. This condition places considerable restrictions on the possible field contents of W-algebras and on their commutation relations. As an example of the ideas presented, we considered the classical Poisson bracket algebras of generalised Drinfeld-Sokolov type. The analysis here held out our theoretical predictions-to each such W-algebra we are able to assign a finite Lie algebra and an su(l, 1) embedding in that algebra. Conversely we used the construction to demonstrate the existence of a classical W-algebra associated with each such pair. Our work suggests that W-algebras can be divided broadly into three categories: the reductive algebras considered in this paper, other deformable algebras, and "non-deformable" algebras which are only associative for specific values of c. There are several questions which present themselves concerning each category. Firstly, although we have demonstrated the existence of a classical W-algebra associated with each finite algebra and su(l, 1) embedding, it is not clear as yet whether one can actually find a quantum W-algebra for each such embedding. The quantisation of these models has a lengthy history and is by no means over yet [29-32], although there seem to be good arguments in favour of their existence. If one can find quantum W-algebras which satisfy the conditions of sect. 2, namely having a good classical limit which is positive-definite, then the question obviously arises, are they unique? That is, to each such embedding can one uniquely ascribe a quantum W-algebra? We know of no counterexamples. Our conditions, although they catch many of the W-algebras which have been studied to date which have proven useful in conformal field theory, still exempt many W-algebras. Indeed we present such an exception with fields of spins 2, 4, and 6. In sect. 5 we have presented what we hope will be a useful approach to the study of these algebras, namely automorphisms of Lie algebras which preserve a subalgebra. For the case we presented this was a Z 2 automorphism which pre served the B 2 subalgebra of A 3 . We hope that we can extend this to other cases. Certainly the idea of dividing out by a finite group action is not new, but rather the idea that we may be able to ascribe a W-algebra uniquely to each such action, and even reconstruct the larger algebra from the smaller, is. There are good reasons to believe that the absence of a good classical limit implies strong constraints on the unitary representations of W-algebras, and we hope to return to this and other topics in the future. As even more distant projects we can mention the idea that one may be able to show that each W-algebra which occurs for a specific set of c-values is simply the extension of a deformable W-algebra by primary fields of integer spin. Thus, it may be instructive to look for 'maximal' deformable subalgebras of such W-algebras.
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P.B. would like to thank the DOE of the USA for support under grant number DEFG02-90-ER-40560 and the NSF of the USA under grant PHY900036, and G.M.T.W. would like to thank the SERC of the UK for a research assistantship. G.M.T.W. would like to thank the EFI for hospitality at the initiation of this work. P.B. and G.M.T.W. would like to thank the Institute of Theoretical Physics at the University of California, Santa Barbara, for hospitality, and where they were in part supported by the National Science Foundation under grant PHY89-04035. G.M.T.W. would like to thank Trinity College Cambridge for a Rouse-Ball travelling studentship. We gladly thank H.G. Kausch for many useful conversations during the course of this project. G.M.T.W. would like to thank C.F. Yastremiz for useful comments on the manuscript.
References [1] P. Goddard and D. Olive, Int. J. Mod. Phys. Al (1986) 303 [2] P. Goddard and A. Kent and D. Olive, Phys. Lett. B152 (1985) 88; Commun. Math. Phys. 103 (1986) 105 [3] F.A. Bais, P. Bouwknegt, K. Schoutens and M. Surridge, Nucl. Phys. B304 (1988) 348; Nucl. Phys. B304 (1988) 371 [4] G.M.T. Watts, Phys. Lett. B245 (1990) 65 [5] P. Bowcock and P. Goddard, Nucl. Phys. B305 [FS23] (1988) 685 [6] A. Bilal and J.-L. Gervais, Phys. Lett. B206 (1988) 412; Nucl. Phys. B318 (1989) 579 [7] J. Balog, L. Feher, P. Forgacs, L. O'Raifeartaigh and A. Wipf, Ann. Phys. (NY.) 203 (1990) 76 [8] V.G. Drinfeld and V.V. Sokolov, Dokl. Akad. Nauk. USSR 23 No. 3 (1981); J. Sov. Math. 30(1985) 1975 [9] M. Bershadsky and H. Ooguri, Commun. Math. Phys. 126 (1989) 429 [10] A.Y. Alekseev and S. Shatashvili, Nucl. Phys. B323 (1989) 719 [11] L. Feher, L. O'Raifeartaigh, P. Ruelle, I. Tsutsui and A. Wipf, Ann. Phys. 213 (1992) 1; L. Feher, W-algebras of generalized Toda theories, Dublin preprint DIAS-STP-91-22; F.A. Bais, T. Tjin and P. van Driel, Nucl. Phys. B357 (1991) 632 [12] H.G. Kausch and G.M.T. Watts, Nucl. Phys. (1991) 740 [13] R. Blumenhagen, M. Flohr, A. Kliem, W. Nahm, A. Recknagel and R. Varnhagen, Nucl. Phys. B361 (1991)255 [14] L.B. Dolan, P. Goddard and P.S. Montague, Phys. Lett. B236 (1990) 165; Nucl. Phys. B338 (1990) 529 [15] I.B. Frenkel, J. Lepowsky and A. Meurman, Vertex operator algebras and the monster (Academic Press, New York, 1988); I.B. Frenkel, Y.-Z. Huang and J. Lepowsky, On axiomatic approaches to vertex operator algebras and modules, Yale/Rutgers University preprint, 1989 [16] M. Bershadsky, Commun. Math. Phys. 139 (1991) 71 [17] W. Nahm, Talk given at the Conf. on recent developments in conformal field theory, Trieste, October 1989 [18] P. Bouwknegt, Phys. Lett. B207 (1988) 295 [19] P. Bowcock, Nucl. Phys. B356 (1991) 367 [20] V.S. Varadarajan, Lie groups, Lie algebras, and their representations (Prentice-Hall, 1974) [21] A.A. Belavin, A.M. Polyakov and A.B. Zamolodchikov, Nucl. Phys. B241 (1984) 333
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[22] P. Goddard, Meromorphic conformal field theory, in Infinite dimensional Lie algebras and Lie groups, CIRM-Luminy July Conf. on Infinite dimensional Lie algebras and Lie groups, Marseille 1988, ed. V.G. Kac (World Scientific, Singapore, 1989) [23] V.G. Kac, Commun. Math. Phys. 53 (1977) 31 [24] P. Goddard and A. Schwimmer, Phys. Lett. B214 (1989) 62 [25] L. O'Raifeartaigh and A. Wipf, Phys. Lett. B251 (1990) 361; L. O'Raifeartaigh, P. Ruelle and I. Tsutsui, Commun. Math. Phys. 143 (1992) 333 [26] M.F. de Groot, T.J. Hollowood and J.L. Miramontes, Generalised Drinfeld-Sokolov hierarchies I. IASSNS-HEP-91/19; N. Burroughs, M.F. de Groot, T.J. Hollowood and J.L. Miramontes, Generalised Drinfeld-Soko lov hierarchies II IASSNS-HEP-91/42; N. Burroughs, Coadjoint orbits of the generalised sl(2), sl(3) KdV hierarchies, IASSNS-HEP-91/67 [27] V.I. Arnol'd, Mathematical methods of classical mechanics (Springer, New York, 1978) appendix 5 [28] E.B. Dynkin, Transl. Am. Math. Soc. Series 2, 6 (1957) 112 [29] A. Bilal and J.-L. Gervais, Phys. Lett. B206 (1988) 412 [30] V.A. Fateev and S.L. Lukyanov, Sov. Sci. Rev. A15 (1990) 1 [31] H. Kausch and G. Watts, Quantum Toda theory and the Casimir algebra of B 2 and C 2 , Durham University preprint DTP-91-35 (1991), Int. J. Mod. Phys. A, to appear
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Reprinted with permission from Communications in Mathematical Physics Vol. 160, pp. 317-332,1994 © 1994 Springer-Verlag
The Relation Between Quantum W Algebras and Lie Algebras Jan de Boer 1 *, Tjark Tjin 2 ** 1
Institute for Theoretical Physics, Princetonplein 5, P.O. Box 80.006, 3508 TA Utrecht, The Netherlands 2 Institute for Theoretical Physics, Valckenierstraat 65, 1018 XE Amsterdam, The Netherlands Received: 19 February 1993
Abstract: By quantizing the generalized Drinfeld-Sokolov reduction scheme for ar bitrary sl2 embeddings we show that a large set W of quantum W algebras can be viewed as (BRST) cohomologies of affine Lie algebras. The set W contains many known W algebras such as WN and W\ . Our formalism yields a completely algo rithmic method for calculating the W algebra generators and their operator product expansions, replacing the cumbersome construction of W algebras as commutants of screening operators. By generalizing and quantizing the Miura transformation we show that any W algebra in W can be embedded into the universal enveloping alge bra of a semisimple affine Lie algebra which is, up to shifts in level, isomorphic to a subalgebra of the original affine algebra. Therefore any realization of this semisimple affine Lie algebra leads to a realization of the W algebra. In particular, one obtains in this way a general and explicit method for constructing the free field realizations and Fock resolutions for all algebras in W. Some examples are explicitly worked out.
1. Introduction W algebras were introduced by Zamolodchikov as a new ingredient in the classifica tion program of conformal field (CFT) theories [1] (for a recent review see [2]). As is well known such a classification would correspond to a classification of all possible perturbative groundstates of string theory. However CFT and W algebras have been shown to be related to several other areas of research as well such as integrable sys tems, 2D critical phenomena and the quantum Hall effect. W symmetries are therefore an interesting new development in theoretical physics and it is the purpose of this paper to provide a step towards understanding their meaning and structure. The point of view that we shall develop in this paper is that the theory of W algebras is closely related to the theory of Lie algebras and Lie groups. The * e-mail: [email protected] * e-mail: [email protected]
468
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J. de Boer, T. Tjin
construction of W algebras as Casimir algebras (with as a special case the Sugawara construction), and the coset construction [3,4] are examples of such a relation, but unfortunately these have some serious drawbacks. We therefore take the Hamiltonian or Drinfeld-Sokolov (DS) [5,6] reduction perspective which for classical W algebras has been extremely successful. The DS reduction approach starts with the observation that certain Poisson algebras encountered in the theory of integrable evolution equations can be considered to be classical versions of the W algebras first constructed by Zamolodchikov [7]. Drinfeld and Sokolov had already shown that these Poisson algebras are reductions of Kirillov Poisson structures on the duals of affine Lie algebras thus providing a relation between Lie algebras and W algebras. A first attempt to quantize the classical W algebras found by Drinfeld-Sokolov reduction (nowadays called WN algebras) was made in [8]. There the Miura transformation was used to realize the generators of the classical WN algebra in terms of classical free fields. The algebra was then quantized by making the free fields into quantum free fields and normal ordering the expressions fo the W generators. In general this is not a valid quantization procedure however since it is by no means clear that the algebra of quantum W generators will close. In fact it only closes in certain cases [2] (which are of course the cases that were studied in [8]). Since DS reduction is in essence Hamiltonian reduction in infinitely many dimensions it is possible to apply the techniques of BRST quantization in order to quantize the classical WN algebras. This was first done in [20] for the special case of die Virasoro algebra and the WN case was solved by Feigin and Frenkel [16]. Even though WN algebras have an appealing description as BRST cohomologies of affine Lie algebras the quantum DS method is still rather limited since WN algebras are by far not the only W algebras. The quantum DS reduction leading to the by now well known W3(2) algebra [9,10] was however the first indication that DS reduction can be generalized to include many other W algebras. In [11] it has been shown that to every sl2 embedding into the simple Lie algebra underlying the affine algebra there is associated a generalized classical DS reduction of this affine algebra leading t o a W algebra. The fact that one considers sl2 embeddings is closely related to the fact that one wants the reduced algebra to be an extended conformal algebra (i.e. it must contain the Virasoro algebras as a subalgebra and the other generators must be primary fields w.r.t. this Virasoro algebra). Since the numer of inequivalent sl2 embeddings into sln is equal to the number of partitions of the number n the set of W algebras that can be obtained by DS reduction increased drastically. The WN algebras turn out to be associated to the so-called "principal" sl2 embeddings. The Polyakov-Bershadsky algebra W^ is associated to the only nonprincipal sl2 embedding into sl3. The reductions considered in [ 11 ] are clasical and it is the purpose of this paper to quantize them. The usual formalism developed in [16,20] constructs the W algebra as the commutant of certain screening operators which is rather difficult to generalize to arbitrary sl2 embeddings. The main reason for this is that it is difficult to find a complete set of generators of this algebra for arbitrary sl2 embeddings (one has to make use of character formulas to check if one has obtained all generators. These characters are however not known in advance). Also it makes use of free field realizations of the original affine Lie algebra which means that one obtains, in the end, the W algebra in its free field form. If the W algebra has affine subalgebras this will therefore get obscured by the not very transparent free field form. In this
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Relation Between Quantum W Algebras and Lie Algebras
319
paper we therefore use the formalism that was developed in [13] to quantize finite W algebras. It turns out that this formalism still works, with some modifications, in the infinite dimensional case considered here. Let us now give an outline of the paper. In Sect. 2 we quantize the generalized DS reductions of [11]. This is done by the same spectral sequence calculation that was used in [13]. We also introduce the quantum Miura transformation for arbitrary sl2 embeddings and show how to obtain free field realizations for arbitrary W algebras. In Sect. 3 we briefly discuss the conformal properties of the quantum W algebras obtained in Sect. 2. Furthermore a general formula for the central charges of the W algebras in terms of the level of the affine Lie algebra and the defining vector of the sl2 embedding is given. In the last section we consider some examples in order to illustrate the general procedure. We end the paper with some comments and open problems.
2. Quantization Let {ta} be a basis of the Lie algebra g = sln. The affine Lie algebra g associated to g is the span of {J£} and the central element K. The commutation relations are given by where gab is the inverse of gab = Tr(ta«b) and [ta,tb] — flbtc. As usual we use gab to raise and lower indices. Let (&kg{k € C) be the universal enveloping algebra of g quotiented by the ideal generated by K - k. It was shown in [11] that one can associate to every sl2 embedding into g a Drinfeld-Sokolov reduction of g leading to a classical W algebra. We shall now quantize these algebras. Let {tQ,t+,t_} be an sl2 subalgebra of g, then one can decompose g into eigenspaces of the operator adto 9= ©
& ,
(2-2)
where gk = {x e g \ [t0,x] = kx}. This defines a gradation of g which is in general half integer. However, it was shown in [12, 13] that in those cases where the grading contains half integers one can replace it by an integer grading which in the end leads to the same Drinfeld-Sokolov reduction. This is done by replacing t 0 by a certain element 6 of the Cartan subalgebra which has the property that the grading w.r.t. the operator ad6 is an integer grading (for some basic facts on sl2 embeddings and the explicit construction of 6 given an sl2 embedding see the appendix). Without loss of generality we can therefore assume that the gradation (2.2) is integral. The algebra g now admits a triangular decomposition into a direct sum of a negative grade piece, a zero grade piece and a positive grade piece denoted by g_, g0 and g+ respectively. Under the adjoint action of the sl2 subalgebra {t0, t±}y g decomposes into a direct sum of sl2 multiplets. Let us choose the basis {ta} such that all elements ta are basis vectors of some s/2 multiplet. Of course this means that all ta are homogeneous w.r.t. the gradation. From now on we let latin indices a, b,... run over the entire basis of g, Greed indices a, (3,... over the basis of g+ and barred Greek indices a, f3,... over the basis of g0 © g_ (i.e. Xata + A % = Xata).
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We now come to the constraints. Since the sl2 subalgebra {t0,t±} is a triplet under its own adjoint action there must be some a + such that t+ = Ata. . Define the character x of g+ (where g+ is the affinization of g+) by putting x(^n) = A6a'a+6n+l 0 . The constraints one imposes are then J" = x(J%)- These constraints are first class [11] for integral gradings which means that one can use the BRST formalism. Thereto introduce the fermionic ghost variables c", b" with ghost numbers 1 and - 1 respectively and relations c^b^+b^c^ = 6ap6n+m0. The algebra generated by these ghost variables is the Clifford algebra Cl(g+ <S> *). As usual one then considers the algebra Qk = ^kg <8> Cl(g+ © g*). For calculational purposes it is convenient (as is standard practice in conformal field theory) to introduce the following "basic fields" Ja(z) = J2 JnZ~n~x; ca(z) = ^Qz~n\ba(z) n
= J2^nz~nl-
I* ' s
we
n
' l known that the commutation relations in
n
Qk can then be expressed in terms of the operator product expansions (OPE), Ja(z) Jb(w) =
UQab
fab
y
^2 + - i £ — Jc(w) + ... , (z — wY z—w
ca(z)b^(w) = — 2 - . z- w
(2.3) (2.4)
Now inductively define the algebra of fields F(Qk) as follows: Ja(z),ca(z), ba(z) are elements of F(Qk) with "conformal dimensions" A = 1,0,1 respectively; if A(z), B(z) e F(Ok), then aA(z) + 0B(z) e F(Qk); if A(z) is an element dA of F(Qk) of conformal dimension A, then — (z) is also an element of F(!?fc) and has conformal dimension A + 1; if A(z),B(z) are elements of F(Qk) of conformal dimensions AA and AB respectively, then the normal ordered product (AB)(z) = A_(z)B(z) ± B(z)A+(z) (where one has the minus sign if A and B are fermionic) is also an element of F(Ok) and has conformal dimension AA + AB. Here A_(z) = £ Anz~n~A^ and A+(z) = A(z) - A_(z). We say that F(f2k) n<-AA
is "generated" by the basic fields. Note that F(f2k) c ^kg^.z,z~l\ The algebra F(Qk) is graded by ghost number, i.e. Ja(z), ca(z) and ba(z) have degrees 0, 1 and - 1 respectively and we have the decomposition F(nk) = @F(nJn).
(2.5)
The algebra of fields F(Qk) is not simply the set of "words" in the fields that can be made using the rules given above, there are also relations. If we denote the operator product expansion of A and B by A(z)B(w) ~ J2 -r ^ - , then the relations valid r (z in F((2k) are [4] ~ w>r (AB)(z) - (BA)(z) = [A,B}(z) = £ ( - l ) r + 1 ^ {AB}r , r>0 ^ (A(BC)) (z) - (B(AO) (z) = ([A, B] C) (z), d(AB) (z) = (dAB) (z) + (AdB) (z).
(2.6)
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Relation Between Quantum W Algebras and Lie Algebras
321 dz -— d(z) -— d(z) and and 2m 2m
// a
a
d(z) = (J (z) - xV (z)))cQ(z)
- \ ff(b^cQc0))
(z).
(2.7)
D is of degree 1 (i.e. £>(F(.f?fc)(i>) c F(/? fc ) (,+1) ) and D2 = 0 which means that F(Qk) is a complex. One is then interested in calculating the cohomology (or Hecke algebra) of this complex because the zeroth cohomology is nothing but the quantization of the classical W algebra [15, 16]. This problem has been solved for the so-called "finite W algebras" in [13]. The first step is to split the BRST current into two pieces [16]: d0(z) = -X(Ja(z))ca(z), a
d,(z) = J (z)ca(z)
(2.8)
- \ ff(b\cac0))
(z),
(2.9)
and to make F(flk) into a double complex F(fik) = 0 F(i? fc ) (r ' a) by assigning the rs
following (bi)grades to its generators: deg(J a (z)) = (-k, k) deg(cQ(z)) = (A:, 1 - k) deg(6a(2)) = (-fc,fc-l)
if if if
ta£gk, ta£gk, taegk.
(2.10)
The operators D0:F(Qk)ir's) — F(j7 fc ) (r+1 - s) and £>,: F0G fc ) (r ' a) -> F(/2 fc ) (r - a+1) associated in the obvious way to d0 and d, satisfy Dg = D2 = D0Dl + D,D 0 = 0 verifying that we have obtained a double complex. Let us now calculate the action of the operators D0 and Dl on the generators of F(Qk). For this it is convenient to introduce Ja(z) = Ja(z) + f^QPc^) (z). One then finds by explicit calculation D0(Ja(z)) = D0(cjz))
-ffX(J\z))c0(z),
= 0,
Q
D0(b (z)) = a
-x(J°(z)), a
Dx{J {z)) = f% P(z)ca(z) Dl(cjz))
=
+ kgaadca(z)
-
f$ef?adca(z),
-\f^(c0c1)(z), Q
D1(6°(2)) = J (z). From these formulas it immediately follows that D(Ja(z)) = 0 and D(ba(z)) = 3a(z) - x(J Q (z)). This means that the subspace Fa(Qk) of F(Qk) generated by J™(z) and ba(z) is actually a subcomplex. The cohomology of this complex can easily be calculated and one finds H*(Fa(Qk); D) = C. Note also that due to the Poincar6-Birkhoff-Witt theorem for field algebras (which follows immediately from the relations (2.6)) the normal ordening map (• • y-Fr^k) ® ®
pa
^)
-» F ^)
(2-ii)
a
defined by -A,(z)<8>.. .®A{(z) ►> - (A{... At)(z) (where we always use the convention (ABC) (z) = (A(BC)) (z)) is an isomorphism of vectorspaces. Due to this and the
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J. de Boer, T. Tjin
fact that the BRST operator acts as a derivation ' on F(Qk) we have H*(F(f2k); D) a /T*(Fwd(/2fc); D) ® (g) H*(Fa(Qk); D) a
SiH*(F^({2k);D),
(2.12)
where in the first step we used a Kunneth like theorem given in [13]. In order to calculate H*(Fred(/?fc); D) one uses the fact that F^Q^ is actually a double complex which makes calculation of the cohomology possible via a spectral sequence argument [13, 16, 17]. The first term E{ of the spectral sequence is the D0 cohomology of F^Q^. Note that we can write D0(J&(z)) = -Tr([t+,t&]t0c0(z)). Therefore D^J^iz)) = 0 iff t& 6 glw, where glw is the set of elements of g that are annihilated by adt (the lowest weight vectors of the sl2 multiplets) and where we used the fact [13] that t& e Ker(adf ) iff t& € Ker(adt+). It can also easily be seen that for all /3 there exists a linear combination a((3)&Ja(z) such that D0(a(/3)&J&(z)) = c0(z). From this it follows [13] that purely on the level of vectorspaces we have if"(Fred(r?fc); D0) a Flw(nk)6kfi,
(2.13)
where Flw(Qk) is the subspace of F(Ok) generated by the fields {J&(z)}t&€g, • Since the only cohomology that is nonzero is of degree 0 the spectral sequence abuts at the first term, i.e. E^ = E{, and we find the end result H^F^in,);
D) a Flw(Qk)6nfi .
(2.14)
Having calculated the BRST cohomology at the level of vector spaces one now can construct the cohomology (or W algebra) generators and their OPEs via a procedure called the tic-tac-toe construction [18]. Consider a generator J&(z) of degree (p, —p) of thefieldalgebra Flw(Qk) (i.e. t& £ glw) then the generator of cohomology associated to this element is given by p
W&(z) = J2(-VlW?(z),
(2.15)
1=0
&
where WQ'(Z) = J (z) and W{*(z) can be determined inductively by D1(Wla(z)) = D0(Wl%l(z)). (2.16) It is easy to check, using the fact that D0(J&(z)) = 0 for t& € glw that indeed D(W&(z)) = 0. The formalism presented above provides us with a completely algorithmic pro cedure of calculating the W algebra associated to a certain sl2 embedding: First determine the space gt . Then take a current J&(z) with t& € glw and inductively calculate the fields WJ*(z) using relations (2.16). The field (2.15) is then the cor responding W generator and the relations in the W algebra are then just the OPEs between the fields {Wa(z)}t €S calculated using the OPEs in F(fik). 1 This follows from the fact that D(X(w)) = {d(z) X(w)},, and from the following general identities for operator product expansions: {AdB}1 = d{AB}l and {A(BC)}K = (~\)AB(B{AC)X) + {{AB},0
473
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Relation Between Quantum W Algebras and Lie Algebras
In principle this algebra closes only modulo D-exact terms. But since we computed the D cohomology on a reduced complex generated by Ja(z) and ca(z), and this reduced complex is zero at negative ghost number, there simply aren't any D exact terms at ghost number zero. Thus the algebra generated by {W&(z)}t_eg closes in itself. As was shown in [13] for finite W algebras, the operator product algebra generated by the fields Wa(z) is isomorphic to the operator product algebra generated by their (bi)grade (0,0) components W°(z) (the proof in the infinite dimensional case is completely analogous and will not be repated here). The fields Wp(z) are of course elements of the field algebra generated by the currents {^a(.z)}t €S • The relations (i.e. the OPEs) satisfied by these currents are almost identical to the relations satisfied by the unhatted currents,
Ja(z)P(w)=
y
o +~
(z - wY
— + ...,
(2-17)
z- w
where fca/5 = / ° A / A • Now, it is easy to see that g0 is just a direct sum of slp and u(l) algebras, i.e. forgetting for a moment about the u(l) algebras one can write
&~SK,--
(2-18)
3
Within the si
component of g0 we have the identity fca'J = ^ ( f t - / i J . > ,
(2.19)
where h is the dual coxeter number of g and fy is the dual coxeter number of slp . We therefore find that the field algebra generated by the currents {>^Q(z)}tae &,. denoted from now on by P0, is nothing but the field algebra associated to a semisimple affine Lie algebra the components of which are affine slp and u(l) Lie algebras. This semisimple affine Lie algebra is not simply g0 (whose field algebra is generated by the unhatted currents) however because in g0 all components have the same level while in P0 the level varies from component to component as follows from Eq. (2.19). This is just a result of the ghost contributions ka/3 in the OPEs of the hatted currents. From the above we find that the map W*(z).-»(-iyW°(z)
(2.20)
is an embedding of the W algebra into P0. This provides a quantization and gen eralization to arbitrary sl2 embeddings of the well known Miura map. In [8] the standard Miura map for WN algebras was naively quantrised by simly normal or dering the classical expressions. This is known to work only for certain algebras [2]. Our construction gives a rigorous derivation of the quantum Miura transformations for arbitrary Kac-Moody algebras and sl2 embeddings (the generalized Miura trans formations for a certain special class of sl2 embeddings were also recently given in [23]). As a result of the generlaized quantum Miura transformation any representation or realization of P0 gives rise to a representation or realization of the W algebra. In particular one obtains a free field realization of the W algebra by choosing
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J. de Boer, T. Tjin
the Wakimoto free field realization of P0. Given our formalism it is therefore straightforward to construct free field realizations for any W algebra that can be obtained by Drinfeld-Sokolov reduction. 2.1. The Stress Energy Tensor It is possible to give a general expression for the stress-energy tensor of a W algebra related to an arbitrary sl2 embedding. For this purpose we write t0 as tQ — sata, where the sa is only nonzero if ta lies in the Cartan subalgebra. Furthermore, let 6a be the eigenvalue of ad* acting on ta> thus [t0,ta] = Sata. From this it is easy to see that 6a = saf£a. Then the stress-energy tensor is T= ^ ^ ( f f ^ ( > > ) + 2 5 6 c t J 6 x ( ^ a ) - 2 ( A : + / i ) 5 a 5 > + 5 6 Q / e b a a J e ) ,
(2.12)
where the indices a 0 , 60 run only over g0, and h is again the dual Coxeter number. By adding a D-exact term D(R) to (2.21), where R
= kTh 9»«(jbja) + 2(kTh) *~f?W°>»
•
< 2 - 22 >
we can rewrite it as T = ^Th)
9ab(JaJb)
' sadJa + <*Q - nbadca
+ 6adbaca ,
(2.23)
which has the familiar form of improved Sugawara stress-energy tensor plus the stress energy tensors of a set of free b — c systems. The other generators of the W algebra cannot in general be written as the sum of a current piece plus a ghost piece. Actually, (2.23) is precisely what one would expect to get from a constrained WZNW model. Notice that 6a is the degree of ta with respect to tQ, whereas a in (2.23) runs over g+ which was defined with respect to a new, different, integral grading of the Lie algebra. In terms of the level k and the Cartan elemet of the sl2 embedding t0 (called the "defining vector" since it determines the whole sl2 subalgebra up to inner automorphisms) the central charge of the W algebra is given by 2
c(k; t0) = dim(50) - j dim(g,) - 12 2
y/k + h
- tnVk + h ,
(2.24)
where , is defined by (2.2), and g is half the sum of the positive roots, a£A+
3. Examples In this section we consider the three simplest cases of quantum Drinfeld-Sokolov reduction, namely the Virasoro algebra, the Zamolodchikov W3 algebra and the socalled Polyakov-Bershadsky algebra W^K For notational convenience we shall omit the explicit z of the fields where possible.
475
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Relation Between Quantum W Algebras and Lie Algebras
3.1. The Virasoro Algebra The Virasoro algebra is the simplest W algebra and it is well known to arise from the affine sl2 KM algebra by quantum Drinfeld-Sokolov reduction [20]. It is the W algebra associated to the only nontrivial embedding of sl2 into itself, namely the identity map. We consider this example here to contrast our methods to the ones used by Bershadsky and Ooguri. Choose the following basis of sl2:
where t0 = -t2, t+ = i, and t_ — t3. The positive grade piece of the Lie algebra § = sl2 is generated by t,, and the constraint to be imposed is J 1 = 1. The BRST current d(z) is given simply by d(z) = ( J ' q ) - c,.
(3.2)
The 'hatted" currents are J 1 = J \ J 2 = J2 + 2(6'c1) and J 3 = J3. The cations of D0 and Dx are given by £>0(J2) = - 2 c , , D 1 (J 3 ) = (J 2 c 2 ) + (fc + 2)ac 1 , £>„(&') = - 1 ,
£,(&') = J \
On the other fields D 0 and £>, vanish. From (3.3) it is immediately clear that //(F red (i? fc ); D0) is generated by WQ = J3, in accordance with the general arguments in Sect. 2. To find the generator of the D-cohomology, we apply the tic-tac-toe construction. We are looking for an element W?(z) e f red (^ fc ) such that D0(W3(z)) = 3 D,(WQ 3 ). The strategy is to write down the most general form of W (z), and then to fix the coefficients. In general, W? must satisfy the following two requirements: 1. if Wf* has bidegree (—k,k), then wf+l must have bidegree (—k — l,k + 1), 2. if we define inductively the weight h of a monomial in the Ja by h(Ja) = 1 - fc if t& G 9k> WAB)) = h(A) + h(B) and h(dA) = h{A) + l 2 , then h^W?) = h(W^+l). These two conditions guarantee that the most general form of Wf will contain only a finite number of parameters, so that in a sense the tic-tac-toe construction is a finite algorithm. In the case at hand, the most general form of W3 is a^P'J2) + a^J2, and the D0 of this equals —4al(J2ci) — (4a, + 2a2)dcl. Thus, a, = —1/4 and aj = -(fc + l)/2. Since D^W3) = 0, the tic-tac-toeing stops here and the generator of the D cohomology reads W3 = W3 -W3
= J3 + { (J 2 J 2 ) + ^ p
dJ2.
(3.4)
As one can easily verify, T = W3/(k + 2) generates a Virasoro algebra with central charge c(fc)=13-6(fc + 2 ) - - 4 - r , fc + 2 a result first found by Bershadsky and Ooguri [20].
(3.5)
2 The weight h is similar to the conformal weight, but not always equal to it. It is independent of the way in which the J are ordered
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Let's now consider the quantum Miura transformation. In the case at hand g0 is the Cartan subalgebra spanned by t2 and P0 is an affine u(l) field algebra at level k + 2 generated by J2. Indeed defining the field d
(3.6)
(3.7)
. This is the usual expression for the Virasoro algebra in terms
3.2. The Zamolodchikov W3 Algebra Having illustrated the construction in some detail for the Virasoro algebra, we will now briefly discuss two other examples. We start with the Zamolodchikov W3 algebra [1]. This algebra is associated to the so-called "principal" sl2 [11]. In terms of the following basis of s/3: / Jat„
J5 - + 4r 6 2 J
-AJ6 + J1)
(J 2 + J 3 )
V
J1
' 3 2
\
J* \ (-J6 + J 7 )
3
HJ -J )
J4 -T
(3.8)
J5 /
the sl2 subalgebra is given in this case by t+ = 4t2, t0 = -2t5 and t_ = 2t 7 . The constraints are therefore J1 = J 3 = 0 and J2 — 1 according to the general prescription. The BRST current associated to these (first class) constraints reads d(z) = J ' c , + (J 2 - l)cj + J3C3 + 2(6'(c 2 c 3 )).
(3.9)
The cohomology //(F red (/? fc ); D0) is generated by J1 and J 8 since <7 and to span <jl . The tic-tac-toe construction gives as generators of H(F(Qk); D) the fields W1 = W 7 - Wj and W* = W08 - IV,8 + W*, where
Wj = -\ (J4J4) - \ (J4J4) - 2(Jfe + 2)dP , W* = -(J5J6) + I (J*J7) -(k + 2)dJ6,
(3.10)
H/» = - i ( i V 4 i 4 ) ) + l ( W ) ) + ( - ^ - (J 4 aJ 4 ) + (fc + 2) (J5dJ4) + Wl±2l
&j4.
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Relation Between Quantum W Algebras and Lie Algebras
With some work, for instance by using the program for computing OPE's by Thielemans [22], one finds that 1 W\ 2(fc + 3) (3.11)
w=
W*
^ (5c+ 22) (fc + 3)3
generate the W3 algebra with central charge 24 (3.12) fc + 3 For any principal embedding the grade zero subalgebra g0 is just the Cartan subalgebra. In the case at hand P0 is therefore a direct sum of two affine u(\) field algebras, both of level fc + 3, generated by J 4 and P. Defining d
d^zWAw)
lJ
=
x2
J
(3.13)
+
{z - wY According to the general prescription the Miura transformation reads in this case W1 >-> -Wj and W% ^ W2*, and the fields l
J<0,0) _
W
=
wJ, W?
( 5 c + 22) (fc + 3)3
also generate a VV3 algebra with central charge (3.12). Note that according to (3.10) T^ 00 ' and W<0'0> only depend on >, and <j>2. This is the well known free field realization of W3. 3.3. The W^2) Algebra The two examples discussed above are both related to principal sl2 embeddings. In order to illustrate that our methods work for arbitrary embeddings we now consider the example of the W\ ) algebra which is associated to the (only) nonprincipal sl2 embedding into s£3. To describe the W^2) algebra, we pick a slightly different basis of s/3, namely 4 / Jr
5 J-J 1
Jb
J8
\
4
J — 3
JaL \
J1
J3
(3.14)
J1 J4
J5
The sl2 embedding reads t+ = t{, t0 = ts and t_ = ts. The gradation of g with respect to adt is half-integer which means that there will be class constraints [11] corresponding to the fields with grade - 1 /2. If one wants to use the BRST formalism
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all constraints should be first class. One way to get around this problem is to introduce auxiliary fields [10]. This is not necessary however as was shown in [12, 13] since it is always possible to replace the half integer grading and the constraints associated to it by an integer grading and a set of first class constraints that nevertheless lead to the same Drinfeld-Sokolov reduction. As mentioned earlier we have to replace the grading by t0 by a grading w.r.t. an element 5. 3 In this specific case 6 = ^ diag(l, 1,-2). With respect to ads, tx and t3 have degree 1 and span g+. The BRST current is d(2) = ( ( J 1 - l ) c , ) + J 3 c 3 . Notice that and J3 = {J4, J6, J1, is generated
(3.15) 1
there is no need for auxiliary fields, since the constraints J = 1 0 are first class. The cohomology H^F^Q^; D0) is generated by J 8 } . Again using the tic-tac-toe construction one finds that H(F(f2k); D) by W4 = W04; W6 = W*\ W1 = W07 - Wj and W* = W$ - Wf, where
W4 = J4,
Wj = i (J 2 ./ 5 ) + \ (J 2 ./ 4 ) - (k + DdJ2 ,
(3-16>
The OPE's of the hatted currents involving shifts in level are in this case
J\z)J\w)~^ 6(*+D U- + --(z — w)2 fc-f)2 3
J\z)J\w)~
(3.17) ,-+■■■,
(z — wY Jz(z)jr'(w) ~
-r + —
(z — wy If we now define the following generators: H =
— +... . (z — w)
-W4/3,
G~ = W\
T=^(W* 3
(3.18)
+
±{W4W4)),
Essentially what one does is split the set of second class constraints in two halves. The constraints in the first half, corresponding to positive grades w.r.t. 6, are still imposed but have now become first class. The other half can then be obtained as gauge fixing conditions of the gauge invariance generated by the first half
479
Relation Between Quantum W Algebras and Lie Algebras
329
we find that these generate the W^2) algebra [10], with c(k) = 25 - 6(/c + 3) - - ^ - , (3.19) k+ 3 a formula that was found in [10] by a counting argument. In the case at hand the subalgebra g0 is spanned by the elements t 4 , t5, t6 and t2. Obviously g0 = sl2 © u(\). Therefore P0 is the direct sum of an affine sl2 and an affine u(l) field algebra, and using Eq. (2.19) the levels of these can be calculated to be k + 1 and k + 3 respectively. Indeed if we introduce the currents 9 0 = i ( J 4 + 3J5),
\J2,
J~ =
J+ = 2 J 6 , then these satisfy the following OPE's: z—w J+(Z)J
(W) =
AZ)J°(W)=J
-r + (z — wY
+ • • •, z—w
+ ... ,
S 1
(z — w)
\ (k + 3) (2 - wY and all other OPEs are regular. As stated before the shifts in the levels that one can see in these OPEs are a result of the ghost contributions. The quantum Miura transformation in this case reads: W4 H-> W$, W6 >-> Wfi, 1 W i-» -Wnx, W% H-> -Wf. This means that in terms of the currents J±, J ° and
2 j0j0 = 2(fc ^7TTT, ) + ( J "- 7 + ) + ( J + J _ ) + 3) ( (
+ (fc + 3)dJ° + \ (dcpdcj)) + QQB1® , where Q0 = -(k + 1). We recognise in the expression for T the improved sl2 Sugawara stress energy tensor and the free boson in a background charge. Note that these formulas provide an embedding of U^2) into F 0 . In [11] a realization of this type was called a "hybrid field realization" since it represents the W algebra partly in terms of KM currents and partly in terms of free fields.
480
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J. de Boer, T. Tjin
It is now easy to obtain a realization of Wj ' completely in terms of free fields by inserting for the sl2 KM currents J±, J° their Wakimoto free field form J~=0, J+ = -(72y9) - kd-/ - V2k + 6-yidtp,
(3.20)
J° = -2(7/3) - V2k + 6id
+ ... ,
*7 idtp(z)id
(3.21) -j + . . . .
(z - w)2 This example gives a nice taste of the general case. By the Miura transformation one can write down for any W algebra a hybrid field realization, i.e. a realization partly in terms of free fields and partly in Kac-Moody currents. When required one can then insert for the KM currents the Wakimoto free field realization giving you a realization of the W algebra completely in terms of free fields.
4. Discussion In this paper we have quantized all generalized Drinfeld-Sokolov reductions. This was done using a formalism that differs from the formalism first used by Bershadsky and Ooguri. The fonnalism of Bershadsky-Ooguri makes use of the Fock space resolutions of affine Lie algebras and W algebras. In the calculation of the BRST cohomology they have to prove that the BRST cohomology and the resolution cohomology commute. This they indeed did for the Virasoro algebra but in the case of the algebra it is an assumption [10]. The W algebras are in the end constructed as the commutant of certain screening operators. Calculating this commutant and finding a complete set of generators of it is in general very difficult. In [10] Bershadsky doesn't prove that the generators that he provides are a complete set nor does he show how he has obtained them. Our method on the other hand does not make any assumptions, is completely algorithmic and works for arbitrary sl2 embeddings. The difference with the cohomology calculations of Feigin and Frenkel [16] is that the spectral sequence they use is different from the one that we use (in principal one can associate two spectral sequences to any double complex). An important open problem is tofindunitary representations of the W algebras in the set 9ST. It is believed that many questions about the representation theory can be answered using the correspondence between Lie algebras and W algebras exhibited in this paper. For example it should be possible to derive character formulas for the W algebras from the affine characters (see also [24]). This is now under investigation.
481
Relation Between Quantum W Algebras and Lie Algebras
331
5. Appendix In this appendix we review some basic facts on sl2 embeddings [25]. The sl2 embeddings into sln are in one to one correspondence with the partitions of n. (Let (nl,n2, . ■.) be a partition of n with n1 > n2> ..., then define a different partition (mx,m2, •..) of n by letting mk be the number of i for which ni > k. Furthermore t
let st = 53 m i - Th e n the sl2 embedding associated to the partition (n1,n2, ...) is i=i
given by n,-l i>l fc=l
.-EE^-')
t» = ^
^
l^-k)El+Sk_iMak_]
o i fc=i
n,-l
v
k n k £
'
* - =1>15 m ( i- ) i-■ l+s ,l+Skk=l /
k
where E^ is as usual the n x n matrix with zeros everywhere except for the matrix element (i,j) which is equal to one. The element 6 which defines the grading on sln, that we use to impose the constraints is given by [13]
E
»fc-,+J,s fc -l+J •
(5 !)
-
One can check that in case the grading provided by t0 is integer then <5 = t0. The fundamental representation of sln decomposes into irreducible sl2 multiplets. This we denote by n —► 0 7 ^ 1 , where i is the i-dimensional representation of sl2. i
We then have the following identities that come in useful when trying to calculate the central charge c(k; S) for a certain specific case:
\ dim(g, ) = *
\g\2 =
^2 i>O,k>0
±{n3-n),
W2 = n£n<(* 3 -*),
(5 2)
-
i
tfo I 0) = n ( l > f r
3
- 0 + 5 ^ i ( i + l)(3r - i - 2 ) n , n \ .
This concludes our discussion of sl2 embeddings. Acknowledgements. We would like to thank H. Goeree and F. A. Bais for useful discussions and comments.
482
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J. de Boer, T. Tjin
References 1. Zamolodchikov, A.B.: Theor. Math. Phys. 65, 1205 (1985) 2. Bouwknegt, P., Schoutens, K.J.: W symmetry in CFT. CERN-TH. 6583/92, ITPSB-92-23 (to be published in Phys. Rep.) 3. Goddard, P., Kent, A., Olive, D.I.: Phys. Lett. 152, 88 (1985); Commun. Math. Phys. 103, 105 (1986) 4. Bais, F.A., Bouwknegt, P., Surridge, M., Schoutens, K.: Nucl. Phys. B304, 348 (1988); Nucl. Phys. B 304, 371 (1988) 5. Drinfeld, V., Sokolov, V.: J. Sov. Math. 30, 1975 (1984) 6. Balog, J., Feher, L., O'Raifeartaigh, L., Forgac, P., Wipf, A.: Ann. Phys. 203, 76 (1990) 7. Bakas, I.: Commun. Math. Phys. 123, 627 (1989) Mathieu, P.: Phys. Lett. B 208, 101 (1988) 8. Fateev, V.A., Lukyanov, S.L.: Int. J. Mod. Phys. A3, 507 (1988) 9. Polyakov, A.: Int. J. Mod. Phys. A 5, 833 (1990) 10. Bershadsky, M.: Commun. Math. Phys. 139, 71 (1991) 11. Bais, F.A., Tjin, T., van Driel, P.: Nucl. Phys. B 357, 632 (1991) 12. Feher, L., O'Raifeartaigh, L., Ruelle, O., Tsutsui, I., Wipf, A.: On the general structure of Hamiltonian reductions of WZW theory. DIAS-STP-91, UdeM-LPN-TH-71/91 13. de Boer, J., Tjin, T.: Quantization and representation theory of finite W algebras. THU-92/32, ITFA-28-92 14. Bais, F.A., Bouwknegt, P., Surridge, M., Schoutens, K.: Nucl. Phys. B 304, 348 (1988) 15. Kostant, B., Steinberg, S.: Ann. Phys. 176, 49 (1987) 16. Feigin, B.L., Frenkel, E.: Phys. Lett. B 246, 75 (1990) Frenkel, E.: W algebras and Langlands correspondence. Harvard preprint 1991, Affine KacMoody algebras at the critical level and quantum Drinfeld Sokolov reduction. Harvard Thesis 17. McCleary, J.: User's guide to Spectral sequences. Mathematics Lecture Series 12. Washington: Publish or Perish 1982 18. Bott, R., Tu, L.W.: Differential forms in Algebraic topology. Graduate Texts in Mathematics 82. Berlin, Heidelberg, New York: Springer 1982 19. Gerasimov, A., Morozov, A., Olshanetsky, M., Marshakov, A., Shatashvili, S.: Int. J. Mod. Phys. A 5, 2495 (1990) Bouwknegt, P., McCarthy, J., Pilch, K.: Prog. Th. Phys. Suppl. 102, 67 (1990) Feigin, B.L., Frenkel, E.: Usp. Math. Nauk. 43, 227 (1988) 20. Bersahdsky, M., Ooguri, H.: Commun. Math. Phys. 126, 49 (1989) 21. Polyakov, A.M.: Physics and mathematics of strings. Brink, L., Friedan, D., Polyakov, A.M. (eds.) Singapore: World Scientific 1990 22. Thielemans, K.: Int. J. Mod. Phys. C2, 787 (1991) 23. Deckmyn, A.: Phys. Lett. B 298, 318 (1993) 24. Frenkel, E., Kac, V., Wakimoto, M.: Commun. Math. Phys. 147, 295 (1992) 25. Dynkin, E.B.: Am. Math. Soc. Transl. 6, 111 (1967) Communicated by R. J. Dijkgraaf
483 Reprinted with permission from Physics Letters B Vol. 315, pp. 304-310,1993 © 1993 Elsevier Science Publishers B. V. (North-Holland Physics Publishing Division)
Extensions of the Virasoro algebra and gauged WZW models * Alexander Sevrin*- 1 and Walter Troost 1 1 , 2 * Department of Physics, University of California at Berkeley, and Theoretical Physics Group, Lawrence Berkeley Laboratory, Berkeley. CA 94720, USA Instituut voor Theoretische Fysica, Universiteil Leuven, Celestijnenlaan 200D, B-3001 Leuven, Belgium
b
Received 11 June 1993 Editor P.V. Landsboff
To any non-trivial embedding of si(2) in a (super) Lie algebra, one can associate an extension of the Virasoro algebra. We realize the extended Virasoro algebra in terms of a WZW model in which a chiral, solvable group is gauged, the gauge group being determined by the si(2) embedding. The resulting BRST cohomology is computed and the field content of the extended Virasoro algebra is determined. The closure of the extended Virasoro algebra is shown. Applications such as the quantum Miura transformation and the eflectivc action of the associated extended gravity theory are discussed.
Extensions of the Virasoro algebra, for a review see [1 ] , such as the Wn algebras, the supersymmetric Vi rasoro algebra, etc., play a crucial role in the study of conformal field theories, 2D gravity and integrable systems. There is a close relation between extended Virasoro algebras and embeddings of sl(2) in a (su per) Lie algebra g. In [ 2 ] , it was shown that given an affine Lie algebra g and an embedding of si (2) in g, one recovers the Ward identities of an extended Vi rasoro algebra from the Ward identities of a WZW model by constraining the affine currents as / 2 = j(Ce-_ + T where e± and «b are the si(2) generators and T e keradf +. Almost [3 ] all known extended Vi rasoro algebras can be obtained in this way. Some al gebras which do not fall into this class can be obtained from an algebra which falls in this class by orbifolding. Another complication which arises is that for certain extended Virasoro algebras, currents of dimension \
* This work was supported in part by the Director, Of fice of Energy Research, Office of High Energy and Nu clear Physics, Division of High Energy Physics of the US Department of Energy under Contract DE-AC0376SF00098 and in pan by the National Science Foun dation under grant PHY90-21139. 1 Address after 1 October 1993: TH Division, CERN, CH1211 Geneve, Switzerland. 2 Bevoegdverklaard Navorser NFWO, Belgium.
304
appear. Dimension \ currents cannot be obtained by the method outlined above. However because of the fact that dimension \ currents can always be decou pled from the extended Virasoro algebra, [ 4 ] , see also [5], these cases are covered as well. Many aspects of these reductions were studied in [ 6,7 ] . Until recently, most considerations were classical. In [8,9] impor tant steps towards the understanding of the quantum theory were made. Parallel to this issue was the development of in duced and effective gravity theories (in the light-cone gauge) associated to extended Virasoro algebras [ 1 0 16]. In this letter we complete the program started in [16] which relates both issues discussed above. For an arbitrary embedding of sl(2) in a Lie algebra g, we realize the corresponding extended Virasoro algebra in terms of a WZW model for which a chiral, solvable group has been gauged, the gauge group being deter mined by the sl(2) embedding. Gauge invariance re quires in certain cases the introduction of extra free fields. The generators of the extended Virasoro alge bra are obtained by solving the BRST cohomology. Due to the presence of the extra, free fields, the BRST charge cannot be decomposed into two mutually anticommuting, nilpotent charges. So, the techniques of [8,9] cannot be applied directly. However, because
484
of the existence of a filtration of the BRST complex, spectral sequence techniques can still be used to solve the cohomology. The quantum Miura transformation immediately follows from this. Finally, choosing a dif ferent gauge yields effortlessly the effective action in the light-cone gauge of the corresponding extended gravity theory. Given a (super) affine Lie algebra g of level K, we call the finite dimensional subalgebra g. Consider a nontrivial embedding of si (2) in a (super) Lie al gebra g. A thorough study of si(2) embeddings can be found in [17]. The adjoint representation of g branches into irreducible representations of si (2). For a given embedding, we denote the generators of g by 'o«t.o;> where j e jN labels the irreducible represen tation of sl(2), m runs from -j to j and a, counts the multiplicity of the irreducible representation j in the branching. The si (2) generators e± and e0 are denoted by*± = /(liLoi/v/Iand^o = »(io,o)Thesl(2) algebra is given by [eo,e±] = ±2e± and [e>,e- ] = e<). The action of the si (2) algebra on the other generators is given by ko,'o»..o;)] =
2mtUmMj),
[e±.W,>l = <-)'+"-l/2±l/2 x \ / ( 7 T m ) 0 ' ± m + l)«(;«,±i^).
(1)
Throughout the paper we will use projection operators 77, e.g. 77 + J = {tUmaj)\m > 0;V/,a,}, 77 >m J = |vy,a ; }.Our conventions are as in [ 16 ] # l . The affine Lie algebra g is realized by a WZW model with action KS~ [g]. The action Si Si
=KS~lg] + — / str Aj(J. XX J
+ ^
- j * ^ - - jic[T,f_l)
y str[T,e_)ST,
(2)
with the affine currents Jx = jKdgg'', the gauge fields AT £ 77+£ and the "auxiliary" fields r e 77+I/JF. is invariant under *' Except that in [16], auxiliaryfieldsr, r and r were in troduced. The relation between the auxiliaryfieldshere and those in [16] is [ri^.r-l = (r + r + r ) , ^ .
Aj^dhh-1
g-^hg,
T^T + nt,/2ri,
+hAjh-\ (3)
where h = expi/, t} e 77+g. Note that as bosonic ir reducible representations of half integer spin always occur in pairs, the introduction of auxiliary fields can be avoided in the purely bosonic case [6,18] by fur ther restricting the gauge group. In the supersymmetric case however, this is not true anymore. The sim plest example, the standard N = 1 Neveu-Schwarz algebra, which is based on the embedding of sl(2) in osp(2| 1), already requires the introduction of one ex tra free fermion. For uniformity and simplicity, we al ways introduce these extra fields whenever represen tations of half-integer spin occur. The gauge fields A? are Lagrange multipliers which impose the constraint fI.Jz = \ice- + jic[T,e_]. Call the constrained current J\. Performing the gauge transformation which brings J\ in the form T + j»cf- where T e ker ade+, we get, by construc tion, the fields T which are gauge invariant modulo the constraints, i.e. modulo the equations of mo tion of the gauge fields AT. They are of the form T« Ili* id<^, + .... We couple these currents to sources and modify the action to
* = 5'
+
4^/S,r"r'
(4)
with the sources n € ker ad e-. We will show that T forms an extension of the Virasoro algebra. As the polynomials are only gauge invariant modulo terms proportional to the equations of motion of the gauge fields, we cancel the resulting non-invariance terms in <5S2 by modifying the transformation rules for the gauge fields suitably. These modifications are proportional to the /i-fields and do not depend on the gauge fields themselves. Because the gauge fields occur linearly in the action, the action £2 is now gauge invariant. In order to gauge fix the system we use the Batalin-Vilkovisky formalism [ 19,20 ]. We introduce ghostfields c e 77+£ and anti-fields /,* 6 g~, Aj e 77- J, T* e Il-iftJ and c' 6 77-g~. The solution to the BV master equation is given by 305
485
SBV
52
- 553F /'• s , r c ' c c
+ ^
[slTJz'(!iKdc+
[c.J,])
strr c + T — 2nx + ^-dependent terms).
(dc + IcAj] (5)
The /i-dependent terms proportional to Aj absorb all complications arising from the non-invariance of T. Determining them requires an explicit knowledge of the extra terms which were added to the transforma tion rule of Aj. We will not need this here. We now perform a canonical transformation which changes Aj into a field, the antighosl b 6 TJ-'g, and Aj into an antifield b'. This amounts to the gauge choice Aj = 0. The gauge-fixed action reads
•%
ijtx J
str[r,e-]dT
1 lux
1
stifiT,
4nix
f
str{c(/ 2 - ^ice. - ^K[x,e-] (7)
where J? = j{6,c}. It is nilpotent. The total current J, = J, + Jf" satisfies the same operator algebra as J,, except for the central extension. If we write J, = tAJ,A, n.J, = t'Jla and (1 - n.)J, = t'Ja, we find J,a(x)Jlb(y)
=
J,.(x)J,-b(y)
=
(9)
(6)
and the BRST charge is Q=
themselves have to be BRST invariant. This deter mines them up to BRST exact pieces. We now study the BRST cohomology in detail. Our methods are inspired by [8,21,9,22]. However the analysis in [8,21,9] is based on the presence of a dou ble complex. As we will see, the T fields obstruct the existence of a double complex. Nevertheless, spectral sequence techniques [22] are still applicable. Consider the algebra A generated by the basic fields {b, y,,T,c}, which consists of all regularized prod ucts *2 of the basic fields and their derivatives mod ulo the usual relations [23,24] between different orderings, derivatives, etc. To every field
The operator product expansions (OPE) are compat ible with the grading. The idea of spectral sequences is now to compute the cohomology in steps. One starts by working to "leading order" only in the first component of the grading, and improves on this successively. The grading splits the BRST charge into three parts Q = Qa + Q, + Qi, with [ & ] = (1,0), [Qi] = (j.j)and [Q2] = (0,1). The operators Qo, Q, and Q2, map Aimjl) to ^ (m+ i,»), .4(»i-fi/2,«+i/2> and^ (m „ + n respectively:
(x-yy'f^J.Ay), i-lKgj+i-)Mfl/fa')lx-y)-* 0l =
+ laMJ,-b{y)
(x-yV,fl£cJlc(y), = {-{Kg-i +
+ lx-y)-,fjJ«iy).
(-)Mfadf
(10)
Nilpotency of Q implies that £$ = Q? = {Qo. Q\) = {Gi,<22} = G2 + {Go,<22} =0,but
(8)
The only unknown in the action is the current T. This again reflects the fact that we did not specify the ex plicit form of the ft dependent terms in eq. (5). For li = 0 the action is BRST invariant. In order to guar antee BRST invariance for n ^ 0, the currents 7° 306
-8^/StrC[T'e-1
G?=-{Go,<22} = 32^/str{C[/7,/2c,*_]>
(11)
*2 We use the standard point-splitting regularization: (AB)U) = (2si)-' / dz'(z' - z)-tA(z')B(z),
486
does not vanish - this is the obstruction to the exis tence of a double complex. The action of Q0} Q\ and Q2 on the basic fields is given by Q0:b->
-J-K*-,
c-0, £--i»c[*-.c], r-.0, :b~>-,iK{r,e-],
Q,
c-.0, J,--lKliT.e-],c], r-
Q2
J/7+I/JC,
-.b-n-j,,
C -» jCC,
r-0,
(12)
where 77- = 1 - / 7 - and [/I, fl] stands for f * , n = (-)M")(*',l'a)/ucfc,
(13)
where (jr*y*) is a regularized product. The BRST charge Q acts as a derivation on a regularized product of fields. To exploit the double grading, we need one more preparation. For afixedghost number £, the sequence of gradings (m, k - m) is unbounded because the first component is negative for some currents and for the bfield. The application of spectral sequence techniques requires this set to befinite.This is remedied by notic ing that the subcomplex A{'', generated by {b,fT-JtjK[r,e- ]} has a trivial cohomology H'(Am\Q) = C. From this and eq. (12) we find that we can as well compute the cohomology of the reduced complex A = A/Au\ generated by {TT-JZ, x,c) as H'(A) = H' (A). The OPEs close on the reduced complex. The double grading on A induces a double grading on A. The filtration Am, m € \Z of A
now leads to a spectral sequence (E,,d,), r > 1, con verging to H'(A\Q). Each term in the sequence is the cohomology of the previous term with a deriva tion that represents the effective action of the BRST operator at that level: £V = H'{E,-,;d,-\). To start with, this means that one neglects terms that are one half unit lower in the first grading component. The first term in the sequence is then E0 = A, d0 = Q0. The next term is E, = H'(A\ Qa). The derivation operator at this level will act like Q up to terms that have the first gradation component at least one unit lower. Thus on E\, the Qo cohomology classes, it acts like Q,, i.e. i f * 6 A [ 0 ] 6 £ i , d i [ * l = [Qi]*Note that although Q\ ^ 0, nevertheless d\ = 0, since Q\ = -Q0Q2 - Q2Q0 implies that on the Q0 cohomology classes it always results in the trivial class. The next term is then E2 = H'(E\\d\). The d2 derivation can be computed as follows. Let
/ , ®^[Tj®^[/7,/2C],
(15)
where we denoted the subalgebra of A generated by * by A [ 0 ]. Using eq. (12) again, onefindsthat £2 is represented by E2^ A [I!*,«,.(?'+
i*lT,[*-,T]])],
C6)
and one has explicitely
= Oolite «..[*']■ ,}
(,7>
From now on A stands for /7_/ r . 307
487
It turns out that E2 has only ghost number zero elements. Therefore, d2 is actually the zero map and the sequence has already stabilized at the previous level. This gives the main result: H'(A;Q)^E2
=
H'(H'(A,Qa),d{).
The unknown function / gets determined by the next recursion relation Q^"2'""2' + Q,^"2'""2' = 0: / ( r ) = y/C(\ic[T,[r,[T,e-]]] -
(18)
Having established the cohomology of Q, we now turn to the explicit construction of its generators. The cohomology is generated by f = ]£ f'-'-°i)t{)j,c,l) e ker ad e+ and r 0 "'' has the form fUA)) _ y ' f ^ j *
(19)
where f,'"' has grading (j - \r, -j + \r). From the previous discussion, we know that the leading term f 0 0 °'' is of the form
[n-.(t ),\nAtA),dx\\).
We have that f'/W>> = f0"/2•<>"!, + f ^ ' / i ' . The explicit form of all generators r^"'' must obviously be computed on a case by case basis. A useful tool for this is the fact that one can al ways construct J'2 6 n > i ? s u c n , n a t [*->■#) = J, - rhtrKif ^'- ^ m s >mPMes l n a t c c a n be written as c = -(*lK)Qa(J'z) + 2Q,U). Note also that QiUz) can be rewritten as QiU,) = j f c , / 7 - / , ] \[fl-J„c] + ±K + hdc + J[/7 0 (/^), [n0(tA),dc)]. The energy-momentum tensor fEM = f "'0) itself can be computed. It is given by fEM =
+ iK:^<5/,oi/.(l(,(r,k-,r]],0&•'><', )
(20)
- {-Kdx
A
^ ( s t r { / > - } + s t r { [ r , *_]/,}
*(/c + A ) v
+ istr {n0U,)n0(J,)}
+ ^^-^str
{e-dJl}
A
+ KUIT {[n0(t ), [n0(tA),dJl]]e-} where the normalization constant C will befixedlater on. The remaining terms are recursively determined by a generalized tic-tac-toe construction. We have
e»r;(/.«,)
-QiT' <M,>
QiT, (/.",)
(21)
K+h -str{[T,e_]3r}).
(23)
Thefirstterm is f j ' 0 ' , the second term f,"01 and the remainder forms T^'"'. It is not hard to verify that fIMP,
?(/.»,)
where T, ' = 0 for r < 0 or r > 1j. This determines f, '*' modulo, the addition of an arbitrary functional of T. As a functional of T only has grading (0,0), it can only appear in T2'"' . It gets determined by the final recursion relation: Qi f^"'' + Qifffi = 0. As an example we compute f '"-"o1 and f (l/2-Qi/J). From eqs. (12) and (17), one immediately gets ^<0.«o) _
f(0<°<,>
_
ytafca,,)
,
1 ^ . 1 , . ,g_
fw.<,m>
308
=
= VCJ,
_VC[T,7I]("2-"2;o'/=>
+
X(K
U ^ s t r / , . / , - ^—streodJ, ixy + h)
^tr([T,e-]at) +
-^slTb[e0,dc)
^ - s t r i a e + —slTdb[e<,,c], 2x Ax
(24)
is also BRST invariant. It differs from f™ by a BRST exact term
T]](00;o0)
(22) For 7 = 5, one has T0 ' From eq. (17), it follows that
fIMP =
/(r).
Q\ \
?-^strfc7 r + • •■) x(K + h) J
Eq. (24) is particularly useful to compute the central extension [16]. One finds c=<,can-{d*-dl)h-6y(K+h), K +h
(25)
488
where d%, dr respectively, is the number of bosonic, fermionic respectively, generators of g, Cent is the crit ical value of the central charge for the extension of the Virasoro algebra under consideration: Ccri, = £ ( - ) , ° ' , ( 1 2 / + l2J + V-
(26)
and y is the index of embedding, which in the case h ^ 0 is given by
>' = i ^ ( - ) < ° ' , ; 0 + l)(2>+ 1), 3h
(27)
J-J
and (-)i"i) = +1 (-1) if »0m.»;) i s bosonic (fermionic). Note that the requirement that 7*** generates the Virasoro algebra in the standard nor malization fixes the normalization constant C to be V2{K + h' Knowing the leading term of the currents, eq. (20), we find that the conformal dimension of T{,"i) is given by 7 + 1. We already observed that the OPEs close on A and preserve the grading. From this we deduce that the OPEs of the generators T close modulo BRST exact terms. However, we work on the reduced complex A, which has no states of negative ghostnumber. So there are no BRST exact terms at ghost number zero. We conclude that the OPEs of the generators T close. The quantum Miura transformation for the gener ators of the extended Virasoro algebra is also easily obtained. As the OPEs preserve the grading, the part of T with grading (0,0), 7"(o,<». closes among them selves. So the map T -» 7"(o,o> is an algebra homomorphism. In order to prove that the map 7 —* 7(0,0) is an algebra isomorphism, we have to show that each generator of the extended Virasoro algebra has a nonvanishing component of grading (0,0). This is shown following a reasoning similar to the one in [21]. Con sider the mirror of the spectral sequence, i.e. the one associated to the filtration
^"^©©Aui-
(29)
We already know that f^ for this spectral sequence vanishes unless the ghostnumber is zero. Using eq.
(12), one shows that £i = H'(A\Qi) is only nonvanishing at grading (\m,\m),m > 0. This implies that £„o is only non-vanishing at grading (0,0). This proves that 7 — r(0,o) is indeed an algebra isomor phism. Finally, the method of working we described is par ticularly useful to compute the effective action in the light-cone gauge, W[T], of the corresponding gravity theory, [16]. The effective action is defined by exp(-ff [t ]) =
x
JlSgg-'}[dr]ldAj)ldn]
v^kf) exp [-( 52 -4^/ str ^)](30)
The effective action is most easily computed by making a different gauge choice. We make a canonical transformation in eq. (S) which in terchanges fields and anti-fields for {r, T*} and {/7 + [e + ,/x],/7-[€_,y;]}. This corresponds to choosing the gauge r = 77+ [e + , J,] = 0. We find W[T)=KcS-[g],
(31) 1
where KC = K + 2h and we used [Sgg' ] = [dJ 2 ]exp(-2AS"[g]). From eq. (25) we get the level as a function of the central charge: l2yKc = I2yh - (c - {ccm) -\j(c-\c^)2-24(d*-dT)7iy-
(32)
Eq. (32) provides an all-order expression for the cou pling constant renormalization. The WZW model in eq. (31) is constrained by dgg-' + ^ s t r {/7NA ( a ^ - ' ) ) 7 7 N A
{dgg-')}e+
where 77NAJ is the projection on the centralizer of sl(2) in g. We also used Jz = ja,dgg~' with a, = K + h. For a detailed discussion on the value of Q«, see [5] and in particular [23]. The strategy developed in this paper has numerous applications. In particular, the representation theory 309
489
of the extended Virasoro algebra should be closely re lated to the representation theory of the correspond ing affine Lie algebra. The approach followed here was closely related to 2 D gravity in the light-cone gauge. In order to study e.g. non-critical strings based on some extended Vira soro algebra, one needs a covariant formulation. It is clear from eq. ( 3 2 ) that a minimal ( p , ) matter sec tor is realized in terms o f a gauged W Z W model with level Ku - PlQ - h and in order to cancel the conformal anomaly we need a gauge sector based on a W Z W model with level Ku = -p/q
- h. The gauge invariant
coupling between the matter and the gauge sector is performed in a way somewhat similar to the path fol lowed in 126]. The main problem is to construct the analogue of eq. ( 4 ) in which both the left and the right moving extended Virasoro are coupled to sources in a gauge invariant way, i.e. we need an action of the formS2 = S, + (4nxy)~'
/ s i r ( / i T + jiT).
This can
be achieved by following a path inspired by the meth ods developed in [27J. Details about this will be re ported on elsewhere [ 2 8 ] .
References [ 11 P. Bouwknegt and K Schoutens, preprint CERNT H 6 5 8 3 / 9 2 , ITP-SB-92-23, hep-th/9210010, Phys. Rep., to be published. (2) F.A. Bais,T. Tjin and P van Driel, Nucl. Phys B 357 (1991) 632. (31 H. Kausch, private communication; W. Eholzer, A. Honecker and R. Hubel, preprint BONN-HE-93-08, hep-th/9302124. (4] P. Goddard and A. Schwimmer, Phys Lett. B 214 (1988) 209. (5) A. Sevrin, K. Thielemans and W Troost, preprint LBL-33778, UCB-PTH-93/07, KUL-TF-93/10, hepth/9304020. | 6 | L. Feher, L O'Raifeartaish. O. Ruelle, I Tsutsui and A. Wipf, preprint DIAS-STP 91 29, UdeM-LPN T H 71/91, hep-th/9112068. (7] L. Feher, L. O'Raifeartaigh. O. Ruelle and 1. Tsutsui, preprint BONN-HE-93-14, D1AS-STP-93-02, hepth/9304125.
310
[8] B.L. Feigin and E. Frenkel. Phys. Lett. B 246 (1990) 75. [ 9 ] J de Boer and T. Tjin, preprint THU-93-05, hepth/9302006. (10) A. Alekseev and S Shatashvili, Nucl. Phys. B 323 (1989) 719. (11) M. Bershadsky and H. Ooguri, Comm. Math. Phys. 126 (1989) 49 (12] H. Ooguri, K. Schoutens, A. Sevrin and P. van Nieuwenhuizen, Comm. Math. Phys 145 (1992) 515. [13] K. Schoutens, A. Sevrin and P. van Nieuwenhuizen, Nucl Phys. B 371 (1992) 315. (14] K. Schoutens, A. Scvnn and P. van Nieuwenhuizen, in: Proc. Stony Brook Conf. on Strings and Symmetries 1991 (World Scientific, 1992). [15] J. de Boer and J. Goeree, Utrecht preprint THU-92/33, hep-th/9211107 (16] A. Sevrin, K Thielemans and W. Troost, preprint LBL-33738, UCB-PTH-93/06, KUL-TF-93/09, hepth/9303133. ( I 7 ] E . B . Dynkin, Amer. Math. Soc. Transl. 6 (1967) I I I . [181 A. Deckmyn, Phys. Lett. B 298 (1993) 318. (I9JJ.A. Batalin and G.A. Vilkovisky, Phys. Rev. D 28 (1983) 2567; D 30 (1984) 508; Nucl. Phys. B 234 (1984) 106 |20| A. van Proeyen, in: Proc Strings and Symmetries 1991 (World Scientific, 1992); W. Troost, P. van Nieuwenhuizen and A. van Proeyen, Nucl. Phys. B 333 (1990) 727; W. Troost and A. Van Proeyen, An introduction to Batalin-Vilkovisky Lagrangian Quantisation (Leuven University Press), in preparation. (211 J. de Boer and T Tjin, preprint THU-92-32, heptta/9211109 (221 R. Bolt and L W Tu. Differential Forms in Algebraic Topology (Springer, 1986) (23] F.A. Bais, P Bouwknegt, M. Surridge and K Schoutens, Nucl. Phys B 304 (1988) 348. [24] A. Sevrin, W. Troost, A. Van Proeyen and P. Spindel, Nucl. Phys. B 311 (1988) 465 (25] A. Sevrin, R. Siebelink and W. Troost, in preparation. [26] J. de Boer and J. Goeree, Utrecht preprint THU-92/14, hep-th/9206098. (27] K Schoutens, A Sevrin and P. van Nieuwenhuizen, Phys. Lett. B 243 (1990) 245. [28] A. Deckmyn, A. Sevrin and W. Troost, in preparation.
493
Reprinted with permission from Nuclear Physics B Vol. 304, pp. 348-370,1988 © 1988 Hsevier Science Publishers B. V. (North-Holland Physics Publishing Division)
EXTENSIONS OF THE VIRASORO ALGEBRA CONSTRUCTED FROM KAC-MOODY ALGEBRAS USING HIGHER ORDER CASIMIR INVARIANTS FA. BAIS, P. BOUWKNEGT and M. SURRIDGE Institute for Theoretical Physics, University of Amsterdam, Valckenierstraat 65, 1018 XE Amsterdam, The Netherlands
K. SCHOUTENS Institute for Theoretical Physics, University of Utrecht, Princetonplein 5, P.O. Box 80 006, 3508 TA Utrecht, The Netherlands
Received 31 August 1987
We consider bosonic extensions of the Virasoro algebra that can be obtained from Kac-Moody algebras g by generalizing the Sugawara construction to the higher order Casimirs of g. In this paper we explicitly construct the algebra of a primary field of dimension 3 constructed from the 3rd order Casimir of AN_V For N = 3 we compare our results to the Z3-extended Virasoro algebra proposed by Fateev and Zamolodchikov.
1. Introduction In recent years the study of (all possible) 2-dimensional conformal field theories (CFTs) has become of vital importance, both for string theory and for the theory of 2-dimensional critical phenomena. Though an impressive number of examples is available, a complete classification is still lacking. Our present knowledge strongly suggests that the mathematical structure, at least of the rational CFTs, derives from the theory of Kac-Moody algebras. In this paper we will construct extensions of the Virasoro algebra by integer spin fields based on Kac-Moody algebras. Before we get into detail let us first discuss the basic ideas and motivations. The spectrum of a conformal field theory can be assembled into irreducible representations of the Virasoro algebra, i.e. the 2-dimensional conformal algebra [Lm,L„] = (m-n)Lm
2
+ n+^cm(m
-l)8m
+ n0.
(l.l)
The irreducible representations L(h, c) are so-called highest weight modules
494
FA. Bats el al. / Extended Virasoro algebras (I)
349
(HWM's) characterized by the central charge c and the L0 eigenvalue h of the highest weight state. The representations which are best understood are those for which c < 1, where it is well-known [1] that the unitarity condition restricts the c-values to a discrete set
c
-c(«)-l _ _ _ _ _ m(m + 1)
- = 3,4,5,....
(1.2)
Furthermore, for each c-value there are only a finite number of possible L0 eigenvalues hp for the highest weight state
( ) 1 1 *sa-' "V r.'^'" .' iW.t"'•• 4m(m + l) \l<m -
(")
Cardy [2] has shown that the condition of modular invariance further restricts the possible spectra considerably for these c-values. If the theory is defined on a torus, then the partition function can be expressed as a sesquilinear combination of Virasoro characters Z=EX*(T)AXX*(T).
(1.4)
Recently all modular invariant combinations of the type (1.4) for c<\ in the unitary series have been classified [3,4]. This classification can also be understood from the point of view of Kac-Moody representation theory by applying the Goddard, Kent, Olive (GKO) construction [5] to the diagonal subalgebra Ax of Ax ® Av Starting from level (m - 2,1) HWM's for the A[X) © A[V affine Kac-Moody algebra one obtains level m - 1 HWM's for the diagonal A^ and c — c(m) modules for the coset Virasoro algebra. From this construction one can also understand why the modular invariants for c = c(m) are classified by modular invariants of A^ at level m - 2 and m -1 [6-8]. Our knowledge of CFTs with c > 1 is far less complete. This is because the unitarity constraint on representations turns out not to be very restrictive here, and it is not known how restrictive the modular constraint is (partial results exist though for c ■= 1 [9,10)). More is known if we consider CFTs with extended symmetries. For instance, similar results to those explained above have been obtained for the W-extended superconformal algebras (N = 1,2,4). In bosonic theories the Virasoro algebra may be extended by a Kac-Moody algebra, as is the case for the Wess-Zumino-Witten model [11,12] where the Virasoro generators are expressed as bilinears in the dimension-1 currents through the Sugawara construction.
495
350
F.A. Bais et al. / Extended Virasoro algebras (I) TABLE 1
Conformal weights for c = 4 / 5 1 4
5
2 3
13 8
3
40 21 40
1 15 1 15
21 40 1 40
7 5 2 5
1} 8
2 3
1 8
0
p
1
2
3
1
0
I
s
2 3
2 5 7 5
4
3
I
On the other hand the GKO construction of the unitary series c (m) for the Virasoro algebra discussed above, leads one to ask what is so special about A^. For example, is there any significance in the series C = C ("> =
21, \ m(m + l)j
in-4,5,6,...,
(1.5)
obtained for the coset-Virasoro algebra by taking the diagonal subalgebra A^ of A^ © A^? To get a clue to the answer of this question it is instructive to look at the first case in this series c(4) = 4/5, because it coincides with one of the cases which is already well understood. The conformal weights for c = 4/5 allowed by unitarity are listed in table 1. There exist two independent modular invariant combinations of characters; the first one being
z - E Ilx„„l 2 . p-l
(i.6)
q-l
This type of combination always occurs. It amounts to the statement that the set of characters at a given c-value form a (projective) unitary representation of the modular group PSL(2, Z). The exceptional modular invariant combination, which is the one corresponding to the 3-states Potts model, uses only a subset of all possible primary fields for this c-value. It is given by Z = IXo + X 3 l 2 + 1X2/5 + X7/5l2 + 2|X2/3l2 + 2 | X l / 1 5 | 2 .
(1-7)
Of particular interest in this model is the occurrence of the integer dimension-3 field. The primary fields occurring in the exceptional modular invariant combina tion are local with respect to this dimension-3 field. Explicitly we have the following
496
F.A. Bats et at. / Extended Virasoro algebras (I)
351
operator product expansions (OPE) [13] VV^2/5
=
[^7/5].
^3-^2/3= [^2/3].
^3 • ^ 7 / 5 = [^2/5] > ^3-^1/15 = ['/'l/is] •
(1-8)
These OPE's strongly suggest the existence of a larger symmetry in this model, the extra generators being the modes of a dimension-3 primary field. The way in which this spin-3 field acts on the other primary fields suggests moreover that the exceptional modular invariant is just the " unitary" sum of squared characters x for this larger algebra Z~ IXot2+ IX 2/5 | 2 + 1X2/3, + I2 + 1X2/3,- I' + IXl/15. + | 2 + IXl/15,-12, (1-9) where + and — refer to the eigenvalues of the " hidden" dimension-3 operator. This kind of reasoning is reminiscent of what happens in the A[X) case. There it turns out that apart from the usual modular invariant combination (which is just the partition function of the SU(2) WZW model [14]) there exist some special modular invariant combinations which either can be interpreted directly as WZW models with an extended symmetry [15,16], or as gauged versions of such WZW models [7,16-18]. In 1984 Zamolodchikov investigated the possibility of obtaining extensions of the Virasoro algebra by adding fields of higher conformal dimension to the dimension-2 field [19]. Indeed he found a solution for an algebra containing a dimension-2 and a dimension-3 field consistent with the requirements of conformal invariance and crossing symmetry of the four-point function (i.e. associativity). Recently Fateev and Zamolodchikov [20] constructed a realization of this algebra in terms of two free scalar fields (coupled to a background charge at infinity), and obtained some results concerning the representation theory of this algebra. They found a series of c-values c-c<"> = 2 | l ), \ m(m + l)j
m = 4,5,...,
(1.10)
for which there exist degenerate representations containing at least two null-vectors (called completely degenerate). It was proven that for these c-values there exist a finite number of primary fields w.r.t. this extended algebra forming a closed operator product algebra (which for c = 4/5 turns out to have precisely the conformal weights occurring in (1.9)). The operator product expansion coefficients turn out to resemble the SU(3) Clebsch-Gordan coefficients. Though the paper [20] gives a realization of this algebra it does not explain the apparent relationship with SU(3). One would like to understand how the dimension-3
497
352
F.A. Bats etal / Extended Virasoro algebras (I)
operator emerges from the A2l) Kac-Moody algebra, and why the series (1.10) is just what one obtains from the diagonal embedding A2l) in A^ © A2^. Motivated by the questions raised in this introduction we have investigated extensions of the Kac-Moody Virasoro algebra by higher dimension operators. A natural choice for these operators is suggested by the observation that the Sugawara construction of the stress-energy tensor T(z) is really based on the form of the second-order Casimir. We therefore generalized the Sugawara construction to higher order Casimirs. Explicitly we considered operators Q{z) = dabc. :JaJbr...:{z),
(1.11)
where the J"(z) are the currents satisfying a Kac-Moody algebra, and dabc is some completely symmetric, traceless tensor characterizing the Casimir. Q(z) turns out to be a primary field of dimension equal to the order of the Casimir. For any simple Lie algebra g the number of independent Casimirs equals the rank of g so one might naively expect that the OPE closes on rank (g) fields. This turns out not to be true in general; extra primary fields appear. In special cases however, they may decouple. For the algebra A2 we have in addition to the second-order Casimir only a third-order Casimir given by the SU(3) d-symbol. This is the case which will receive most attention in this paper. We should remark that the expression (1.11) does not produce a Casimir operator of the Kac-Moody algebra §, because it does not commute with all the Kac-Moody generators. Nevertheless we will often refer to (1.11) as a Casimir of g. The paper is organized as follows. In sect. 2 we will introduce some manipulations with OPE's and focus on the algebra of the dimension-3 operator corresponding to the third-order Casimir of the AN algebras. We show that this field is primary under the Virasoro algebra obtained by the Sugawara construction and that for the OPE of two of these fields we obtain Zamolodchikov's result up to an extra primary field. In sect. 3 we will discuss the role of this primary field. In sect. 4 we restrict ourselves to level 1 representations of the A$ Kac-Moody algebras, where we have an explicit realization in terms of vertex operators using N — 1 free scalar fields. For A2 the dimension-3 operator in this realization is shown to reduce to the FZ expression, which can be interpreted as the construction (1.11) where the indices run over the Cartan subalgebra only. Finally, in sect. 5 we present some conclusions, further lines of development and some arguments for the existence of higher order generaliza tions, thereby touching upon beautiful new mathematical formulae for polynomial sums of Lie algebra exponents. Three appendices are added. In appendix A we will show how to do OPE's involving normal ordered "composite" operators, by giving an integral representa tion for the normal ordered expression of two operators. We also derive some rearrangement formulas needed to compare different nestings of normal ordered expressions. Appendix B gives our conventions for the AN normalizations and some
498
F.A. Baia etol / Extended Vireuoro algebras (I)
353
contraction identities and in appendix C we give some specific fonnulas for the vertex operator realization of A$.
2. The operator algebra for die third-order Casimir of A N _, The starting point for our discussion is a conformal field J(z) which take values in the Lie algebra AN_1 of SU(N), N>3. The components J"(z) w.r.t. an antihermitian basis {Ta} satisfy the following operator product expansion -k8ab
/"(*)/» -
Jc(w)
-j
+/"6cT5-f
(z — w)
+ ■ • •.
(2.1)
z— w
where a = 1,2,...,N 2 - 1, fbc are the structure constants of Af,^ and k is a positive integer, called the level. The Fourier components J° defined by
form the Kac-Moody algebra - d ^ [JZ,Jnb] =fabcK+,-km8<">8m+n,0.
(2.2)
More complicated operators are constructed as composite expressions in the ele mentary fields J"(z). In order to be well-defined these expressions must be normal ordered (which we will denote by brackets). There are various options for doing this; the method we used is explained in some detail in appendix A. We stress here that in our convention the normal ordered product is neither commutative nor associative. For example, consider (/V»)(z) - {JbJ"){z) ~f°>»{dr){z), (j'(JbJe))(z)
- ((JaJb)J')(z)
=
(2.3)
-f"d{jddJb){z) +fbed(dJaJd)(z) + \fttcdfdbad2Ja(z).
+ $k(8acd2Jb + 8bed2Ja)(z) (2.4)
In appendix A some general results for rearranging normal ordered expressions are given. Before we introduce the third-order Casimir operator for the Kac-Moody algebra A$Llt iV> 3, we recall Sugawara's expression for the stress-energy tensor [21-24], which in our terminology corresponds to the second-order Casimir operator. This
499
354
F.A. Bais el al. / Extended Virasoro algebras (I)
operator is defined as
The contraction J" (z)T (w) can be evaluated by invoking the Wick theorem (A.6)
1
b
b
J (x)f° <J<(w)-z-w 2(k + N) =
l
^
(z-w) »
^(-2kSad
+
k8ab -3 (z-w)
fabcfcbd)Jd(w)
-
(2-6)
(z-w) Note that in the term proportional to ((z - x)'1 - (z — w)"1) a singular term in Jc(x)Jb(w) is picked up which contributes to the final result. The contraction T(z)T(w) is evaluated similarly: T
^w)=2lj^)T{z^ja)iw) k8aa
1 A
2(k + N) (z-w)
^ 2T(w) (z-w)
2
|
dT(w) (z-w)'
It follows that T(z) is just the (correctly normalized) energy momentum tensor; eq. (2.6) then states that the J°(z) are primary fields [13] of dimension 1. The central charge c is read off from (2.7) c = k(N2-l)/(k + N).
(2.8)
The construction (2.5) of the operator T(z) can be generalized to higher Casimir operators. In analogy with the finite dimensional case we define the third-order
500
F.A. Bais et at, / Extended Vlrasoro algebras (I)
355
Casimir operator Q(z) for A$_lt N^ 3, as follows Q(z) = iAN(k)d°»<{j°(J »J<)){z).
(2.9)
dabc are therf-symbolsfor AN_l (see appendix B for some of their properties) and AN(k) is a normalization constant to be determined later. The brackets in (2.9), indicating the normal ordering, are in fact superfluous since the ^-symbols are totally symmetric and traceless. This means that Q(z) is the unique candidate for the dimension-3 operator, because different arrangements of the brackets are equivalent. For convenience we define a field Qa(z) by Qa(z) = dabc{JbJc)(z).
(2.10)
It is straightforward to evaluate the OPE's of the newly defined Qa(z) and Q(z) with the other fields in the theory. A first result of interest is that Q"(z) and Q(z) are primary fields of dimension 2 and 3 respectively: T(z)Q°(w) =
^Q'(w) + (z-w)
T(z)Q(w) =
dQ'(w) + (TQ°)(w)
+■■-,
z-w
3
1 ^Q(w) + — 3 3Q(w) + (TQ)(w) +■■■ . (z-w) z-w
(2.11)
The OPE's of the elementary fields J°(z) with Qb(w) and Q(w) read Ja(z)Qb(w)
-5(2* + N)d""Je(w) +
= (z-w)
J°(z)Q(w)
= -^^(k
+ N)iAN(k)Q°(w)+
{/""<}'(">)) z—w ■■■ .
+••-, (2.12)
After a tedious calculation, using extensively the rearrangement lemmas of appendix A, we arrive at the following result for the OPE of Q(z) and Q(w): Q(z)Q{w) = ~ ~r + —K—^ + (z — w) (z-w) (z — w)
(z-w)
{2b2A(w) + ±d2T(w) + R4(w)}
{b2dA(w) + ^ 3 r ( w ) + ±dR4(w)}
+ z—w
+ (GG)(»0+---,
(2.13)
501 356
F.A. Bais etal. / Extended Virasoro algebras (I)
where we made the following choice for the normalization AN(k) A
»(k)2=^,,
1
N , „ ,2„ „ . „ , „ . . , 2 ,s 18 (k + N) (N + 2k)(N -4)
(214)
and we use the notation [19,20] A(z) = (TT)(z)-±d2T(z),
b2=^J~c-
(2-15)
R4(z) is a new primary field which will be discussed in sect. 3.
3. Comments on die algebraic structure In this section we comment on the results obtained in sect. 2 and extend them for the case N=3. Let us first compare the result (2.13) with the general form of the OPE of two primary fields
*.(*)*.(0) - Led Z #i<Jk>^+*.-*.-^*>(0)) • V
p
{*1
(3.1)
'
The index p runs over the primary fields that appear on the r.h.s.; the correspond ing descendant fields ^* } (z) occur with relative coefficients j 8 / ^ * } that can be expressed in the dimensions Am, Am and A and {k). In the singular part of the expansion (2.13) we recognize two primary fields: (i) the identity at level (z - w)~6. The coefficients of the corresponding descendant fields agree with the result in [19]. (ii) A primary field R4(z) of dimension 4 which is defined as R4(z) = -2b2A(z)
- \d2T{z) + T"(z) + 9(* + N)AN(k)2(Q'Q')(z),
(3.2)
where Tl 1{z)=
'
2(k
+ N)idJ°dJa){z)-
(33)
At level (z — w)~l we find its descendant dRA with coefficient 1/2, in agreement with £ # = 1/2. The emergence of extra primary fields in the subleading terms of an OPE like (2.13) may look curious but is in fact a generic feature which, for example, also
502
F.A. Bais etai. / Extended Virasoro algebras (I)
357
occurs in the theory with a single scalar field
" (z-w) +
2
- 2T(w) -(z-w)
8T(W)
(z-w)\-iA(w)-i5d2T(w)
+
+ (z-w)\-ldA(w)-^d3T(w)
+ ^
. . . , (3.4)
where r(z)=-}(<M
(3.5) + ±d\d
(3.6)
In this expression we recognize the identity operator at level (z - w)~2 with the corresponding "tail" of descendant fields (cf. [19]) and, at level (z - w)2, a second primary field <j>4(z) Vi{z)
= JA(x) + &2Hz) + k{(9\p)(99))(i).
(3.7)
The main distinction with (3.13) is that in this example the extra primary field turns up only in the regular piece of the expansion and is therefore usually not noticed. The algebraic structure of the present construction is certainly more complicated than it is for the usual Sugawara construction. The Fourier components Ln of the second-order Casimir operator form a Lie algebra with central terms that depend on the level k through the relation (2.8). In contrast, the components Q„ of the field Q(z) do not form a closed algebra but generate a large associative algebra which in general includes an infinite number of generators which are multilinear combina tions of the components J° (i.e. which are in the enveloping algebra of the original A'j!j>_1 Kac-Moody algebra). The structure of this algebra depends non-trivially on k, not only through the central terms but also through the non-constant terms (note that the coefficients in (3.2) are ^-dependant). Let us explore the algebraic structure somewhat further in the case of A$\ In order to do this it is convenient to rewrite the field R4(z) in a simpler form. Note that for general N two independent primary fields of dimension 4 can be con structed from the elementary ./-fields which are of the form X(7T)(z) + M 82T(z) + PTl-\z)
+ o(Q'Q")(z),
(3.8)
For N — 3 the identity (B.12) and the rearrangement lemmas of appendix A can be used to express (QaQ")(z) in terms of (TT\z), d2T(z) and Tl<\z) and we are left with a unique primary field of dimension 4 which can be written as 8+ c 22 + 5c A(z) - (TT)(z) - — a 2 r ( z ) + —^T^iz).
(3.9)
503
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F.A. Bais el al. / Extended Virasoro algebras (I)
The field R4(z) is proportional to A(z) RA(z)=f(k)A(z),
(3.10)
where / (
*
) =
36 (k + 3)2 " T ( 3 U + 33)(2A: + 3 ) '
(31l)
Using the above relations we can now evaluate the OPE of the Casimir operator field Q(z) with R4(w) for N = 3 Q(z)RA(w)
=
f(k) (z-w)
+-
-j3(l - \c){Q(w) + descendants}
-j {Rs(w) + descendants) + ••• ,
(3.12)
(z-w)
where R5(w) is yet another primary field given by where R5(w) is yet another primary field given by R5(z) = \d2Q(z) + v{dQ°dJ°)(z) R5(z) = \d2Q(z) + v{dQ°dJ°)(z) with 7c-38
,
J
+ p(TQ)(z) + p{TQ)(z)
c-6
(3.13) (3.13)
\
( i - 5(22 + 5c),
The example of iV = 3 indicates clearly that for general k the algebra generated by the Casimir operator Q(z) will contain an infinite number of primary fields {/, Q(z), RA(z), Rs(z),...}. An important exception to this general behaviour is the case N = 3, k = l. It will be shown in sect. 4 that in that case the field R4(z) vanishes identically. Accordingly, the OPE (2.13) simplifies and the commutator algebra of the components Q„ coincides with the algebra described in [19,20] for c = 2. 4. k = 1; reduction to the Cartan subalgebra The results derived so far are valid for any level k. In this section we specialize to the case k = 1 where we have an explicit realization of the Kac-Moody algebra A$_x in terms of vertex operators at our disposal. In this realization the Heisenberg subalgebra is represented by free fields H'(z), i = \,2,..., N-1, and the off-diago-
504
F.A. Bus et al. / Extended Virasoro algebras (I)
359
. -n a
* * fa*
X* ^•if»
Tfi iS
Fig. 1.
nal generators are represented by vertex-operators E"(z), where a runs over the roots of AN_X (we use the notations of [25]). It turns out that the expression for Q(z), which is a composite expression in H'(z) and Ea(z) to begin with, can be rewritten in terms of H'(z) only. This leads to a free field realization for the algebra (2.13) for k = 1, c = N - 1. The analysis can be done for any N > 3; here we present the case N = 3 in some detail. In the Cartan-Weyl basis the generators of ^4^ are Hl(z), H2(z), E^{z),
E^{z),
E^{z),
where a„ a 2 , a 3 are the positive roots of A2 obeying aj = 2, / = 1,2,3 (see fig. 1). The relation between these generators and the generators in the Gell-Mann basis J"(z), a = 1,2,..., 8, and their mutual OPE's are given in appendix C. The genera tors E"(z) are realized as vertex operators H'(z) = /
E"(z) =
c_a(Cia^)(z), i-l,2
a(=A (4.1)
(see ref. [25] for details). It is now straightforward to derive explicit expressions for the fields Q"(z) and Q(z) for A^ in this realization. The field Qa(z) can be evaluated by using the lemma (C.l) and the list (B.14) of ^/-symbols for SU(3). In the Cartan-Weyl basis its components are Ql(z)=-lJ6i(HW)(z), Q\z)=-\j6i(HW-HW){z), Q±°iz) = i((yrH)E±°<)(z), /= 1,2,3.
(4.2)
505
360
F.A. Bats et at. / Extended Virasoro algebras (I)
The vectors y, (/= 1,2,3) obey (see fig. 1) Y,-«,-0,
VY,«?.
(4.3)
Again using (C.l) we derive
Q(z)--iA3(l){
E (H'Q>)(z)+ Z(E'Q-' + E-'Qm)(')) W-1,2
a>0
'
=7 ( 3 V ( W ) "V( W))(*)-
(4.4)
6 This formula expresses the third-order Casimir operator Q(z) of the full A^ algebra in terms of the generators of its Cartan subalgebra only! Note that if we evaluate a similar expression for the Cartan subalgebra only we find a result which is proportional to (4.4) but smaller by a factor of 10 G CARTAN ( 2 )
=
-iA,{\)[dn2{H\HxH2)
+ H\H2Hl) +
+
H2{HW)){z)
d222{H2(H2H2))(z)\
-i^(-^)(mH>H2)-H2(H2H2))(z)
= -■kQ(')-
(4-5)
This situation is reminiscent of a similar proportionality for the 2nd order Casimir operator in the usual Sugawara construction [25]. It was noted in [20] that the operator Q(z) as given in (4.4) satisfies the OPE 2/3 (z — w)
2T(w)
8T(w)
(z — w)
(z — w)
+ TJ-T5(A(>v) + ^2r(>v)) (z-w) {L2dA(W) + i-idiT(w))+---.
(4.6)
z—w
In section 2 we derived that for general k the OPE of Q(z) and Q(w) is similar to
506
F.A. Bats et al. / Extended Virasoro algebras (I)
361
(4.6) but with an extra primary field R4(z) coming in at the level (z - w)~2. The combination of both observations shows that the field R4(z) vanishes identically for N = 3 in the vertex operator realization. This result can be checked directly by inserting the realization (4.1) into the expression (3.2) for the field R4(z). By repeatedly using the lemmas (C.4) and (C.6) for evaluating normal ordered products of vertex operators and the rearrangement lemmas in appendix A we verified that indeed R4(z) is identically zero in this realization. We stress once again that the occurrence of new primary fields in the OPA is not unusual. Also in the free field realization of Fateev and Zamolodchikov new primary fields occur in the regular part of die OPE. So, although (4.4) gives a realization of the commutator algebra, it is not a realization of the full OPA proposed by Zamolodchikov in [19]. 5. Discussion and further developments We have shown that a consistent operator product algebra can be made out of the Sugawara stress-energy tensor and a dimension-3 primary field, corresponding to the third-order Casimir of SU(3). Up to now we have only discussed how the algebra can be realized unitarily on integrable HWM's of the A^ Kac-Moody algebra, thereby restricting the central charge in the Virasoro algebra to c=^-j7j>2,
*-l,2,3,....
(5.1)
We have shown that for c = 2, corresponding to the vertex operator realization, we have full agreement with the algebra and its realization occurring in the work of Fateev and Zamolodchikov. To make contact with the series (1.10) of completely degenerate representations one would have to generalize the GKO coset-construction to this spin-3 algebra, at least for the diagonal subalgebra of A2®A2. In particular one would like to find the coset analog Q of the dimension-3 operator such that Q is primary w.r.t. the coset Virasoro and commutes with the Kac-Moody sub-algebra, in this case the diagonal A2. It turns out that such a Q can be constructed [26]. This paves the way towards a complete treatment of the series (1.10), including the determination of characters and classification of modular invariants, using a generalization of the finite reducibility theorem [27]. (This was the motivation in [7] to suggest the investigation of existence of higher order Casimir algebras.) It is obvious that the construction we explored is not restricted to A2 but can be applied to every Lie algebra g, assuming one includes all (independent) Casimir operators. For AN_V N > 3, one can already see the fourth-order Casimir emerging in the OPE of two third-order Casimirs, because the AN_l analog of (B.12) contains a rank 4 symmetric tensor characterizing the fourth-order Casimir. It is clear that
507
362
f[A. Bais et al. / Extended Virasoro algebras (I)
the actual computations with the techniques of this paper become rather cumber some, but one might hope to construct some kind of Feynman diagrammatic techniques along the lines of [28] to shed light on the structure of these algebras. Assuming the computational difficulties can be overcome, one expects to find a realization or coset construction for which the other primary fields, which emerge naturally, decouple so that the OPA is determined by the set of Casimirs alone. Though we have no proof of this, we will spend the rest of this section explaining a convincing argument to support our expectation. Recently J. Thierry-Mieg constructed a BRST operator for the Zamolodchikov algebra by introducing ghosts for the dimension-2 stress-energy tensor and the dimension-3 operator [29]. A condition for this BRST operator to be nilpotent is that the central charge c = 100. This can be understood as the contribution of a dimension-2 and a dimension-3 ghost to the conformal anomaly. In general for a dimension-X ghost the contribution is c = 2(6X2-6X + l ) .
(5.2)
If we assume that the generalization of the Zamolodchikov algebra to all Casimirs of a Lie algebra exists, the critical value of the central charge for the corresponding BRST operator would clearly be* ccrit = 2 £ ( 6 X 2 - 6 X , + l ) ,
(5.3)
i-i
where X;, / = 1,2,..., / are the orders of the independent Casimir operators. On the other hand one can naively generalize the pattern emerging from the null-state construction of the dimension-3 algebra in [20]. One then ends up with the following value for the critical central charge of the higher order Casimir algebras [30] ccrit =
2/ +
4hdimG: =
2/(2h2 + 2h + l)
(5.4)
valid for all simply-laced Lie algebras g. In this, / is the rank of g and h is its Coxeter number. Equating this to (5.3) one arrives at the following equality £(6X 2 - 6X,. + l) = /(2h2 + 2h + 1).
(5.5)
In terms of the exponents e, = X, - 1, / = 1,2,..., / of g [31] we have 2 > , ( e , + l) = }/h(h + l ) . * P.B. wishes to thank J. Thierry-Mieg for pointing this out.
(5.6)
508
F.A. Bats el al. / Extended Virasoro algebras (I)
363
This relation can be checked exphcitly for all simply-laced g and turns out to be valid (to our knowledge this type of relation is not yet known in hterature). The validity of this relation strongly supports the belief in the existence of higher Casimir algebras and the generalization of the patterns emerging in the dimension-3 case. As a last observation we notice that (5.6) together with the well-known relation
I>, = */h
(5.7)
suggest further relations. Indeed, one can check that £ e , ( e , + l)(e, + 2) = i/h(h + l)(h + 2)
(5.8)
is also valid for every simply-laced Lie algebra. The relevance of (5.8) is however unclear to us. We would like to thank E. Verlinde for discussions on the OPE (3.4) for the free scalar field, P. Batenburg for discussions and pointing out ref. [19]. P.B. acknow ledges J. Thierry-Mieg, who is working on related ideas, for stimulating discussions. P.B. and K.S. are financially supported by the "Stichting voor Fundamenteel Onderzoek der Materie" (F.O.M.), and M.S. is supported by a SERC/NATO postdoctoral fellowship.
Appendix A First of all we adopt the usual convention that wherever we write the product of two operators at non-coincident points we implicitly assume that the operators are radially ordered. Furthermore the + • • • in OPE's always means the addition of regular terms of order in (z — w) at least one higher than the last term which is exphcitly written down. We have chosen to define the normal ordered product of two operators A(z) and B(w) at coincident points as {AB)(z) = —$—A(x)B(z). Z.1TI
J
z
(A.l)
X — Z
Interpreting the contour around z as the difference between two contours |*| > \z\ and \x\ < \z\ we find that the equivalent expression for the mode expansion coefficients is (AB)n=
Z
*pBn-P+
E
Bn_pAp
(A.2)
509
364
F.A. Bats el al. / Extended Virasoro algebras (I)
in which AA, AB etc. are the conformal dimensions of the fields A(z), B(z) etc. (A symmetrized version of (A.1) was used in [32].) If we write an operator product expansion for the two operators at distinct points „
(AB)(w) \r_\/+{AB)M+-~
A(z)B(w)-Z
(A.3)
we see from (A.l) that (AB)(z)={AB}0(z)
(AA)
so the normal ordering defined above is really the most natural from the OPE point of view. The contraction A(z)B(w) is defined as the singular part of (A.3) i
i
^
A(z)B(w)=Z
(AB}(w)
,
V
W>H-
'
^
One easily proves the following version of Wick's theorem for calculating the OPE of A(z) with a composite field (5CXw) A(z)(BC)(w)
= — <(,——{A(z)B
(X)C(W)
+ B(X)A(Z)C(W)}
. (A.6)
An analogous expression exists if we contract with the normal ordered operator on the left. In practice we used (A.6) and determined the other contraction by interchanging the operators in the OPE. We now proceed to establish two useful rearrangement lemmas which are of crucial importance when considering nested normal ordered products of more than two operators, such as (A(BC)\z). (i) Firstly, using the mode expansion (A.2) we can easily discover the surviving terms in the commutator ([A, B])(z). In modes
E E
K-*..-,] \B„-P>AP\
if
n^-AA-AB iln>-AA-AB.
Alternatively by reversing the arguments z and w in the expansion (A.3), and using
510 F.A. Bais et al / Extended Virasoro algebras (I)
365
Taylor expansions about w for the operators {AB}n(z), we can deduce that B(z)A{w)=
2L, L —; „
7
(A.8)
TT=M-+---
{BA),(w)
= E 1 rV+WoW+-.
(A.9)
Picking out the terms from (A.8) contributing to {BA}0(w) in (A.9), we find from (A.4) that ([A,B])(z)=
E Q-8'{AB)r(')-
(A10)
(ii) Next, using modes we calculate the expansion coefficients of (A{BC))(z) {B(AC)Xz), using (A.2). We begin (A(BC))n-(B(AC))n=
£
Ap(BC)m-,+
£
" E Bq{AC)n-q-
(BC),-^
E (^C),-^.
We continue using (A.2) for (BC)n_p, etc. and obtain eight terms, which reduce (with some relabelling of summation indices) to (A{BC))„-(B(AC))n=
E
L
[Ap,Bp_9]Cn_p
p+AB-\
+
E p>-A/t-A„
=
E q--A/t
C._,[B,_,,A,] +\
(([A,B))C)n.
That is to say (A(BC))(z)
- (B(AC))(z)
= (([A, B])C)(z),
(A.ll)
Clearly we can substitute from (A.10) to obtain an expression involving the fields [AB}r(z) from the OPE A(z)B(w). There are two points which should be noted from (A.10) and (A.ll). Firstly, in normal ordered products of three operators or more, we have to specify how the normal ordering is carried out between successive pairs of operators. Otherwise we
511 366
F.A. Bats el al. / Extended Virasoro algebras (I)
will be faced with an ambiguity since (A(BC))(z)-((AB)C)(z)*0.
(A.12)
Our convention for such normal ordered products is to nest the successive orderings according to the rule (ABC)(z) = (A(BC))(z).
(A.13)
(ABCD)(z) = (A(B(CD)))(z).
(A.14)
Thus for example
We refer to such a normal ordered product as fully normal ordered. Where some other nesting of normal ordering is required, this will be specified expUcitly, as in the right-hand side of (A.ll), for example. Secondly, using eqs. (A.10) and (A.ll), we can derive rearrangement lemmas for the interior nesting of higher order products, by iteration. For example ((AB)(CD))(z)
= ((CD)(AB))(z) = (A((CD)B))(z) =
([(CD),(AB)])(z)
- ([(CD),(AB)])(z)
+ (([(CD),
A))B)(z)
(A(B(CD)))(z)-([(CD),(AB)])(z) + (([(CD), A])B)(z) + (A([(CD), B]))(z)
(A.15)
which was used in sect. 4. Appendix B With respect to an antihermitian basis {Ta}, normalized according to Tr(7"T*)= -8ab
(B.l)
the /- and rf-tensors for AN_l are defined by fbc=
_Tr([r a , Tb]Tc),
dabc= -iTr({Ta,Tb}Tc).
(B.2)
(Our conventions are related to those of ref. [33] by a factor of Jl). They satisfy the following properties (i) fabc is totally antisymmetric, dabc is totally symmetric and traceless daab = 0.
(B.3)
512
F.A. Bais etaL / Extended Virasoro algebras (I)
367
(ii) Normalization fabcfdbc=1N8ad^
(g 4 )
2 dabcddbc=—(N2-4)8ad.
(B.5)
N (iii) Triple contractions (iii) Triple contractions fadbfbecfcfa _ _ jfjdef ^
(g
jadbfbtyc/a
( g 7)
=
_ ^jd*/ (
6)
/tf2-4\ dadbdbecfcfa
_
yd*/ ^
( g g)
iV 2 - 12' dadbdbecdcfa
=
|
|^
(39)
(iv) Jacobi identities fadepbc
+
jbdepca + fed*f tab = Q ^
( g JQ)
fad^ebc
+
fbdejeca
(g
+
fede^ab
=
Qf
n
)
(v) A relation only valid for A2 dabcddec = *(8ad8b' + 8"' 8bd - 8ab 8de) + L^fdJfW+ fff
(B.12)
In the Cartan-Weyl basis for A2 the generators {H\ i' = l,2, E±a\ j= 1,2,3} satisfy
[#',#>] =0,
[£°,£"] = /o-/f 10
a+0=O otherwise.
(B.13)
513 368
F.A. Bats et at. / Extended Virasoro algebras (I)
In this basis the -symbols take the following values
«.-«. 2 = - 1 , 7 6 ,
da*-a*2 = d">-a>2= \iyf6 ,
rf«.«2-«, = -«.-«2«3= _ / .
(B.14)
Appendix C In this appendix some technical aspects of the vertex operator realization of the level 1 representations of A^_x are gathered. Starting from the free fields
i=
£«(*) = c_ a (e"*)(z),
l,2,-..,N-l, aeA,
(C.l)
where A is the set of N2 - N roots of AN_l. The details of this construction and the properties of the quantities ca can be found in [25]. Together the generators (C.l) form a so-called Cartan-Weyl basis for the Kac-Moody algebra A§\. t . Their OPE's are H'(z)H'(w)
#'(z)£°(w)
8>J (z-w) a'Ea(w) z—w 1 (z-w)
Em(z)E*(w) = {
j+-
(a-H)(w) —-+•■• z-w
a +0 = O
E"+"(w) e(a,p) regular
—-+••• z—w
(C2) a + ]8ed otherwise.
For A^ the explicit relation of the current components in the Cartan-Weyl basis
514
F.A. Bais etaL/
with the Gell-Mann basis J\z)
Extended Virasoro algebras (I)
369
reads
Hl(z)-iJ3(z),
H2(z) =
iJ\z),
(z)--j=(Ji±iJ*){z),
E± +
-jT(ji±iJi)(z))
E±°>(z) =
E±°>{z) = -^{j*±iJ%z).
(C.3)
The following expressions for the normal ordered products of vertex operators are useful (£«£-« + E-"Ea)(z) = (a • H (£»£* +EiEl>)(z) =
)\z), e(f},y)(((fi-y)-H)E^)(z) if/S + y e d ,
(«\-H)E-)((\-H)E-) = £ * ( « • H)\z)
+
(C.5)
(«»-a))(z)
- f (X • «)((X • H)(a ■ H)3)(z) + ((X • H)\a • H)2)(z)
+ }x(a • dH)\z)
- (X • a)((X • 8H)(a ■ 8H))(z)
+ \X((a.d>H)(a-H)){z)
+
({\-d*H)(\.H))(Z)
-(\a)((\d2H)(a-H))(z)-^a)((\-H)(ad2H))(z),
(C.6)
where x = X2 + (X • a) 2 . These relations can all be derived by explicit multiplication of the vertex oper ators at distinct points, subtracting the singularity and applying l'Hopital's rule in the limit that the two points coincide [25]. To derive (C.6) one also needs (A.15). References [1] D. Friedan, Z. Qiu and S. Shenker, Phys. Rev. Lett. 52 (1984) 1575; in Vertex operators in mathematics and physics, eds. J. Lepowsky et aL, p. 419 (Springer, 1985); Comm. Math. Phys. 107 (1986) 535 [2] J.L. Cardy, Nud. Phys. B270 [FS16] (1986) 186 [3] A. Cappelli, C. Itzyiuon and J.-B. Zuber, Nud. Phys. B280 [FS18] (1987) 445; Comm. Math. Phys. 113 (1987) 1
515
370 [4] [5] [6] [7] [8] [9] [10] [11] [12] [13] [14] [15] [16] [17] [18] [19] [20] [21] [22] [23] [24] [25] [26] [27] [28] [29] [30] [31] [32] [33]
f.A. Bate et al / Extended Virasoro algebras (I) A. Kato, Mod. Phys. Lett A2 (1987) 585 P. Goddard, A. Kent and D.I. OUve, Phys. Lett B152 (1985) 88; Comm. Math. Phys. 103 (1986) 105 D. Gepner, Nucl. Phys. B287 (1987) 111 P. Bouwknegt, Amsterdam preprint ITFA 87-05 (March '87) P. Bowcock and P. Goddard, Nucl. Phys. B285 [FS19] (1987) 651 R. Dijkgraaf, E. Verlinde and H. Verlinde, Utrecht preprint THU-87/17 (July '87) P. Ginsparg, private communication J. Wess and B. Zumino, Phys. Lett B37 (1971) 95 E Witten, Comm. Math. Phys. 92 (1984) 455 A.A. Belavin, A.M. Polyakov and A.B. Zamolodchikov, Nucl. Phys. B241 (1984) 333 D. Gepner and E. Witten, Nucl. Phys. B278 (1986) 493 F.A. Bais and A. Taormina, Phys. Lett. B181 (1986) 87 P. Bouwknegt and W. Nahm, Phys. Lett B184 (1987) 359 W. Nahm, in ICTP series in theoretical physics, Vol. 2, eds. Furian et al., p. 364 (World Scientific, 1986) W. Nahm, Stony Brook preprint, ITP-SB-87-7 A.B. Zamolodchikov, Theor. Math. Phys. 65 (1986) 1205 V.A. Fateev and A.B. Zamolodchikov, Nucl. Phys. B280 [FS18] (1987) 644 H. Sugawara, Phys. Rev. 170 (1968) 1659 V.G. Knizhnik and A.B. Zamolodchikov, Nucl. Phys. B247 (1984) 83 P. Goddard and D.I. OUve, Nucl. Phys. B257 [FS14] (1985) 226 I.T. Todorov, Phys. Lett B153 (1985) 77 P. Goddard, D.I. OUve, Int I. Mod. Phys. Al (1986) 303 F A Bais, P. Bouwknegt, K. Schoutens and M Surridge, Nucl. Phys. B304 (1988) 371 P. Goddard, W. Nahm and D.L OUve, Phys. Lett B160 (1985) 111 P. Cvitanovic, Group theory, Nordita notes (1984) I. Thierry-Mieg, Cambridge preprint DAMTP 87-14 P. Bouwknegt, unpublished V.G. Kac, Infinite dimensional Lie algebras (Cambridge University Press, 1985) M. Bershadsky, Phys. Lett B174 (1986) 285 A.J. Macfarlane, A. Sudbery and PH. Weisz, Comm. Math. Phys. 11 (1968) 77
516
Reprinted with permission from Nuclear Physics B Vol. 304, pp. 371-391.1988 © 1988 Hsevier Science Publishers B. V. (North-Holland Physics Publishing Division)
COSET CONSTRUCTION FOR EXTENDED VIRASORO ALGEBRAS FA. BAIS, P. BOUWKNEGT and M. SURRIDGE Institute for Theoretical Physics, University of Amsterdam, Valckenierstraat 65, 1018 XE Amsterdam, The Netherlands
K. SCHOUTENS Institute for Theoretical Physics, University of Utrecht, Princetonplein 5, P.O. Box 80 006, 3508 TA Utrecht, The Netherlands Received 5 October 1987
We discuss extensions of the Virasoro algebra obtained by generalizing the Sugawara construction to the higher order Casimir invariants of a Lie algebra g. We generalize the GKO coset construction to the dimension-3 operator for g"AN^l and recover results of Fateev and Zamokxkhikov if N — 3. Branching rules and generalizations to all simple, simply-laced £ are discussed.
1. Introduction In a previous paper [1], henceforth referred to as I, we discussed extensions of the Virasoro algebra which we constructed from Kac-Moody algebras g by generalizing the Sugawara construction to higher order Casimir invariants of the underlying finite dimensional Lie algebra g. This was done in an attempt to understand the occurrence of larger symmetries in d = 2 conformal field theories and their implica tions for the physical spectra. The starting point in I was a conformal field J(z) taking values in a Lie algebra g. Its components J"(z), defined with respect to an antihermitian basis {Ta, a = l,2,...,dim(g), Tr(7"T*) = -Sab), satisfy the operator product expansion (OPE) —kSab
Jc(w)
^Mw).T—?+r.-U-+....
(!,)
The Fourier modes J" satisfy the commutation relations of an untwisted affine
517
372
F.A. Bats et al. / Extended Virasoro algebras (II)
Kac-Moody algebra g. We proposed to consider the operators T^{z)
=^ ( X '>(g, k) dab< • ( J"(jb(jc(...
)(z),
(1.2)
where Jf(X'\g, k) is some normalization constant and dabc- is the completely symmetric invariant tensor of order A, (ii = 1,2,...,/ = rank(g)) of g, so that b c T(K) = d'hc T"T T ... is the X^th order Casimir of the underlying Lie algebra g. In particular, the operator T(z) = Ti2)(z) is the usual Sugawara stress-energy tensor satisfying the OPE T(z)T(w) = f^—^
+—
(z-w)
^
+ -—Mr + ■ • •
(z-w)
(1.3)
(z-w)
with central charge c(g
'*
) =
fcdim(g) fr + g '
(L4)
when the normalization is chosen as
In these formulas g is the dual Coxeter number of g [2]. It is not very hard to show that the other fields r (X() , / = 2,3,...,/, are primary fields w.r.t. T(z) if the
= E i ^ L r>0(2-
W
+0(,-w).
(1.6)
)
Let us denote by S the set of currents generated this way. The following is obvious i. r (X '>(z)GS, 2. 1 G S, 3. A(z)(=S=>dA(z)<=S, 4. A ( z ) , J ( : ) G S = » ( ^ X z ) 6 ^ A case of special interest is when S is the minimal set of currents obeying these requirements, i.e. when all the fields generated in the singular part of OPE's can be written as normal ordered products of the TiX<\z), i = 1,2,..., /, and their deriva tives.
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F.A. Bais etal. / Extended Virasoro algebras (II)
373
The set S together with the products { )r: (A, B) -» {AB}r, r e Z >0 , can be viewed as an abstract operator algebra, which we will denote as Vir[g, k\ The operator algebra Vir[g, k] is equivalent to the commutator algebra of the Fourier modes A„=* $(dz/2iri)A(z)zn+AA~1. However, due to the presence of composite expressions this commutator algebra is not a Lie algebra in general (an exception is the case VirT^1*, k\). It is therefore not very natural to pass to a formulation in terms of components An in this situation; we will instead do the analysis directly on the level of currents A(z) and products { } r , r e Z > 0 . In this context we define a representation of Vir[g, A:] to be a linear map p from Vir[g, k] to a set S" of currents acting on some Hilbert space V such that (i)
P(1) = V ,
(ii) (iii)
P(dA)(z)
= d(p(A))(z),
^eVirfg,*],
p({AB)r)(z) = {P(A)p(B)}r,
r>0,A,Be=Vir[g,k].
In I we explicitly investigated the operator product algebra of the Sugawara stress-energy tensor r(z)=
2(*Tiy f i a v v 6 ) ( z ) '
a-?)
and the third-order Casimir operator T^(z)=jr^(A^llyk)dabc(ja(JbJc))(z),
for g = AN_! (for conventions-and method of calculation we refer to I). Apart from the result that T(z) satisfies the Virasoro OPE and that T (3) (z) is a primary field of dimension 3 we found that the OPE of T(3)(z) and T(3)(w) is given by m/
. ,, w
x
c/3
2T(w)
{z-wf l
(z-w) 1
4
(z-w)
(z-wf
[2b2A{W) + ±d2T(w)+RM(W)]
^jZ^[b2dA(w) + •■• ,
dT(w)
+ ^d3T(w) + ^dR^(w)] (1.9)
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F.A. Bais el at. / Extended Virasoro algebras (II)
where
A(W) =
(TT)(w)-±d2T(w),
c-cU*
N2 l)k
k)J
~
*--¥-
(110)
In the expansion (1.9), apart from the identity operator and its descendants, an extra primary field Rw(z) and a corresponding descendant field 8R(*\z) are present in the singular terms. For general N the field Rw(z) contains a term proportional to the 4th order Casimir of AN_V For N = 3, however, no independent 4th order Casimir exists and one therefore expects some simplifications. In I we have shown that in the vertex operator realization of the level 1 representation of A2l) the field R(4)(z) vanishes identically. This shows that for k = 1 the field /?(4)(z) plus the fields generated in OPE's with /?(4)(z) form an ideal in the complete operator algebra and can consistently be put equal to zero. Thus the operator algebra V i r ^ ^ l ] is minimal in the sense described above; we read off from (1.9) that it is actually equivalent to the algebra given by Zamolodchikov in [3] with c = 2. It was shown in I that in the vertex operator realization for A$\ k = l, the expression for T (3) (z) reduces to the free field realization of this operator as given by Fateev and Zamolodchikov [4]. Our main goal in this paper is to present an extension of the Goddard, Kent, Olive (GKO) coset construction of a so-called coset Virasoro algebra to the dimension-3 field T(3)(z). This will allow us to make contact with the results for c < 2 in [4]. In fact we expect that a similar extended coset construction can be given more generally whenever we have a Kac-Moody subalgebra g' c g. The operators resulting from this construction constitute a representation of an extended Virasoro algebra which we will denote by Vir[g, g', k]. In this paper we focus on Vir[gffig, g, (k, 1)] where g c g © g is the diagonal embedding. This paper is organized as follows. In sect. 2 we explicitly give the construction of the coset dimension-3 operator f0)(z) of V i r t ^ ^ ! ®A^Llt A^^k^ k2)]. For N = 3, k2 = 1, the operator product algebra is shown to reduce to Zamolodchikov's spin-3 algebra. In section 3 we present some results on the representation theory of Vir[gffig, g,(k, 1)] for simple, simply-laced g. We do not have a complete proof of these results but we give a number of non-trivial consistency checks which strongly support our formulas. In particular we will point out the relation of V i r l ^ ^ !ffiA^_lt A^>_ly(l,l)] with the parafermion algebras [7]. Sect. 4 deals with the branching rules for irreducible HWM's of gffig into HWM's of g ^ ffi Vir[g ffig, g,(k, 1)]. Also here we give no complete proof but we go through a number of convincing consistency checks, one of which is the construction of some
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375
modular invariants. In sect. 5 we end with some conclusions and remarks. An appendix is added to explain some of our notations.
2. Coset construction In this section we discuss how to extend the GKO coset construction [5,6] to the Casimir operators of higher conformal dimension. We make this explicit for the dimension-3 operator associated to Aty^x (N> 3) For N = 3 we compare the resulting operator product algebra with Zamolodchikov's spin-3 algebra. Before we address the construction of the extended coset Virasoro algebras let us first review the ordinary GKO coset construction. The construction starts from a set of currents (with central charge k) correspond ing to an untwisted affine Kac-Moody algebra g. The Sugawara construction (1.2) gives a field T(z) satisfying a Virasoro algebra with central charge c(g,k) as in (1.4). Let g'c g be a Kac-Moody subalgebra of g. Restricting the Sugawara construction to the currents corresponding to g' we obtain the Virasoro current T'(z) with central charge c(g', k1). The value k' is determined by the embedding g'c g through k' =jk where j is the Dynkin index of this embedding [9]. Now it is easily shown that the difference f(z) = T(z)-T'(z)
(2.1)
also generates a Virasoro algebra Vir with central charge c(g, g', k) given by c{g,g',k)
= c(g,k)-c{g',k').
(2.2)
An important property of ihe coset Virasoro algebra Vir is that in the commutator algebra it commutes with the subalgebra g'. This allows us to write every HWM L(A) of g as a sum over irreducible HWM's of the direct sum g' © Vir. It can be shown that an irreducible integrable HWM L{A) is finitely reducible into irreduc ible HWM's of g' © Vir if and only if c(g, g', k) < 1 [10-16]. This property is very powerful. For the diagonal embedding A[l) c A^ © A{^ at level (k, 1) it has been shown that most (if not all) properties of the Virasoro algebra can be derived from those of A^ by exploiting this embedding. For c(g, g', k) > 1 we have no finite reducibility in terms of g' © Vir alone. This indicates that for those cases we should look for an extension of the coset Virasoro algebra which includes more generators than f(z) alone. It is the aim of this section to provide such an extension which will allow us to extend the finite reducibility theorem beyond c(g, g', k) < 1. The following is a tentative definition of what we mean by an extended coset Virasoro operator algebra.
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For a given untwisted affine Kac-Moody algebra g let Vir[g, k] be the operator algebra generated by the Casimir operators T<x>\z) at level k. Let g' be a Kac-Moody subalgebra of g. The extended coset Virasoro operator algebra Vir[g, g\ k] should have the following properties (i) the generators of Vir[g, g', k] are local currents constructed by taking normal ordered products of the currents for g at level k and their derivatives. (ii) Vir[g, g', k] contains the Virasoro generators f(z) as in (2.1) and coset analogues f{X,)(z), i = 2,3,...,/, of T(X'\z) which transform under f (z) as primary fields of dimension X,. (iii) Mutual operator products of Vir[g, g', k] with the currents of g' are regular, i.e. in the commutator algebra Vir[g, g', k] and g' commute. Here we construct explicitly the dimension-3 operator contained in Vii[A^)_1 © ^/}-i» ^#-l.C^i. M l w n e r e ^ # - i c ^ / } - i ®^#-i is the diagonal embedding. De noting the generators of A^)_1®A(l!j)_1 as Jfaiz) and ^ ( z ) and those of the diagonal Afi^t as J'a{z) we have the relation J'°(z)=Jfo(z)+J?2)(z),
k' = kl
+
k2.
(2.3)
The Virasoro generator for Vir(>4JJLx ® A^_ly A$_1,(kl, k2)] is given by f(z) = Tm(z) + T(2)(z)-T'(z),
(2.4)
with T(1)(z) and r (2) (z) as in (1.6). The coset central charge is c= =
c(A%l1
*i
k^ + N
k2 + N
kl + k2 ki + k2 + N
(2.5)
In order to write down the coset analogue f0)(z) of (1.7) we inspect the requirements (i), (ii) and (iii). From (i) and (ii) we learn that r ( 3 ) (z) is a normal ordered product cubic in the Kac-Moody currents J°i)(z) and J^y(z) (it is easily seen that bilinear terms involving a derivative are no good). The requirement (iii) implies that T (3) (z) is a singlet under the underlying AN_r subalgebra of g'. This restricts us further to the terms (WDKZ).
{JhQvMz),
(WD)(*),
{JmQ'mM (2-6)
where Q°(z) = dabc{J"Jc){z)Notice that the combination T$(z) + T$(z) - T'°\z),
(2-7) which is the natural
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FA. Bais el aL / Extended Virasoro algebras (If)
377
analogue of f(z) in (2.4), does not satisfy the requirement (ii). We therefore allow a general linear combination of the terms appearing in (2.6) and proceed by imposing the requirements (ii) and (iii). Extensively using the results of I (in particular (2.11), (2.12) and the techniques of appendix A) we have found that the requirement that f ( 3 ) (z) is a primary field of dimension 3 under f(z) uniquely fixes f (3) (z) up to a normalization factor BN(/cj, k2): f<3>(z) = JBN(A:1,A:2){A:2(JV + A:2)(Ar + 2A: 2 )(^ ) e ( '' 1) )(z)
-HN + kJiN + kJiN + lkJiJhQfoKz) + 3(N + k,)(N + k2)(N + 2*1)(^)<2(<2))(z) -k^N + kJiN + lkJij^Q^iz)}.
(2.8)
It turns out that the remaining requirement (iii), expressed as f (3) (z)/'°(w) = regular,
(2.9)
is now already satisfied. The next step in our construction is to determine the structure of the operator algebra Vir[^<J>_i 9A$Llt A^_v{kx, k2)\, i.e. to calculate the OPE f<3)(z)f<3)(M'). After much arithmetic one finds
rc>(,)r«(*) = — i — j + —i-(y + — ^ 3
\z — w)
\z — w)
(z — w)
+ —^—I[2b2A(W) + ^d2f(w) + R^(w)] (z-w)
+ ■■■ ,
(2.10)
where A(w)-(ff)(w)-^82f(w),
b2=^jz
(2-11)
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F.A. Bats et al. / Extended Virasoro algebras (II)
provided the normalization is fixed as
**(*1.*2) =
3(N + kJiN + k2)(N + kt + k2)
X
N / V 2(N + 2ki)(N + 2k2)(3N + 2kY + 2k2)(N2 - 4) '
^"l1'
The field Rw(z) is a primary field of dimension 4 under f(z). Notice that the structure of the OPE (2.10) in Vii[A%i_1 © A^i^ A^l^ik^, k2)] is similar to that of the dimension-3 operator in Vir[i4j}Li, k], eq. (1.9). For general N the field Rw(z) will contain the coset version of the 4th order Casirnir of AN_V One therefore expects that for N = 3 the expression for Rw(z) simplifies. For general (kv k2) this is not the case but we found that the field R(4)(z) decouples from the theory if one of the levels (A^, k2) is equal to one! We derived this remarkable result by showing that if we put k2 = 1 and we explicitly insert the vertex operator realization for the level 1 currents J°2)(z) then the field /i (4) (z) vanishes identically. Let us briefly discuss some of the details of this calculation. First of all, for k2 = 1 many of the terms in Rw(z) vanish simply because they contain a multiplicative factor (k2 - 1). The remaining terms can be written as R*(z)
+ C2(^Ul)*$a)(*)
= C^k^R^R^iz) + C3(kl){j?2)R$°)(z),
(2.13)
where fl(3)a(z) = 3 ( J T ) ( z ) +fabc(jbdJc){z) RV)ab(z) = (l8ab8cd+24
- 2 d2Ja(z),
8ac8bd-%fcmf'"'m)(JcJd){z),
(2.14)
and Ct(kx) are some constants with the property C, (/c^ = 1) = 0 whose precise form is irrelevant for the following discussion. The fields R°-)ab(z) and R0)a(z) are primary fields of dimension 2 and 3 respectively (we remark that (J"R^)a)(z) is proportional to the field Ri4)(z) occurring in the expansion (1.9)). Furthermore, by inspecting the OPE's of Ja(z) with Rmab(w) and Ri3)a(w) one finds that Rm"b and R(3)a transform respectively as the 27 and the 8 representations of the SU(3) algebra generated by the Jg. By inserting the vertex operator realization of the currents J^(z) (remember k2 = 1) and using the techniques described in I one easily shows that both R(2)ab(z) and rt(3)o(z) vanish.
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379
We do not fully understand why the terms occurring in (2.13) turn out to have nice transformation properties under both f(z) and Jff but we believe that this observation is essential if one tries to generalize the present construction to the higher order Casimirs. The operator product algebra Wii[A^® A^\ A^\(m-3,1)], (m = 4,5,...) has thus been proven to be equal to Zamolodchikov's spin-3 algebra "W with central charge given by (2.5) C(m
>-2(1-^1))-
"-"• 5 -"
<215)
In the remainder of this section we summarize some results on the representation theory of this algebra [4], which form a starting point for the generalizations we present in sect. 3-5. These results were obtained by Fateev and Zamolodchikov, who constructed a free field representation in the spirit of Feign and Fuks [17], and Dotsenko and Fateev [18]. They considered highest weight modules L(h{i)) of "W which contain a highest weight vector |A(,)) obeying 4'>|A<'>> = /t<'>|/j<'>>, £0)|/,0)) = o,
«>0,i-2,3
(2.16)
where L<° = ^(dz/2iri)zn+'~1Tv\z). The main result of [4] is that precisely for the c-values give given in (2.15) there exist (completely) degenerate representations L M £ of iT with
1/2"
*ll s■*2-
>1
*l'
1/2
s2\
>1 r
[(m + l ) r - m f ] [ j
^][(m + l ) r - w « ] - 6
6in(i» + l)
'
K
'
[(m + l)(2r x + r2) -m(2sx + s2)] [(m + l)(2r 2 + rt) -m(2s2 + s^] 9m(m + l)/(2m + 5)(2m-3)
' (2.18)
such that the finite set of primary fields
e
e [•(? ?)]
(2.19)
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generate a closed operator algebra, with OPE coefficients that resemble the A2 Clebsch-Gordan coefficients. The construction we have given above clearly demon strates why it is that properties of A2 come into the game. In sect. 3 we will discuss how these representation theoretical results can be extended to Vir[g ©g, g,(/c,l)] for all simple simply-laced Lie algebras g. In particular we will give the analogues of the expressions above.
3. Generalizations It is rather cumbersome to find explicit expressions for the other extended Virasoro algebras Vir[g, k] and the coset algebras Vir[g, g', A:] by the methods we have explored for A^. In I we showed that the expression for T(3\z) in the algebra Virf^^, A: = 1] can be reduced to an expression depending only on the Cartan subalgebra generators, thus giving a free field representation which is determined by the d-symbols in the Cartan subalgebra only. Assuming that a similar reduction can also be done in more general cases we can try to obtain information on the extended Virasoro algebras by generalizing the free field construction as given by Fateev and Zamolodchikov [4]. Though we have not yet completed our analysis, the structure given below is seen to emerge. Independent arguments for this generalization were presented in sect. 5 of I. The main result is an expression for the conformal dimensions of primary fields $(/>> <7) which generate highest weight states for irreducible representations of the extended coset Virasoro algebras Vir[g © g, g,(A:,l)]. This information is then used in the following section to postulate branching rules for certain products of Kac-Moody representations. In the following we make frequent use of the notation of Kac and Peterson [2,19] concerning Kac-Moody algebra theory. The appendix contains a summary of notation and definitions. Let g be a finite dimensional, simple, simply-laced Lie algebra. Consider / = rank(g) free scalar fields
(3.1)
coupled to a background charge y". The stress-energy tensor T(z) = Ti2\z) reads T(z)= -]i8ab{d<pad
(3-2)
The central charge for its corresponding Virasoro algebra is given by c = /-24|y|2.
(3.3)
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F.A. Bate etal. / Extended Virasoro algebras (II)
381
iX
Let T '\z), i = 2,...,/, be the expression for a higher order Casimir in the free field realization. A set of highest weight states in the spectrum is provided by the vertex operators Vp{z) -= exp(i'/?
(3.4)
It is easy to see that the state ^(0)|0) is also a highest weight state w.r.t. /L^>„^jiiz»+x,-ir<x,)(z)\ of L£X|) eigenvalue, say, hiX'\fi). In order to construct null-states following Fateev and Zamolodchikov [4] we have to find solutions to A<2)(/0 = 1.
(3-5)
In principle we could take any background charge y, but the most natural general ization of the construction in [4] seems to be to take y = a0p, where p is the defining vector of the principal Al embedding in g defined in the appendix. In this case (3.S) allows for 2/ solutions j8-«±5„
1-1,2,...,/,
(3.6)
where a ± = i ( a o ± / « o + 2 )> a++a_=a0,
a+a_=-$,
(3.7)
and 5„ i - 1,2,...,/, are the simple roots of g. The fact that the vertex operators K, ( ± ) (*)-(e' B **»)(z)
(3.8)
have conformal dimension 1 assures that It* )K/±>(w) = a w | - L -
K/*>(W))
+•••.
(3.9)
Certainly (3.6) does not give all solutions to (3.5), but there is reason to expect that they are precisely the solutions such that T^(z)V<±\w) = dw
±
A - 1
K<±>(w) + ( z - w)
i
+ (3.10)
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F.A. Bais et al. / Extended Virasoro algebras (II)
This implies that the states
^
K | ( + ) ( Z l )
-^
K
'
< + ) ( z
"
) ,
'2'-'-"«^
( 0 ) | 0 >
(3
-U)
occurring in the Verma module with highest weight vector J^(0)|0) will be null states. The condition for these states to be non-vanishing is 2 a 2 + ( n - l ) + 2a + ( 5 / , 2 Y - ) 3 - / i a + 5 , . ) = - m - l ,
m,n = 1,2
(3.12)
This equation can be reduced to ( 5 „ fi) = a + (l - n) + a _ ( l -
m).
(3.13)
In terms of the fundamental weights A„ j = 1,2,..., /, of g the solution of (3.13) reads 0U.?,)«-(/>••« + +fc«-)A„
1-1,2,...,/,
/>„<7, = 0,1,2
(3.14)
Writing /> = £'_i/>,A, we can interpret the pt, i = 1,2,...,/, as the Dynkin labelling of a finite dimensional representation of g. It is convenient to add one more positive integer p0 to the set (/>,} and associate to it a dominant integral Kac-Moody weight p = L'^oPfA, e />* of level k = EU>,If one substitutes (3.14) into (3.4) the result is that degenerate representations L(p, q) of the free field algebra {T(X'\z)} exist for hm
{p,q)
= (/>«++ ? « - + « O P > Pa++ ? « - + «OP)
l-c
(3.15)
where c = /-24a2|p|2 = /-2ga2(dimg), 4g(dimg)
l-c 8g(dimg) 1 ± \\ 1 +
l-c
(3.16)
(3.17)
In general the operator product algebra of the fields 4>(p,q) corresponding to degenerate representations L(p,q) will involve infinitely many of the fields $ ( p, q). Taking however 2a\ = (m + Y)/m (or equivalently a2, = l/2m(m + 1)) where m = g + 1, g + 2 , . . . we find the so-called main sequence of minimal models [20] with c{m) = l 1 -
m(m + l) I'
m = g + l , g + 2,...
(3.18)
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F.A. Bais etal / Extended Virasoro algebras (II)
383
Since the coset charge c(g ©g, g,(m -g, 1)) of the diagonal embedding g c g © g equals c(m) (use (A.10)) we see that this main sequence is the one relevant for the coset algebra Vir[gffig, g, (m - g, 1)]. It should be possible to prove positivity by using this correspondence. Comparing the above with the results for g'=Alp leads us to the following claim. Let g be a finite dimensional, simple, simply-laced Lie algebra, g = g(1). The operator algebra Vir[g, k = 1] is minimal in the sense described in sect. 1. The Cartan subalgebra reduction of the vertex operator representation of Vir[g, 1], which has c = /, results in a free field representation of this algebra; It corresponds to the above construction with background charge 0, i.e. m -* oo. The coset operators f (X,) (z), defined for the diagonal embedding gdg®g at level ( m - g , l ) , m = g + 1,..., generate the operator algebra Vir[g, g®g,(m — g, 1)] which differs from Vir[g, 1] only through the value of the central charge which is now c = c(m) < / as in (3.18). These c-values, which correspond to the free field construction in the presence of a background charge with strength al = l/2m(m +1), are precisely such that unitary HWM's L(p,q) of the algebra exist. The unitary HWM's for c = c(m) are parametrized by dominant integral g-weights p and q of level m — g and m — g + 1 respectively. The fields ©
8
[*iP,q))
(3-19)
form a closed operator algebra. The conformal dimensions of the fields found by combining (3.15), (3.17) and (3.18), read h(2Xm) =
'•"
$(p,q),
((m + 1)^ - mq, (m + \)p - mq + 2p) 2m(ro + l) />ei>?-*,9eP?-*+1.
(3.20)
Precise information on how, the HWM's L(p, q) are contained in level (m - g,l) tensor product representations of g © g is provided by a branching rule which we present in sect. 4. If we write (3.20) in terms of the labels r,=/»,-+ 1 and s-t = q,, + 1 , / = 1,2,..., /, and the inverse Cartan matrix G of g the expression becomes }
((m-H)r < -/ny < )G < y ((/w-H)r < -w^ < )-(g/12)dimg 2m(m + l)
/■/,5, = 1,2
/ Ea'iKm-1,
/ X)a^<w.
i-l
i-l
(3.21)
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F.A. Bats et al. / Extended Virasoro algebras (II)
In this form it can more easily be recognized as a generalization of the dimension formula for the Virasoro algebra [21] and of (2.17) for g = A%\ We stress that the validity of (3.20) and (3.21) in particular hinges on the assumptions that Vir[(g © g, g,(k, 1)] exists and that eq. (3.10) holds. There is little doubt that the proposed formula is correct because it passes the following tests. (i) For all the c-values (3.18) in the region c < 1 [15] one can check that eq. (3.21) produces h(2) eigenvalues which are allowed by unitarity. Especially interesting is the case c(£„(1) © £g(1),(2,1)) = 21/22 where the h(1> values given by (3.21) give the subset of all Virasoro h-values at c = 21/22 contained in the non-standard modular invariant combination (Al0, E6) [22]. (ii) For \ii[A<^_ l © A$lx, A$_lf(1,1)] the values c(^)_1ffi^)_1,^L1,(l,l)) = ^ ^ ,
JV-2,3,...
(3.22)
exactly reproduce the set of c-values of the Z N parafermion algebras [7]. Moreover, in this case the h(1) values (3.20) agree precisely with the set given by [7,8]. By (3.20) we have
+ 2(N+l)(N
+ 2(N +
l)2t(l,m)},
k,l,m = 0,\,...,N-l,
(3.23)
+ 2)(£(k,k)-Z(k,l)-t(lc,'n))
where (N-a)b H ' -\(N-b)a
a>b a^b.
a b)
So for instance in the region
k^l^m
(N-k)(k-l) where
f(N-i)
ht= ; r-, ' 2N(N + 2)
1 = 1- m, k = k — m, 1 = 0,1,...,k,
k=
0,l,...,N-m-l.
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385
Formula (3.24) is precisely the result of ref. [8]. The other regions can be identified similarly. Let us conclude this section by making a remark about Viif(g ©g, g,(l, k)]. From the expression (3.20) for h(2>(p,q) it is clear that A(2) is at least invariant under the action of the automorphism group of the weight lattice of g which in particular contains the Weyl group W(g) of g. In general, however, the eigenvalues A(X,)(/>, q) of the higher order Casimir operators will break this symmetry. Consider for example the case of g = A2l\ By explicitly working out the action of the Weyl group one finds that A(2) is invariant under the order-6 group S3~W(A2) 2 3 generated by two elements R and S with R = S = 1 which act on the labels ' l as R:
Pi Pi
ql
P\
9i
Pi
\
H
ft. -
m-3-(pl+p2)
m
Pi
2 - ( ? i + <72) ft
(3.25)
It is however easy to check from (2.18) that A(3) is in general only invariant under 5. This breaks the symmetry to Z 3 [4]. This breaking also shows up if one computes the table of A(2) values for all p e P?" 3 , q e P?" 2 . One finds that the /i(2) values are either 3- or 6-fold degenerate. Those which are 3-fold degenerate have h(y) eigenvalue 0 whereas the 6-fold degenerates split into two sets of 3 with opposite A(3) eigenvalue. We expect that in the case g = A$_1 one should be able to prove in the same way that the symmetry of the coset model is ZN, which we know to be the case for the first term, i.e. Wu[(A^>_l © ^ J J L L J 4 $ - I , ( 1 , 1 ) ] where we have shown the correspon dence with the Z ^parafermion models.
4. Branching rules Let us from now on assume that for g simple and simply-laced the coset algebra H^— Vir[gffig, g, (m - g, 1)] can be constructed and that our formula (3.21) for the conformal dimensions of the fields is correct. As pointed out in sect. 2, one expects if to provide the additional structure necessary to extend the finite reducibility theorem for the diagonal embedding g<^g®g with certain c-values larger than unity. In other words, we claim that the irreducible HWM's of g ®g at level ( m - g , l ) (m = g + 1 , g + 2,...) are finitely reducible into irreducible HWM's of £dUg ® ^ a t l e v e l w - g + 1 for gjj.j and coset charge c(m) given by (3.18). Let X/T(p,?) be ^ character of the irreducible HWM L(p, q) of if, i.e. XUp.q)
1
lT
L(p,<,)H
'
2wir
(4.1)
531 386
F.A. Bats et at. / Extended Virasoro algebras (II)
where LQ is the zero component of the coset stress-energy tensor T(z). The full character also contains information on the L^ eigenvalue of the states, but the specialization (4.1) is sufficient for our purposes. We propose the following branching rule (4.2) qeP?-**1
for r G P\, p e P+~g, where the sum runs over all irreducible integrable HWM's L(q) at level m — g + 1 such that f + p - q is an element of the root lattice AR(g) of g. x£(A) denotes the character of the HWM L(A) of g in its homogeneous specialization [2,19] (i.e. only L0 eigenvalues). For g = A^ this branching rule is well-known [6]. Though the generalization (4.2) is presumably hard to prove we make four independent checks which provide strong evidence for its validity. (i) In order to prove that both sides of the branching rule (4.2) have the same transformation property under T -» T + 1 we have to check that the conformal dimensions on both sides of (4.2) match modulo positive integers. Let L(A) be an integrable HWM of g at level k = Z'_0aJ''«„ then (A,A + 2p) Therefore
*£& + *£&-*£»,-*£,.„ _ (m + 1)(p, p + 2p) -m(q,q 2m(m + l)
+ 2p)
((m + l)p - mq,{m + l)p - mq + 2p) (r, f + 2p) + 2m(m + l) 2(g+l) = -i(p-g.P~g)+0/
,,Ar,f+2p).
(4.4)
Now use that p - q= -r + a where a^AR(g), and that n = \(a,a) + (r,a)G Z>0 for simply-laced g. The expression (4.4) reduces to
2(g+l)
(g(r,r)-2(r,p)).
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F.A. Bais et al. / Extended Virasoro algebras (II)
387
It is not very hard to show explicitly that g(r, r) - 2(r, p) vanishes identically for all level 1 integrable HWM's L{r) of simply-laced g. This proves our assertion. (ii) In all the cases we checked (4.2) reproduces the well-known branching rules for tensor products of the finite dimensional representations of g occurring at the highest grade of the Kac-Moody HWM. It should be remarked that if one succeeds in proving (4.2) one actually has a generating formula for branching rules of tensor products of representations. (iii) One can use the branching rule (4.2) to construct modular invariant sesquilinear combinations of characters (string partition function). For details of this procedure of constructing modular invariants we refer to ref. [16]. For "W-= Vi^A^eA^, A$\(m-3,1)] the result is the following. First of all, the set { xT(p,t,)\P G P?~3>1G P?~2} ^ stable under the modular group. Secondly, there exist modular invariants of if labelled by three modular invariants H}$- of A^ at level k = 1, m — 3 and m - 2. If we use the explicit form of the two ^4^ invariants at level 1 [23] I: (1,1)+ (3,3)+ (3,3),
i.e. H^, = 8AA.,
II: (1,1)+ (3,3)+ (3,3),
(4.5) (4.6)
corresponding to the level 1 WZW models on the group manifolds of SU(3) and SU(3)/Z 3 respectively, the results are I: HZ:ff II: HZ:??
= H<;r»H$-»8((p-p>)-(q-q>)), = H%-»H%-»8((p+p')-(q
(4.7) + q>))y
(4.8)
where fi(\) is defined by «<*>-(i \0
X
! A ^ 2 ) otherwise.
(4-9) v '
If we use in particular Hffi. = 8AA. for both k = m - 3 and m — 2 we obtain from I P1< P
PP
Taking into account the redundancy in the labelling with p and q we can rewrite this as
^•;^~ 3 v.,^.v>.^)
(4.io)
which is precisely the "unitary" combination we would have expected to occur anyhow. As a second example, if one takes m = 4 (c = 4/5) and uses the known
533
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F.A. Bail elal. / Extended Virasoro algebras (II)
SU(3) and SU(3)/Z 3 invariants at level 1 and 2, the eqs. (4.7) and (4.8) give a total of 8 possibilities which can all be identified as either (4.10) or H
Z:?P - 8»°\ *« V - *«•> •
(4-n)
However, if we take into account only the T-dependence of the characters (as in (4.1)) both (4.10) and (4.11) reduce to the partition function of the 3-states Potts model (eq. (1.7) in I). From the analogy with the A^ case one might expect that (4.7) and (4.8) give all modular invariants for W. On the other hand, by using the result (4.10) one can for instance inductively construct the modular invariant partition function at level k for the SU(3)/Z3 WZW model by starting with the level-1 invariant (4.6). One finds successively k = 2:
(1,1) + (8,8) + (3,3) + (5,3) + (6,6) + (6,6),
k = 3:
(l + 10+T0\l + 10 + 10) + 3(8,8),
Jk = 4:
(1,1) + (8,8) + (27,27) + (10,10) + (10,T0) + (6,5) + (6,6) + (3,24) + (3,2?) + (24,3) + (23,3) + (151,I51) + ( I ^ l S j + (152,152) + (T52,152).
The k = 2 and k = 3 results were already given by Gepner and Witten [23]. It is clear that the above construction can be extended to all simply laced g [24]. It may even be possible to achieve a complete classification of all modular invariants this way. (iv) For the special case of g = A§) we have been able to show, by explicitly acting with the operator L^3) on the highest weight vector occurring on the l.h.s. of (4.2), that the /i(3) eigenvalues given in (2.18) are also in agreement with the branching rule (4.2)*.
5. Discussion In this paper we have shown that a coset construction for the 3rd order Casimir operator T (3) (z) of V i r l ^ ^ j , k] exists and we determined the corresponding operator algebra. In particular this determines the complete coset algebra Virf^^ © * In this way we discovered that eq. (5.6) in ref. [4] is wrong by a factor of 2.
534
Fjl. Bais etal / Extended Virasoro algebras (II)
389
A2l), A^,(ku k2)]. For k2 = 1 this algebra has been shown to reduce miraculously to Zamolodchikov's spin-3 algebra. We conjectured the existence of coset algebras Vir[g, g', k] for every Kac-Moody subalgebra g' of g and gave expressions for the conformal dimensions h(2)(p, q) of a main sequence c = c(m) of minimal models corresponding to the diagonal coset algebras Virfg 9g, g,(m — g,l)] for simple, simply-laced g. We also postulated branching rules for HWM's of g © g in terms of HWNTs of g^^ ffi Vir[g © g, g, (m -g.1)]. It is clear that a lot of work remains to be done in proving these conjectures (though a number of consistency checks have made them more than plausible) and extending them to all coset algebras Virfg, g', k] or even to super Kac-Moody algebras. We believe that a complete understanding of Virfg, g', k] might very well lead to a classification of all (rational) 2D conformal field theories, which would be of great interest in string theory and statistical mechanics. In all the work on 2D conformal field theory which has been done so far there seems to be an intriguing relationship among a triplet (i) a (rational) 2D conformal field theory. (ii) a coset pair (g, gO, (iii) an integrable lattice model. In this paper we have tried to work out the relationship between (i) and (ii). Concerning (iii) we can remark that recently Jimbo et al. [25,26] constructed a family of exactly solvable two-dimensional lattice models by extending the construc tion of "restricted solid on solid" (RSOS) models by Andrews et al. [27]. These models are based on the weight space of A^*_ v It is conjectured that the local state probabilities of these models in the continuum limit are related to the irreducible decomposition of characters for the coset pair (A$_i QAftLi, ^ $ - i ) as is known for N = 2 [28]. It therefore seems likely that the coset Casimir models we have constructed are the continuum limits of the RSOS models of Jimbo et al. It would be very interesting to unravel this correspondence and, in particular, to make explicit the higher symmetries in these lattice models.
Note added After completion of this paper we received a preprint by Fateev and Lykyanov [29] containing results for A$_r agreeing with ours in sect. 3. We also received a thesis by Hayasbi [30] who studied higher order Casimir operators. We would like to thank M. Jimbo for providing refs. [29,30] and O. Foda for interesting comments. P.B. and K.S. are financially supported by the "Stichting voor Fundamenteel Onderzoek der Materie" (FOM) and M.S. is supported by a SERC/NATO postdoctoral fellowship.
535
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F.A. Bais el aL / Extended Virasoro algebras (II)
Appendix In this appendix we give some conventions for our notation. We will follow mostly the conventions of Kac and Peterson [2,19]. An untwisted affine Kac-Moody algebra will be denoted by g, its underlying finite dimensional Lie algebra by g. A bar on a root or weight of g will always denote the corresponding root or weight in g. h and h* are respectively the Cartan subalgebra of g and its dual. The simple roots of g are {a„ z = 0 , 1 , . . . , / = rank g} c/i*. Their duals {a", i = 0,1,..., /} c h are such that the Cartan matrix atJ is given by a,, = <«,,<>.
(A.l)
The element p^h* is defined by (P,<> = 1,
i = 0,l,...,/,
(A.2)
and the central element c of g is given by
c-£«?«?,
(A.3)
i-O
where the dual coxeter labels a" constitute a left zero eigenvector of the Cartan matrix a i; . The dual Coxeter number g is defined by S=
(A-4)
(-0
The irreducible integrable highest weight modules (HWM's) L(A) are labelled by the integral dominant weights A: AGP+={\GA'|(A,<)eZ>0,
* = 0,1
/}.
(A.5)
Every A e P+ can be expressed as a sum A = L'_omi^i> where {A,} is a set of fundamental weights = «,,.,
i,;-0,1,...,/,
(A.6)
and the positive integers m, = (A, a") are the so-called Dynkin labels of the HWM. The level k of a A e P+ is the positive integer /
* = =2»,; i-0
(A.7)
536
F.A. Bais et al. / Extended Virasoro algebras (II)
391
we denote Pk+ = {AeP+,(A,c)
= k).
(A.8)
Finally, we often used the Freudenthal strange formula
2g
24
{A9
>
and a formula only valid for simple, simply-laced algebras g dimg = /(g + l ) .
(A.10)
References [1] [2] [3] [4] [5] [6] [7] [8] [9] [10] [11] [12] [13] [14] [15] [16] [17] [18] [19] [20] [21]
[22] [23] [24] [25] [26] [27] [28] [29] [30]
FA. Bais, P. Bouwknegt, K. Schoutens and M. Surridge, Nucl. Phys. B304 (1988) 348 V.G. Kac, Infinite dimensional Lie algebras (Cambridge University Press, 1985) A.B. Zamolodchikov, Theor. Math. Phys. 65 (1986) 1205 V.A. Fateev and A.B. Zamolodchikov, Nucl. Phys. B280 [FS18] (1987) 644 P. Goddard, A. Kent and D.I. Olive, Phys. Lett. B152 (1985) 88 P. Goddard, A. Kent and D.I. Olive, Comm. Math. Phys. 103 (1986) 105 A.B. Zamolodchikov and V.A. Fateev, Sov. Phys. JETP 62 (1985) 215 D. Gepner and Z. Qiu, Nucl. Phys. B285 [FS19] (1987) 423 F.A. Bais, F. Englert, A. Taormina and P. Zizzi, Nucl. Phys. B279 (1987) 529 V.G. Kac and D.H. Peterson, Proc. Natl. Acad. Sci. USA 78 (1981) 3308 P. Goddard, W. Nahm and D.I. Olive, Phys. Lett. B160 (1985) 111 P. Goddard and D.I. Olive, Nucl. Phys. B257 [FS14] (1985) 226 P. Goddard and D.I. Olive, Int. J. Mod. Phys. Al (1986) 303 P.G. Bouwknegt and W. Nahm, Phys. Lett. B184 (1987) 359 P. Bowcock and P. Goddard, Nucl. Phys. B285 [FS19] (1987) 651 P. Bouwknegt, Nucl. Phys. B290 [FS20] (1987) 507 B.L. Feigin and D.B. Fuks, Funct. Anal. Appl. 16 (1982) 114 Vl.S. Dotsenko and V.A. Fateev, Nucl. Phys. B240 [FS12] (1984) 312 V.G. Kac and D.H. Peterson, Adv. Math. 53 (1984) 125 A.A. Belavin, A.M. Polyakov and A.B. Zamolodchikov, Nucl. Phys. B241 (1984) 333 D. Friedan, Z. Qiu and S. Shenker, Phys. Rev. Lett 52 (1984) 1575; in Vertex operators in mathematics and physics, eds. J. Lepowski et al., p. 419 (Springer, 1985); Comm. Math. Phys. 107 (1986) 535 A. CappeUi, C. Itzykson and J.B. Zuber, Nucl. Phys. B280 [FS18] (1987) 445; Comm. Math. Phys. 113 (1987) 1 D. Gepner and E. Witten, Nucl. Phys. B278 (1986) 493 Work in progress M. Jimbo, T. Miwa and M. Okado, Mod. Phys. Lett. Bl (1987) 73 M. Jimbo, T. Miwa and M. Okado, Kyoto preprint RIMS-572 (April 1987) Lett. Math. Phys., to be published G.E. Andrews, R.J. Baxter and P.J. Forrester, J. Stat. Phys. 35 (1984) 193 E Date, M. Jimbo, T. Miwa and M. Okado, Kyoto preprint RIMS-548 (Sept. 1986) V.A. Fateev and S.L. Lykyanov, The models of two dimensional conformal quantum field theory with ZN symmetry, Landau preprint T. Hayashi, Sugawara operators and the Kac-Kazhdan conjecture, Thesis, Dept. of Mathematics, Nagoya University
537
Reprinted with permission from Nuclear Physics B Vol. 305 [FS23], pp. 685-709,1988 © 1988 Bsevier Science Publishers B. V. (North-Holland Physics Publishing Division)
COSET CONSTRUCTIONS AND EXTENDED CONFORMAL ALGEBRAS Peter BOWCOCK and Peter GODDARD Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Silver Street, Cambridge, CB3 9EW, UK Received 21 June 1988 (Revised 8 August 1988)
The structure of coset theories, and the extensions of conformal symmetry which they realise, is considered, using the properties of two special classes of fields, ft scalars and 0 scalars. Series of representations of extended conformal symmetry, associated with cosets of the form gx ffi "m/nm*y< where the subscripts denote the level of the affine algebra, and m runs over the positive integers, are discussed. Those theories possessing a field extending the conformal algebra of weight ij, where 1 < ij < 2, are listed. The ability of various coset models to be supersymmetrised is established using these techniques. The concept of a dual pair of cosets possessing related partition functions, but not sharing the same extended conformal algebra, is developed.
1. Introduction The conformal group plays a crucial role wherever it occurs as a symmetry of a two-dimensional theory. The generators of infinitesimal conformal transformations form two commuting copies of the Virasoro algebra 0 [Lm,Ln] = (m-n)Lm+n+t2cm(m2-l)8m,_n,
(1.1)
where the number e, called the central charge, is a characteristic of the theory. The states of a conformal field theory must fall into representations of the Virasoro algebra, v. It is often a physical requirement that the spectrum of L0 in each irreducible representation of 6 must be bounded below, and that L\ = L_n with respect to some positive-definite scalar product. Such unitary, highest weight representations exist if and only if either c ^ 1 or c is contained in the discrete series of values less than one [1,2], c = 1
~;
±,\t
4.1V
*-0,l,2,....
(1.2)
(m + 2)(m + 3) The theories which are easiest to analyse are those whose states fall into a finite number of irreducible representations of the Virasoro algebra, i.e. the theory is
538
686
p. Bowcock. P. Goddard / Conformal algebras
finitely reducible. An additional requirement, which seems to be physically moti vated in a variety of contexts, is that the partition function of the theory should be modular invariant. This places strong constraints on the combinations of representa tions of v that can occur. An argument of Cardy [3] demonstrates that, if a modular-invariant theory is finitely reducible under v alone, then the central charge must be less than one, and hence it must belong to the discrete series (1.2). The possible partition functions for such theories have been classified completely [4]. Although theories for which c £ 1 cannot be finitely reducible with respect to v. the states of such a theory might be related by some extension of the conformal symmetry, with respect to which the theory is finitely reducible. Such enlarged symmetries facilitate the study of a wide class of conformal field theories with central charge c ^ 1. It has been noticed that most known extensions of the conformal algebra occur as symmetries of coset theories. These two observations motivate the study of extended conformal algebras of coset models presented in this paper. The coset construction [2] relies on the relationship between affine Kac-Moody and Virasoro algebras to construct a Virasoro algebra associated with a pair he g of finite-dimensional simple Lie algebras. Denoting an orthonormal basis for the algebra g by {T"), normalized so that the length squared of long roots is two, we can define the associated Kac-Moody algebra, g, by the commutation relations [K, T„b] = ifabcT^n + xm8°»8mi _„,
(1.3)
where m, n e Z, fbc are totally antisymmetric structure constants for g and x is a central element called the level of g\ (For unitary representations and with the given normalisation x must be a positive integer; see e.g. ref. [5] for a review.) Using the Sugawara construction [6] we can construct a Virasoro algebra {£?*} given by j
*-P
dimg a-\
oo
/--oo
where 0s = x + h', h* is the dual Coxeter number for g and the crosses denote normal ordering with respect to the modes {T°}. The central charge associated with £" is c < s
- ^ £ . x + hg
(1.5)
It can be shown that cg ^ rank g so that it cannot belong to the discrete series (1.2). However, the difference
539
P. Bowcock, P. Goddard / Conformal algebras
687
also satisfies a Virasoro algebra vK with central charge given by cK = cg- ch. (Note that the level ft is determined by the level x of g and the index / of embedding, y = Ix.) For suitable choices of g and h, the whole of the series (1.2) can be produced in this manner. In this discussion we have assumed, for the convenience of exposition, that both g and h are simple, but these and the following considerations are easily extended to cases where g and h are arbitrary compact Lie algebras. For each coset g 3 h and choice of level x for g, we shall assume the existence of a conformal field theory for which {Km} are the generators of conformal transfor mations. The theory consists of a subspace of states of the Wess-Zumino-Witten model [7], with symmetry algebra gLxgR, where gL,gR are two copies of g associated with the left- andright-movingparts, respectively. The space of states for this theory can be written ©x J f $ ; ® ^f\.. Here the space J^fx is an irreducible highest weight representation space for g at level x, for which the states, which are annihilated by T° for n > 0, transform under the irreducible representation of g= {TQ}, which is labelled above by the highest weight X. For a given x there is a finite number of possibilities for X. Now we consider decomposing the representation space Jf?xg\ with respect to the sub-algebra he g. This decomposition can be written
X.'.x- © < „ • . * ' * . „ ,
(1.7)
where the sum is over the representations of h that occur in the decomposition. The coset theory associated with gih has a space of states given by
^ * = 8
0 < , < y
(1-8)
If the sum is taken over each admissible representation of g at level x once, then the partition function for the resulting theory is modular invariant [8]. (There can be other modular-invariant theories associated with non-trivial combinations of repre sentations for g but we shall not consider these possibilities here.) In what follows, for simplicity of notation, we shall consider only the left-moving part. The Virasoro algebra vK acts in the space J^x.^ which falls into a finite or infinite number of irreducible representations of vK according to whether cK < 1 or 0*2:1.
It is of interest to classify series of theories which provide representations of the same extended conformal algebra. For example, the family of models associated with the coset su(2)2 © su(2)m/su(2)2+m (where the subscripts label the level of the Kac-Moody algebra) possess superconformal invariance for differing values of m [2,9]. Generalising from the form of the cosets in this and other examples of families possessing a common conformal algebra, a systematic method of producing such a series of models was given in ref. [10].
540
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P. Bowcock, P. Goddard / Conformal algebras
The construction involves cosets of the form gx®hm/hy+m and §x^hr is a conformal embedding, i.e. one for which K=&*-&h vanishes. The example given above falls into this category, together with a number of others that have recently received attention. An algebra with Z 3 symmetry and containing a confor mal weight-3 field has been put forward by Fateev and Zamolodchikov [11], and has been shown to be associated with the coset su(3)mffi su(3)!/su(3) m+1 [12,13]. The conformal weight-3 field is constructed using the third-order Casimir of su(3). This suggests that the coset construction for gm9 §1/§m+1 describes a theory with a conformal algebra extended by operators corresponding to the higher Casimir operators of g. The extensions of the Virasoro algebra are neither Lie algebras (nor Lie superalgebras) in the normal sense, their commutators involving infinite sums of products of the fields constructed from the Casimirs. More general algebraic structures, in which the operator product expansions involve branch points, can also be considered. The fields involved in such structures are generically referred to as " parafermions" [14,15]. The first such conformal system to be studied was a model possessing a ZNxZN symmetry. This has been shown to be associated with the cosets su(N)l © su(A'),/su(A r ) 2 [16]. The assumption that §.^h is a conformal embedding implies that the representations of §x are finitely reducible with respect to hy. It follows that we could in some sense associate the coset theory with h © hm/hy+m. However, we have to take together the appropriate representations of h to realise the gx symmetry so the ix ® hy/hy+m description is more natural. In sect. 2 of this paper, we study some general properties of coset theories. developing the approach of ref. [10] which in turn is related to suggestions put forward by Douglas [17]. In particular, we discuss the existence of fields, acting in the coset, which generate extensions of the conformal algebra. Amongst the fields, corresponding to states which are highest weight for both h and vK, are two complementary families of fields: A-scalar fields, commuting with h and extending the conformal algebra and 5-scalar fields, commuting with vK, which can be regarded as defining an extension of h. We can show that the two families commute. Next, in sect. 3 we consider the series of coset theories gx © h„/hy+„ possessing a common extended conformal symmetry and develop further the results of ref. [10]. We show that features of the coset construction of the superconformal discrete series hold in general, in particular that the hy+m scalars appearing for all values of m correspond to A^-scalar fields. The details of the analysis depends on the conformal weight r\ of the field extending the conformal algebra. A complete list of choices for (g, h), such that the corresponding theory contains a field with 1 < TJ < 2, is given in table 1. In sects. 4 and 5, we illustrate the ideas of sect. 2 by applying them to a variety of coset models. In ref. [18] a list of coset theories was given whose partition functions were expressible as a sum of products of characters for the superconformal algebra, strongly suggesting that the models possess superconformal symmetry. This is
541
P. Bowcock. P. Coddard / Con formal algebras
689
shown in sect. 4 by explicitly finding a fermionic spin- \ field and showing that its operator product expansion with itself closes to form the superconformal algebra. In sect. 5 of the paper, pairs of cosets are considered which are dual in a sense made precise in that section. Dual pairs share a common value of cK and there is a relation between the branching functions for the two pairs. An example of such a pair is su(2)m© su(2)„/su(2)m+„ and sp(m + n) l /sp(»i), © sp(n)i. The coset mod els associated with dual pairs do not in general possess the same extended conformal symmetry. In particular, for the example just given, it is shown that for n = 2 the first model possesses superconformal symmetry, while the second model does not except for an isolated value of m. In sect. 6 we offer some comments and conclusions.
2. The structure of coset theories A central concept in the theory of Kac-Moody and Virasoro algebras is that of a highest weight representation. An irreducible highest weight representation for the Virasoro algebra (1.1) is one which is generated by the action of the algebra on a state \
(2.1a)
M*> = \I<J>>,
( 2 -!b)
where h^ is the conformal weight of the highest weight state |
for n > 0 ,
(2.2a)
( 2 - 2b )
TO,->« *,'!+>>.
where M°- is an irreducible representation of g with highest weight X. The representation space is denoted J^fx, where x is the level of g. Consider the decomposition of some irreducible highest weight representation 3ff*x for a Kac-Moody algebra g with respect to hffi0K, where hag and vK is the coset Virasoro algebra defined by eq. (1.6). The representations of h and vK occurring in the decomposition are highest weight and unitary, and we can refine eq. (1.7) into
X'*x®K>®X'l*
-
(2-3)
542
690
where J^X.M
P. Bowcock, P. Goddard / Conformal algebras c a n De
written as the direct sum
•*x.,- © • * £ „ .
(2.4)
p
of irreducible representations of vK labelled by (cK, hp). So the pair (p, /i) labels a space of states Jfy^8Jf{ , which forms an irreducible representation for h®vK built up from some multiplet of states |WM) which are simultaneously highest weight for both h and vK. The field
* ( * ) - Y.Knz-"-\
(2.5)
acts in the coset space 3?x an<* indeed m each of the spaces J ^ M separately. We shall assume the existence of a coset conformal field theory acting in the spaces **"x,,i> f° r which K(z) acts as the generator of conformal transformations. We shall look for other fields which have a trivial action on the spaces JVh and only act in the coset spaces 3^x ^. A field with this property must commute with all of h and can be thought of as belonging to the coset theory. We shall call it an h scalar. Its modes will generate an extension of the conformal algebra for the coset theory. Similarly, the generators of h, and hence S£h, act non-trivially only on the spaces
**(*)= Y.2y-\
(2-6)
neZ
can be thought of as the generator of conformal transformations for some h theory. It is interesting to consider fields beside h which.have trivial action in the spaces 3fx M. These must commute with vK and therefore we shall call them 0 scalars. In order to consider other fields besides the currents of h Ta(z)=
£ r^-"-1
(2.7)
neZ
and K(z), we shall assume a one-to-one correspondence between states |i/») in Jr"g and a collection of fields i//(z) satisfying ^(z)|0)-e^-*'|^>,
(2.8)
where |0) is the vacuum state, the lowest state in Jff0g for which the corresponding field is the identity operator. The operator JS?_«, generates translations, satisfies the commutation relation
l*-V*(*)l-^. and annihilates the vacuum.
(2.9)
543
P. Bowcock, f. Codaard / Conformed algebras
691
It will be assumed that all the fields \p(z) are local with respect to T"(z), K(z), and hence L(z), in the following sense. Two fields are said to be local with respect to one another if A(z)B{$), \z\ > |f |, and B(j;)A(z), |f | > \z\ are related to one another by analytic continuation and the continuation is meromorphic at z = f. This operator product has the expansion A(z)B(n~ i ^ - n " ,
(2.10)
neZ
valid for \z - f | < |f | and |z| > |f |, and equal to B(£)A(z) if the latter inequality is reversed. The sum over integers in eq. (2.10) involves only finitely many negative values of n. The coefficients C„(f) in eq. (2.10) can be shown to be the fields associated with states \Cn). (For a discussion of this see ref. [19].) They can be evaluated using contour integration about a small circle about z = f. This can be rewritten
A*)B(t)(z-t) — l-^6
C„{t)-^-4 2lTl '\z\>\{\
B(!)A(z)(z-!)-"-1.
Ifl
J
\t\<\r\
(2.11) Acting with both sides of the equation on the vacuum, the second term is seen to be regular in z about the origin and thus vanishes, while taking the limit f -♦ 0 we find that \Cn)=A_n_iA\B),
(2.12)
where A(z) = I.neZAnz~n~AA, and AA is the conformal weight of A. It is therefore natural to denote the field Cn by A-„-&(B)(z). Now consider a field tfiz) corresponding to a simultaneous highest weight state |^,^M) for h and vK. By the above argument it satisfies the following operator product expansions about z = f
* ( * ) + r ( f ) = -f^T (z-s)
+
,
\ \ U-s;
+ 0(1).
1 -s^(z)^r(n = wr(n ;(z-n;:,2 + w(Q ;.'_,; + °( ). (*-« H ^ ^ f ) =
A/"^^(f) | y ; l f ) + 0(1).
(2.13a)
(213b) (2.13c)
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P. Bowcock, P. Goddard / Conformal algebras
where
Q is the quadratic Casimir for the representation n, y is the level of h, and hh is the dual Coxeter number for h. Also in eq. (2.13b) we have made use of the fact that &JMXz) = d^(z) which follows from eq. (2.9). Fields satisfying eq. (2.13b) are called primary with respect to the Virasoro algebra &*. Of particular interest are those fields ^/""(z) which behave like scalars under the algebra h. The matrix M°j vanishes in this case, so that the operator product expansion (2.13c) is non-singular. Using the usual contour-rearranging argument it is easy to see that the fields Ta(z)eh and 4>f°(z) commute. Thus the fields tf°(z) are h scalars. In order to see that these /i-scalar fields form a closed algebra in the operator-product-expansion sense, consider the following argument. Suppose that \pl and \p2 are two h scalars and that their operator product expansion has the form
V(zH2U) ~ £(* - n\U),
1*1 > If I •
(2-15)
Taking the limit f -+ 0, we have
* , (*)I* 2 >-I>U>-
(2-16)
n
If we act on the states on the right of eq. (2.16) with T°G.h, we can commute it past ^(z) and it will annihilate on |^2> if n £ 0. Thus the states \4>n) are annihilated by the non-negative modes of T"(z) 6 h, and so the corresponding fields are h scalars. Each of the ^-scalar fields \pp0 act in the coset theory, and can be considered as the generators of the extended conformal symmetry that the theory possesses. Indeed K(z), corresponding to the state A"_2|0), is a particular example of an A-scalar field. The operator SCh(z) commutes with h scalars and so K_l4>p0(z) d$p0(z). 0 Substituting this in the expansion (2.13a) we see that ty" is primary with respect to the Virasoro algebra 0K and that + r°(z)\0) = ezK-W°).
(2.17)
Thus the \f/p0(z) have all the properties of conformal fields with respect to the coset Virasoro algebra, vK. We shall now consider which of the fields corresponding to highest weight states for hffivK are scalars with respect to vK. For fields ip0*, corresponding to highest
545
P. Bowcock, P. Goddard / Conformed algebras
693
0
weight states l^ *) which are annihilated by K0, the leading term in the operator product expansion (2.13a) of ty°* with K vanishes, and it has the form ■K-I* 0 M (?)
*(*)*»(£)- (z-f)
(1)
f r |Z|>lfl
°
'
(218)
The state created from the vacuum by K_ ^"''(f) is AT_ ,|I//0M> and its norm satisfies
= 2(+°o\K0\+0») = 0.
(2.19)
Since we are working in a space with a positive-definite norm, it follows that the state K_1\\f/0'1) vanishes and, by the assumed one-to-one correspondence, so must the second term in the operator product expansion (2.13a). Since the operator product expansion (2.18) is non-singular, it follows that K(z) and ^ ( f ) commute. We shall call such a field a 6 scalar. Particular examples of v scalars are the k currents, T"(z), which correspond to the states Ta_ JO), T"_x^h. The collection of £ scalars extend the algebra h; they can be thought of as "pure" primary fields for h. The closure of 6 scalars, in the operator-product-expansion sense, can be proved in an exactly analogous way to the closure of h scalars. The v scalars ^°M(f) are primary not only with respect to the Kac-Moody algebra h but also with respect to the corresponding Virasoro algebra J?h, because K acts trivially on such fields implying that the actions of if * and if* are identical. We have isolated two complementary families of fields. The h scalars, including vK, form a family commuting with h; the 0 scalars, including h, commute with vK. in fact, all the members of one family commute with all the members of the other. This may be proved as follows. Suppose that <{>(z) and i|/(f) are v- and ^-scalar fields, respectively. Their conformal weights are given by jStf|*> = ]) =
2 (
^)l»).
W)-**)!*)-*,!*).
(2.20a) (2-20b)
where the states \4>) transform under the representation ft of h. (We suppress the labelling of the different states of the multiplet.) We suppose we can write the operator product expansion of $(z) and i//(f) in the form
^(n=EL(^-frx^) j «;>o
(2.2D
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P. Bowcock. P. Goddard / Conformal algebras
where the indices fij allow for the possible branch points in this expansion, and they are chosen so that pj - nk is not integral for j # k. Our objective is to prove that M, = 0. Considering the action of Sf£ on
*(*)!*> « E E^ + "lxi y ) >.
(2-22)
j niO
one deduces that
-gyixy > >-(* J > +
2(>,+V)
-My-HJlxl/')-
(2-23)
Because Jfm commutes with <j>(f) and |^) is a highest weight state for vK, it follows that each Ix'/') is also a i^ highest weight state with K0\x'nJ))-hp\x^).
(2.24)
On the other hand, since
(2.25)
where the matrices M" realise the representation /x of h and act on the suppressed index of
(2-26)
and combining this with eqs. (2.23) and (2.24), we deduce that each /iy = 0; that is the operator product (2.21) is regular at z = f, assuming that it can be analytically continued into the region \z\ < |f |. It follows that 4>(z) and i//(f) commute as claimed.
3. Coset theories of the form g®h/h In this section, we shall discuss the construction of series of coset theories possessing a common extended conformal symmetry following the approach of ref. [10]. The construction involves cosets of the form gxffihm/hY+m, where gx 3 hy is a conformal embedding, i.e. i ? * = i ? \ This implies that if we take g to be a simple Lie algebra then either g = h or x = \ [8]. The significance of the conformal embedding is that it ensures that the coset model that we construct is not factorisable in the following sense. Instead of directly decomposing gx®hm with
547
P. Bowcock, P. Goddard / Conformal algebras
695
respect to hy+m consider the following series of nested algebras gx®hmz> hy ® hm 3 hy+m. The coset model associated with the second pair is always non-triv ial, but the coset model associated with the first pair is trivial if and only if gx o h is a conformal embedding. If this is not the case then the coset theory associated with gffih/h is reducible into two coset theories associated with gx^>hv and h
y®
h
m/hm+y
As a preliminary to analysing the extended conformal algebra common to the whole series of theories gx®hm/hy+m for differing values of m, we first consider the particular example of the "supersymmetrisable" coset su(2)2ffisu(2) m /su(2) m+2 which was mentioned in sect. 1. The generators of su(2)2 can be represented in terms of free-fermion fields as \UiJk^J{z)^ik(z) and we shall denote the generators of the level m representation of su(2) by T'. In terms of these fields the fermionic generator of the superconformal transformations can be written G(z)=\UijkV{z)V{z)*k{z)+-T'(z)V{z). m
(3.1)
In the limit that m -» oo, only the first term remains. This term is a scalar under the rigid rotations generated by the zero modes of the generators of su(2). We shall now argue that the more obvious general features of eq. (3.1) hold in general in gx®hm/hy+m theories, that is (i) A +m-scalar fields 4>(z). associated with the extended conformal algebra common to the whole series, involve fields associated with gx together with only the currents associated with hm, and (ii) in the limit m -» oo these fields become /i-scalar fields within gx. To establish the former, we note that, if |<J>) is the representation of gxffihm with highest weight (X, i>) for g®h,
where N is a non-negative integer, and this must be independent of m. If we assume that X and v are constant as m -» oo it is evident that we must have Qr = 0, i.e. v = 0, in order for h^ to be independent of m. More generally, even if we allow X to vary, it is only permitted to take a finite number of values, and so there must be a subsequence of the sequence defined by the right-hand side of eq. (3.2) for which Qx is the same. Restricting attention to this subsequence, if v assumed an infinite number of values, h+ would be unbounded, whereas if it is restricted to a finite set, it can clearly only be constant if again v = 0. Thus |
548
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P. Bowcock, P. Goddard / Conforntal algebras
tion of g. If PN denotes the orthogonal projection onto the eigenspace -Sf0*- = N, for non-negative integers, A' I4>> =
E
^l*>.
(3.3)
h.zNzNo
for some N0 2: 0, and v;pN = pNv;,
T:PN
= pN_ j°n,
(3.4)
since V° commutes with JSf0*- and [7;°, JSf0A-] = «J„°. We wish to show that N0 = 0 and P0\) = 0 for
„>N0,
(3.5)
because, if it were non-zero, this state would be an eigenstate of &£" with a negative eigenvalue. Since \
n^O.
(3.6)
For N0 ^ n > 0, we apply PN _„ to eq. (3.6) to obtain {TnaPNo+V:PNo-n)\
(3.7)
and the second term is zero by eq. (3.3). Thus, combining this with eq. (3.5) W v » = 0 for n>0,
(3.8)
i.e. PN \<j>) is a highest weight state for hm in J^fx 9JfJl0. Hence either No = 0 with P0\
(3.9)
But r0° = 0 if &£~ = 0, so we deduce that ^ l ^ ) is an h scalar, TO*>
= 0.
(3.10)
To complete the argument we wish to show that \) -* Po\4>) as w -» oo. In eq. (3.6), as we take this limit, V" is constant whereas T° satisfies the defining relations [77, Tn°] = if °»
(3.11)
for which if0*- is bounded by some fixed JV, e Z
549
P. Bowcock, P. Goddard / Conformal algebras
697
as m -» oo, we have that -7=7?-<,
7y-»0,
(3.12)
where the a° satisfy the commutation relations
k , a j ] =/*•**,,_„.
(3.13)
Thus eq. (3.6) becomes in the limit K0"|4>> = 0,
<|*>=0,
n>0.
(3.14)
These latter conditions serve to determine 3fx\ in 3ffx\®3VyQ in the limit m -» oo and so, asymptotically, P0\4>) = \
(3.15)
We note that the first term in eq. (3.1) can be identified with the /yscalar ^ while the second term is proportional to T"_iV^(z). Since these two terms are
'
550
698
P. Bowcock, P. Goddard / Conformal algebras
clearly h ,.+m-scalars, and also since their weight is less than two, we need only check that eq. (3.6) is satisfied for n = 1. It is straightforward to show that the combina tion 1 . . * « * > - - 7 1 .Kfo m
(3.16)
is annihilated by 7"" + V° and so gives a general expression for the h scalar associated with an h scalar of conformal weight between one and two. If g = h, the requirement that an adjoint highest weight representation for /; exists constrains the level x = y to be greater than one. For the case in which g = h = su(2) and x=y = 2, the formula (3.2) correctly reproduces the weight of G(z). If g D h then x = 1 but, for the adjoint to be a permissible highest weight representation, we need y > 2. (If h is not simple then we need at least one simple component of h to be embedded in g at a level greater than or equal to two, and a field transforming under the adjoint representation of this component and trivially with respect to the other components.) An example of this situation is used in the coset construction given in ref. [10] of the DN symmetry algebra of Fateev and Zamolodchikov. In this construction, g and h were taken to be su(N)1 and so(N)2, respectively. Here there is a A-scalar field extending the conformal symmetry of the coset model of weight 1 + N — 2/N. It can be checked using the tables in ref. [20] that the adjoint representation of so(Ar) occurs in the decomposition of the second-rank antisymmetric representation of su( N), which is an allowed level-1 representation. The weight of the corresponding field is correctly given by eq. (3.7). Using the complete list of conformal pairs given in refs. [8,21], we can list all the cases which will contain an /i-scalar field whose weight lies between one and two. In order to do this we must consider all the non-trivial representations of g which are permissible at level 1, and decide whether their decomposition with respect to h contains an adjoint representation of h. For this to happen we know that at least one of the simple components of h must be embedded at a level greater than one. This reduces the number of cases we need to examine. The results are listed in table 1. For higher values of h^ (3.16) will contain more terms [10], and will not be discussed here. 4. SupersymmetrisaMe coset models In this section we use the concepts introduced in sect. 2 to investigate various coset models and show that they are superconformally invariant or "supersymmetrisable." Kac and Wakimoto [18] noted that for certain cosets g/h the decompo sition of linear combinations of characters for g could be written in terms of a finite number of terms which are products of characters for h and characters xsv for the
551 P. Bowcock, P. Goddard / Conformal algebras
699
TABLE 1
A-scalars of weight ij, 1 < JJ < 2 hy
g so(dimg) sp(M) su(M) su(3) K(N)
c2
V
«*•
i 2
su(M) 2 ®u(l) so(W) 2 »(3)4 $0(^-3)^80(3^
2 - 2/M + 2 M £ 2 2-2/M M>3
(A,),©^,), (A 2 ) 2 e(A 2 ),
F* g
(JC + 2 / I * ) / ( X + A»)
gx
x>l
super-Virasoro algebra
Lxix=£x*,„xs*V X
(4.1)
Xfi
Associated with each term on the right-hand side of eq. (4.1) is a highest weight state |4>xM> f° r " ® s v whose conformal weight with respect to the coset Virasoro algebra K is hx . Such a sum can be finite if and only if cK< § and in this case belongs to the superconformal discrete series discovered by Friedan, Qiu and Shenker 8 cjc-f 1 - _ , _ , ^ , m(m + 2)
m-2,3,4,....
(4.2)
This strongly suggests that the model posses superconformal invariance and so must contain a conformal weight- \ field. In each of the three examples, for which the decomposition is given expUcitly in ref. [18], we shall show that there is an h scalar of weight \ corresponding to the superconformal generator G(z) and, assuming that its operator product expansion with itself is merormorphic about z = f, we argue that it must be of the form G(z)G(!)~
7 ^ b + r ^ T + 0(1)
(*-s)
f° r M > l ? l ;
(4.3)
U-O
thus explicitly demonstrating the conjecture of superconformal invariance of the theory. We deal with the three examples in turn. Example 1. (E g ) 2 D (A 2 ) 2 © (E 6 ) 2 We shall label the irreducible representations of g in terms of the fundamental weights, X, where 0 s /' :£ rank g, for g = Eg, E6 and A 2 . The assignment of these fundamental weights to points in the Dynkin diagram is shown in fig. 1.
552
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P. Bowcock, P. Coddard / Conformal algebras
0
1
2
3
4
5
6
7
(X)
A l^»°2 a
Fig. 1.
The points labelled 0 correspond to the additional point needed to convert g to §. The value of cK is § which corresponds to eq. (4.2) with m = 5. We label the possible values of hx in the standard notation as hrs where 1 ^s^r^m-l and
h..=
[(m +
2)r-ms]2-4
8w(m + 2)
+ t«.
t = r — s mod 2.
(4.4)
The extended Dynkin diagrams for both A 2 and E 6 have a Z , symmetry, and we shall denote by a a generator of these two groups which we identify. The level-2 representations of E g have highest weights 2X0, Xj and X7. There are superconformal combinations of these, with decompositions as in eq. (4.1), as follows X2X0 + X x ' =
iL
(xMl2Xr +Xo(2M,)X«(>) + X«jJ<M,)Xr*(»',))x? >
(4-5a)
.-1.3 y-i.3,5
x£- E ( x ^ ^ x ^ , x ^ + x X A ) ) i , v (4-5b) ; -1,3 7-1.3.5
where in terms of the fundamental weights X,, /x, *= 2X0, /t3 = Xj + X2 for A 2 and v^ = 2X 0 , i»3 = X6, vi = X, + Xj for E 6 . If there is a superconformal algebra in this theory, the field G(z) must correspond to a state G_ 3 / 2 |0) in the representation of the superconformal algebra with the vacuum as highest weight; that is, it belongs to the representation with character x*h • Also, if G(z) is to act in the coset, it must be an it scalar, and so G_3/2\0) is the highest weight state for the representation of A 2 © E 6 whose character is X*2xff- The decomposition (4.5a) does indeed contain a term x^'X^X?,» ^d so any candidate for G(z) must belong to either the
553
P. Bowcock, P. Goddard / Conformal algebras
701
representation 2X0 or the representation X7 of Eg. It can not be the former because all states in the representation xfx n a v e integral eigenvalues with respect to if0E». The highest weight states in the X7 representation of Eg have conformal weight 0A7
= i
4 + 2/»£«
(4.6)
2
(where we also use X7 to denote the corresponding representation of Eg). It can be verified (e.g., using the tables in ref. [20]) that the decomposition of the X7 representation of E8 with respect to A 2 ©E 6 contains the scalar representation. The corresponding state \\ps) is an A scalar of weight f belonging to the "triv ial" representation of sv and thus must be proportional to G_ 3/2 |0). The only other independent h scalar \\j/'s) comes from the term x^'X^X**, and has weight h "4.1
= 21 16-
Since X7 is a real representation of Eg, it follows that the field yj>s(z) can be taken to be hermitian. The operator product expansion with itself, using the assumption of meromorphicity, must be of the form
Hz)+M)~-,
+
(z-nZ^3' ~(w)^ 12 + 7T-TT (*-n + O(l)
for
1*1 > l * l . ( 4 - 7 )
where A is a constant and B(f) and C(f) are A-scalar fields of conformal dimension one and two, respectively. There are no h scalars of weight one and the only h scalar of weight two is K(z) itself. Thus Z?(f) = 0, and we can choose the normalisation so that B(f) = K(£). Using Jacobi's identity we find A = \cK so that G(z) satisfies eq. (4.3) and our proof of the "supersymmetrisability" of this coset theory is complete. Following the analysis given in sect. 2, it would also be natural to see whether the decomposition (4.5) indicates the presence of v scalars associated with this coset. A v scalar is defined to have zero weight with respect to the coset Virasoro algebra K and so must be associated with terms containing \^ . There are non-trivial v scalars which are the highest weight states for the representations whose charactersare
,• Xs2(«t,)Xa>(i'1)X*liExample 2. (E g ) 2 D (G 2 ) 2 ©(F 4 ) 2 This case is rather similar to example 1. The value of the coset central charge is given by (4.2) with m = 9. The decomposition of characters is given by XO(MI)XO(»,)XA,
XSL+XS-
E
x^xfxs;,,
(4-*o
1-1.3,5,7 y-1.3,5,7,9
X5?-
I 1-1,3.5.7 y-1.3,5,7,9
xS'xfxl,,.
(4.8b)
554
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P. Bowcock. P. Goddard / Conformal algebras
where we have that /^ = 2X0, /i 3 = 2X2, /i 5 = X0 + X2, /x7 = Xj and ^ = 2X0, v3 = 2X4, fj — X0 + X4, r 7 » X3, P, = X r Again we can argue that G(z) is associated with the character Xx? ^ ^ X^xf'X*',, in «!• (4.8a). The representation X7 of E8 decomposes to give a singlet with respect to G 2 © F4, and this state is proportional to G_ 3 / 2 |0). All other arguments concerning G(z) are as for example 1. The only other /i-scalar field associated with xt' and x^'X^X**, in eq- (4.8b) has conformal weight 8 ^ . The model possesses no 0 scalars. Example 3. (£3\ © ( C ^ D (C 3 ) 2 The value for the coset Virasoro algebra is given by eq. (4.2) with m = 10. The decomposition of characters is given below Xx'Xx,3 + Xx3Xx,3 = (xx3+x, + Xx23+x3)x?5.6 + 2xx,5+x2X?,.4 + 2x^ + x,X? 3 . 2 . (4.9a) Xx'Xx3 + Xx.'Xx3 = (xx 3 + x 2 + Xx.'+Jx?,., + ( x S , + x S j x * , . , +
(xS, + x a i ) x 5 „ .
(4.9b)
xfcxfc + xfcxfc = (xS0 + xS,)(x^., + x?J +
yXxo+Xj + Xx,3+Xj J(x*v9 7 + X*v,, j
+ (xS, + xS1)()4., + JfS.l).
(4.9c)
xfcxS' + xfcxfc = (xS, + xS J(xy„ + x?,,) + (xS. + x&,)(x£, + x£,) + fex, + X^ + x 3 )(x?, 7 + X ? J . 2Xx 0 'Xxj
=
2XXO+AJ^XA,, 0 + X A , 2 ] + vXx03+x, + X X 2 + A J X A , ,
+ 2Xx%x2(x£,, + X*;,4)> 2Xx,3Xx2 =
(4.9d)
2XX,3+X2^XA3<
(4.9e)
+ X», 4 j + vXx03+x, + Xxj+xjx*,,
+ 2x^ 0 3 + x,(x?, 2 + X?7.2).
(4.9f)
555
P. Bowcock, P. Coddard / Conformal algebras
703
The terms in this decomposition containing the character x2x correspond to h scalars while the terms containing x" correspond to 6 scalars. There are h scalars associated with the terms X2X0XA51<
X2\0(iX*l, + X*91)> X2\0[Xhy, + X*,,]-
The field G(z) is in the "trivial" representation and is thus associated with the term X2A XA* 1 o n t n e "6"* °f ^ (4-9c). Because it has spin \ the corresponding state is in the representation of C3 © C3 labelled by the character Xx'Xx3 o n the left of eq. (4.9c). In fact, if the states which are primary with respect to the two copies of C3, and transform under C3 according to the representation A3 are denoted by |\ l 3 > and |X23 >, then it is clear that the state l*>-D* 3 3.,>®l* 2 3.,>.
(4-10)
i
is an h scalar and a calculation shows its conformal weight to be \. None of the other h scalars have weight one or two and so by the argument of example 1 we can assert that the model has superconformal invariance. In addition, the term x2x X*v,, m eq- (4.9c) indicates the presence of v scalars associated with the highest weight states for this representation of (C 3 ) 2 © sv. There are 74 states in the representation and their weight is \. They provide a kind of supersymmetric extension of (C3)2. We conclude this section by justifying the assumption of meromorphicity of the operator product expansion of the weight- * /i-scalar with itself in each of the three examples above. In the first two examples the h scalar corresponds to a highest weight state for the irreducible representation of (E8)2 labelled by X7. We shall show that all fields corresponding to highest weight states for the A7 irreducible representation of (Eg)2 have meromorphic operator product expansions with one another and, in particular, with themselves. To see this consider the embedding (Eg)! © (E 8 )! 3 (E g ) 2 . The central charge of the coset Virasoro algebra K is \ in this case, and so (E8)j © (E8)i is finitely reducible with respect to (E 8 ) 2 © vK. The decomposition can be written A2X0 X2X0
X2X0 X o ^ X X ,
Xl/16^XX7
Xl/2 •
V^- 11 ^
The (Eg), © (Eg), theory only contains the currents generating the affine algebra, which have meromorphic operator product expansions with each other. In particu lar, the decomposition (4.11) indicates the presence of a set of fields which correspond to simultaneously highest weight states for the irreducible representation of (E 8 ) 2 © vK acting on the space Jffff ® JCf^. We assume that each field in this set can be factorised into the product of an h scalar and a v scalar. The v scalar
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P. Bowcock, P. Goddard / Conformal algebras
corresponds to a highest weight state in the irreducible representation of (Eg)2 labelled by X7. The superconformal generator G(z) is such a v scalar. The h scalar has conformal weight \ and must correspond to a free fermion field y\>(z), so that
H^)Hi)--^—^
+ o{\),
\z\>\s\.
(4.12)
Thus we can find a field <j>(z) in the (E8)i © (Eg), that can be expressed as *(z)«G(r)*(z).
(4.13)
Both 4>(z) and t//(z) have meromorphic operator product expansions with them selves and because i//(z) and G(z) commute, this implies that G(z) has a meromor phic operator product expansion with itself. The third example is treated differently. As remarked in eq. (4.10), G(z) can be written as G{z)= ! # ( * ) * ? ( * ) .
(4.14)
/-l
where the fields \l/(z)),\j/(z)* correspond to states which are highest weight for the respective copies of (£3), and belong to the irreducible representation labelled by X3. The fields \l>)(z) and tfiz) can be represented using vertex operators, and one can use this to show that their operator product expansion is of the form
*?(* W ) - (* - n1/2[ j—^2 + - j ^ - + o c 1 ) } .
(4-15)
where b = {1,2}, Mfj is the irreducible representation for C3 labelled by \3, T"($) is the corresponding current in (C3)lt and 0(1) indicates terms which are regular at z = f. Combining eq. (4.14) with eq. (4.15), we see that the operator product expansion of G(z) with itself is meromorphic. 5. Dual pairs of cosets It has been pointed out in the mathematical literature [18,22] that between certain pairs of cosets sharing the same central charge there exists a form of duality. For example, in ref. [18] it is pointed out that the central charges associated with sp(m + /i)j/sp{m)i ©sp(n)j and su(2)mffisu(2)„/su(2)TO+), are equal and in the decomposition of these cosets, the same representations for the coset Virasoro algebra occur. This is an example of a dual coset pair which we shall define below. It is natural to ask whether the coset models associated with each of these cosets are related and in particular whether the extended conformal symmetry associated
557
P. Bowcock, P. Goddard / Conformed algebras
705
with each of these models is the same. Using the methods of sect. 1, we shall show that this is not the case. In particular it is shown that while (su(2) m ©su(2) 2 )/su(2) m+2 is "supersymmetrisable" the dual coset sp(m + 2)!/ (sfXm)! © s p ^ ) ^ is not so (with the exception of the case m = 8). We define the pair of cosets (gx, hy),(gx., h'y.) to be dual if there exists an affine algebra G such that both GDgx®h'y,,
(5.1a)
6 =>*,«&,
(5.1b)
are conformal embeddings. It follows that for each of the embeddings gx?hy
(5.2a)
gx,Dh'y,
(5.2b)
G^hy®h'y.®vK,
(5.2c)
the coset Virasoro algebra vK has the same central charge. Now consider the character decomposition of the embeddings (5.1) and (5.2), X?(T,«,*')- E^XJ(T,*)X;'(T,*'),
(5.3a)
X ? ( T , M ' ) - E™„X!(T,*)XJ'(T,»'),
(53b)
y.p
xX(T,*) = E6tf*(T) X :(T,*),
(5.3c)
r
= Zbpg/h'(^')xh,(r',e'),
Xf(r',8')
xf(T,«,»')-
EX!(T,C)XJV.«')X;(T),
(5.3d) (5.3e)
y.p
where bf/,h, b^/h' are called the branching functions for the cosets (gx, hv),(gx., h\.) and are a small of (possibly infinitely many) characters for vK. Substituting eq. (5.3c) into eq. (5.3a) and eq. (5.3d) into eq. (5.3b), comparing these equations with eq. (5.3e) and utilising the independence of characters we have that
XJ,(T)=E«^(T)=Im^(T). x
P
(5#4)
558
706
P. Bowcock, P. Goddard / Conformal algebras
This is the relationship between the branching functions for dual coset pairs. Now let us consider the example mentioned above. We see that if we set G = so(4n + 4m) 1 ,
(5.5a)
g = sp(m + n)i> g' = £(2) m ©s^(2)„,
A = sp(m) 1 ©sp(n) 1 ,
(5.5b)
h' = w(2)m+n,
(5.5c)
then the pair sp(n + w)/sp(«)ffisp(m) and su(2)m© su(2)/»/su(2)()I+m) is dual in the sense defined above. The notation for labelling the representations of these algebras is defined as follows. The trivial and vector representations of so(4«) are labelled 0, v, respectively. These are n + 1 minimal representations for sp{n)1 and these are labelled from 0 to n. Similarly, there are n + 1 different irreducible representations for su(2)„ and these are also labelled from 0 to n according to the spin of the representation. We have the following decomposition: xrn,=
L xj*2,xr\ o
(5.6a)
xeven
Xr 4
4B)
4 0
0 xodd
= t
X^X?"'. 4 0
(5.6b) 4
0
X ^ " " " = xSr^xS* " + X ^ X ? " .
(5.6c)
X? 4 n + 4 , n ) = X? 4 "^? 4 "' + X? 4n) X? (4m) -
(5.6d)
We shall denote the branching function for sp(/i + m)/sp(n)©sp(m) by B$t), where x, y and z label the representations of sp(n + m), sp(«) and sp(m), respectively. Similarly the branching function for su(2)rtffi su(2))M/su(2))I+m will be denoted by B^z), where x, y and z label the representations of su(2)((1+(B), su(2)(n) and su(2)(m), respectively. Using the basic relation (5.4), we have that
s { <;)„-%'),
(5.7)
where the branching functions are non-zero for JC, y, z in the permissible range and x =y - z mod 2. This is the result obtained by different methods in ref. [18]. We now can see why the coset models associated with this dual pair do not necessarily share the same extended conformal symmetry. The ft scalars for the
559
P. Bowcock, P. Goddard / Conformal algebras
707
TABLE 2
Examples of dual coset pairs
(a) (b) (c) (d) (e)
(0 (g)
(a) (b) (c) (d) (e) (f) (g)
G
Si
A.
so(4(/i + m)) so(W) su(A/) E, E7 E» E,
(C„. m ), soCn)! si^n), (F 4 ), (A 5 ), (E 7 ), (E 6 ).
(Cj,®^), s^m), su(m), (C 3 ), (C 3 ), (E 6 ), (EJl
«2
*2
(A,) m ©(A 1 )„ so( M - m), s u ( W - m), ® u(l) (G 2 ), (G 2 )! (A 2 ), (G 2 ),
(A,) m + „ sa(M-n)i 1< m< n < M su(W - n ) , ® u ( l ) 1 <m
su(2)nffi su(2)m/su(2)(/I + m) theory are highest weight states for the representations of 0K occurring in Bffi-z). The corresponding states in the dual coset theory occur in the branching function B[f:). Such states transform under sp(«)ffisp(m) according to the representation y ® z and so are, in general, not h scalars and so do not act in the dual coset theory. To see this more explicitly, let us consider the case when m = 2. The coset theories su(2)„© su(2)2/su(2)(/I + 2) can all be supersymmetrised. An h scalar 4>(z) for the coset sp(« + 2)/sp(n)ffisp(2) has conformal weight given by x(2n + h<,= QT"+2) + N= - 1 —
6-x) -7T~^+N
for
#e^.
(5-8)
If ^ = 2 t n e n Qx^n*1)= \, \. It is straightforward to show that there is no solution (n,x) to the first possibility and the two solutions (4,6), (8,4) to the second. Using ref. [20] we can see that the 6 representation of sp(6) contains no singlets under sp(4)ffisp(2), so ruling out this possibility. On the other hand, the 4 representation of sp(10) does contain a singlet under sp(8)ffisp(2). Thus only for the coset sp(10)/ sp(8)ffisp(2) is there an h scalar with conformal weight § which is a candidate for a supersymmetry generator G(z). In table 2, we provide a list of other examples of dual coset pairs, together with the algebra G.
560
708
P. Bowcock, P. Goddard / Conformal algebras
6. Comments and conclusions We have shown how, by considering the /t-scalar fields within the representations of gx, we can understand the extensions of conformal symmetry realised within a coset theory, gx/hy, for example when it can be supersynunetrised. We have also explained the complementary role played by the commuting family of fields, v scalars, in understanding the decomposition gx with respect to hv. These ideas have been applied in particular to discussing the structure of the discrete series. §x® ^m/^m+y We showed that the extended conformal algebras, common to the theories in a given series of this form, have fields corresponding to A-scalars in gx. There are many questions which might be addressed within the framework adopted here that we have not yet considered. The representations of extended conformal algebras constructed here are manifestly unitary but we do not know which other unitary representations exist, except in the case of the superconformal algebra. In general, we do not know whether continuum representations exist as well as discrete series or indeed whether the series that appear to be discrete really are so. To decide this, we would need the analogue of the Kac determinant formula and the analysis performed by Friedan, Qiu and Shenker. Other results one might conjec ture, and which it would be of interest to decide, are: (i) thefinite-reducibilityof the coset theory with respect to the extended conformal algebra common to the members of one of the "discrete series" gxffihm/hy+m\ and (ii) the uniqueness of a coset theory gx/hy given the extended conformal algebra of ^-scalar fields. Another subject which might reward study is the generalisation of eq. (3.16) to fields of higher conformal weight and the way such ^-scalar fields close amongst themselves. More basically, one would like to have precise proofs of the existence of g and g/h theories in some suitable sense. We are grateful to Adam Schwimmer for discussions on the structure of confor mal field theory and also to Ruth Gregory for help in preparing the manuscript. We wish to thank the School of Mathematics of the Institute of Advanced Study, Princeton, for hospitality whilst most of this work was being performed. Peter Bowcock would like to thank the Science and Engineering Research Council and Trinity College, Cambridge, for their financial support.
Note added After completing this work we received a preprint [23] which also discusses dual coset pairs, overlapping with our sect. 5, but concludes, in the particular case of superconformal symmetry, that such pairs should share the same conformal algebra. This would not hold from the point of view adopted in this paper where the extended conformal symmetry associated with a coset theory depends on the pair gD/i from which it has been constructed, and commutes with h. In particular, we
561
P. Bowcock, P. Coddard / Con/ormal algebras
709
have shown that the cosets sp(n + 2)1/sp(w) © sp(2), do not have superconformal symmetry, whereas the dual cosets su(2)„ e su(2)2/su(2)n+2 do. References [1] [2] [3] [4) [5] [6] [7] [8] [9] [10] [11] [12] [14] (15] [16] [17] [18] [19] [20] [21] [22] [23]
D. Friedan, Z. Qiu and S. Shenker, Phys. Rev. Lett. 52 (1984) 1575 P. Goddard, A. Kent and D. Olive, Phys. Lett. B152 (1985) 88 J.L. Cardy, Nucl. Phys. B270 [FS16] (1986) 186 A. Cappelli, C. Itzykson and J.-B. Zuber, Nucl. Phys. B280 [FS18] (1987) 445; D. Gepner, Nucl. Phys. B287 (1987) 111 P. Goddard and D. Olive, Int. J. Mod. Phys. Al (1986) 303 H. Sugawara, Phys. Rev. 170 (1966) 1659 E. Witten, Commun. Math. Phys. 92 (1984) 455 P. Bowcock and P. Goddard, Nucl. Phys. B285 [FS19] (1987) 651 P. Goddard, A. Kent and D. Olive, Commun. Math. Phys. 105 (1986) 105 P. Goddard and A. Schwimmer, Phys. Lett. B206 (1988) 62 V.A. Fateev and A.B. Zamolodchikov, Nucl. Phys. B280 (1987) 644 F.A. Bais, P. Bouwknegt, M. Surridge and K. Schartens, Nucl. Phys. B304 (1988) 348; 371 A.B. Zamolodchikov and V. A. Fateev, Sovt. Phys. (JETP) 62 (1986) 215; Sovt. Phys. (JETP) 63 (1986) 913 D. Gepner and Z. Qiu, Nucl. Phys. B285 (1987) 423 V. Dotsenko and V.A. Fateev, Nucl. Phys. B240 (1984) 312; Nucl. Phys. B251 [FS13] (1985) 691 M.R. Douglas, Caltech preprint CALT 68-1453 (1987) V.G. Kac and M. Wakomoto, in Conformal groups and related symmetries: physical results and mathematical background, Lecture notes in physics 261, (Springer, New York) p. 345 P. Goddard, Lecture notes on conformal field theory (unpublished); to appear W.G. McKay and J. Patera, Tables of dimensions, indices and branching rules for representations of simple lie algebras (Dekker) A.N. Schellekens and N.P. Warner, Phys. Rev. D34 (1986) 3092; F.A. Bais and P. Bouwknegt, Nucl. Phys. B279 (1987) 561 M. Jimbo and T. Miwa, Adv. Stud. Pure Math. 6 (1985) 17 D. Altschuler, preprint LBL-TH-25125
562
Reprinted with permission from Physics Letters B Vol. 245, No. 1, pp. 65-71,2 August 1990 © 1990 Hsevier Science Publishers B. V.
W-algebras and coset models G.M.T. Watts Department ofApplied Mathematics and Theoretical Physics. University of Cambridge. Silver Street, Cambridge CBS 9EW, UK Received 17 April 1990
We define a W-algebra as a special class of meromorphic conformal field theory. We then show that there are closed W-algebraic structures in coset models of the form gixgi/gi*' based on the simple Lie algebras A„, B„, D„and Em for sufficiently high values of*.
1. Introduction In studying two-dimensional conformal field the ories [1], it is useful to consider algebras with re spect to which one may decompose the Hilbert space. One such algebra is the Virasoro algebra of which there are always two copies present in a conformal field theory, corresponding to the modes of the fully holomorphic and fully anti-holomorphic compo nents of the stress-energy tensor. The Virasoro alge bra includes the element c which always takes a par ticular constant value in a given field theory. For values 0 < c < 1, the Hilbert space has afinitedecom position into representations of the left- and rightVirasoro algebras when you additionally impose modular in variance of the partition function [2]. This property of finite decomposition makes the study of such field theories much easier and has enabled the complete characterisation of the possible field contents [3J. As a result of these successes, there has been much interest in a study of possible extended algebras which contain the Virasoro algebra as a sub-algebra [4-6], for which there might be a finite decomposition of the Hilbert space for different ranges of c. A wide range of such algebras are generically known as Walgebras [7], and are based on finite simple Lie-al gebras in their construction. These algebras are formed of the modes of purely (anti-) holomorphic fields; the commutator of any two of these modes is an infinite sum of products of modes and is an ele
ment of the closure of the universal enveloping alge bra. This property means that the operator product algebra of thesefieldscloses on normal ordered prod ucts of thefieldsand their derivatives. It has been suggested that such W-algebras may also be found in affine Kac-Moody algebras and coset models based on them [ 5,6 ]. There are many corre spondences indicating that this is the case, and here we prove that such W-algebraic structures may be constructed in coset models [8] of the form 8Sxgi/i* +1 ,
(i)
with g one of the finite Lie-algebras A„, B„, D„ and E„. (This is a generalisation of the results obtained in ref. [6].) In these models there are rank(g) indepen dent fields in the W-algebra with spins one greater than the exponents of g. Certainly this construction is not valid for all k, since it would predict indepen dentfieldsof spins 2, 8, 12, 14, 18, 20, 24 and 30 in the model
e 8 x£j/£|.
(2)
This is the Ising model at c = { and the only indepen dent bosonic field in this model is the stress-energy tensor with spin 2. It is possible to prove, however, that in each of the series of models (1) there is a Walgebra for k sufficiently large. This proof is in three stages. Firstly we define a Walgebra as a meromorphic conformal field theory (MCFT) [9] with suitable restrictions. Secondly we show that if the Hilbert space of a MCFT takes a par65
563
ticular form to a sufficiently high level, then it is the Hilbert space for a W-algebra. Thirdly, to apply this result we show that the coset models in question are MCFTs, and that their Hilbert spaces are spanned by states of the requisite form to a sufficiently high level. The proof does not produce the structure constants of the algebras, and only shows that the algebras exist for values of the parameter A: higher than some (un determined) value.
dered products of the fields W'(z) and their deriva tives. The definition of the normal ordering is not es sential, since any two will differ only by finite local terms, but for convenience we may use the following [ 5 ], which has the advantage that is known to be lo cal by the results of MCFT. The normal ordered product of the two fields
(5)
This vertex operator has models which are expressi ble as an infinite sum of the modes of the fields 0,
2. W-algebras and normal ordering If a conformal field theory is spanned to a suffi ciently high level by states of a particular form, then there is a W-algebra in this field theory. We shall de fine a W-algebra to be a conformal field theory with the following properties. (i) A W-algebra is defined to be a meromorphic conformal field theory (MCFT) [9] and as such has the following properties. A MCFT consists of a Hilbert space Jf and a set of local vertex operators V(u. z) for each of the states in this space. There is a distinguished state, the "conformal state" \Ly, whose vertex operator is the stress-energy tensor of the the ory, and whose modes form a copy of the Virasoro algebra. We define the mode decomposition of a ver tex operator of weight A of a bosonic state, and of a Neveu-Schwarz vertex operator for a fermionic state, as
Lexicographic ordering means that there is a fixed choice for the order in which the creation modes are applied to the vacuum. One ordering is
<»(--)= I 0-„,-jZm-
(3)
"•'l-n,-,
With this, the operator product expansion of two fields 0.0' of weights J. A' may be rigorously defined as the series expansion
m,»Q,
5#'5„= I
I
(6)
rmZ
=
r>-A.
(7)
We shall, however, make use of an equivalent, but more useful requirement. (iii)' Jf is spanned by the states which consist of lexicographically ordered creation modes of the fields W'(z) acting on the vacuum. The fact that L, anni hilates the states | / ) implies that W:„-^.|0>=0,
m>0.
(8)
»":,„„-j.. 10>,
"l€Z
=
f
(z-z'YV(O_,_^_,\0y,z'),
p.-A-A |z|>|z'|.
(4)
(ii) Amongst the states in Jf, there is a finite set of states, {I/>}, including the conformal vector, whose vertex operators are V( |/>, z) = W'(z). We require that these states are eigenstates of L<, of weight A', and that they are annihilated by L,. (iii) The space of fields is spanned by normal or 66
(9)
although the particular choice is immaterial. The condition that the Hilbert space is spanned by states of this form is equivalent to the requirement that the space of fields in the theory is spanned by vertex op erators for lexicographically ordered states. To show that (iii)' is equivalent to (iii), we need to show that the space of states is spanned by states of the form (9). We prove firstly that the states at each level are spanned by states consisting of crea tion modes of the fields W, which are not necessarily in lexicographic order. Suppose that all the states to level n may be ex pressed in terms of lexicographically ordered states.
564
The states in Jf at level n + 1 are created by the action of the fields of weight n+1 on the vacuum. AH the fields may be written in terms of repeated normal or dered products. From (6) we know that the modes of any field may be written in terms of the modes of the fields W. A typical field at level n+ 1 will create a sum of states, each of the form WLm-,,u,
m>0.
(10)
The state u may contain annihilation modes of the basic fields. However, it is at level n or lower, and so it can be re-expressed as a sum of states which only contain creation modes. Thus Jf is spanned by states which contain only creation modes. We may now show inductively that any state of the form (9) which is not necessarily in lexicographic or der may be written as the sum of ordered states. We assign a gradation to the space of states by g(»"-„-*u)=g(u)
+ (A-),
*(|0>) = 0.
(11)
Suppose the space of states with gradation less than or equal to m are spanned by lexicographically or dered states. Consider a non-lexicographically or dered state v, of gradation m+ 1. This state must be of the form v=OWpW',,P\Qy
,
(12)
where W'f and W'q are not in lexicographic order and 0, P consist of creation modes of the W. We have v=6H»,lY'l,P\Oy+0[iVp,
(VJ,]P\0y .
(13)
The commutator [ WP, W',] consists of modes of the fields which appear in the singular part of the opera tor product expansion of the fields W and WK From (4) we can see that the fields in the singular part of the operator product expansion of W and W' have gradation less than A'+A*. Thus the second term in (13) has gradation less than or equal to m, and so can be expressed in terms of lexicographically or dered states. In this way, it can be seen that all the states may be re-ordered lexicographically, and that all such orderings are equivalent. There is a corresponding associative algebra of the modes of the vertex operators W'(z). This algebra closes in -W, the completion of the universal envel oping algebra of the modes with respect to the topol ogy induced by taking matrix elements in Jr\ To con sider the representation theory of a W-algebra, it is
sometimes more useful just to study this algebra than the whole field theory. The algebra contains all the information necessary to reconstruct the field theory, but it does not have as nice a definition, since only certain of the elements of * appear as the modes of vertex operators of states in Jf. (The study of II' has been started in ref. [10].) The field and mode normal ordering as defined above are neither associative nor commutative. However, it is possible to define a commutative field normal ordering [ 11 ] by i$(zW(z)i
= V(»0.^.A
|0>,r),
(14)
where 9 projects onto the space of states which are annihilated by L,. This differs from (5) by finite lo cal fields. However in this case the expression for the modes of this field are not as simple as (6). If the Hilbert space of a MCFT is spanned by states of the form (9) for fields W(z) up to level 2 max (J) - 1 , then the MCFT generated by these fields is a W-algebra. This relies on the fact that the operator product of two fields in a MCFT takes the form (4). For any two fields W'(z), fVJ(z), the singular terms in their operator product expansion are vertex operators for states of weight less than 2max(^f). These states may be written in the form of lexico graphically ordered creation modes acting on the vacuum and so their vertex operators are (repeated) normal ordered products of the fields W(z). Modes of such fields are (infinite) sums of normal ordered modes W'm, and so the commutator of any two modes w 'm< w'» is expressible as an (infinite) sum of modes of the basic fields. If we wish to find the operator product expansion of any two normal ordered fields, we need only evaluate a finite number of states to find the contributions to the singular part, and by as sumption these can all be expressed in terms of lexi cographically ordered modes of the fields W(z) act ing on the vacuum. Thus we can show inductively that all the fields which appear in the operator algebra of the fields Wi(z) can be expressed in terms of normal ordered products of these fields and their derivatives. Addi tionally, the commutator algebra of the modes W'„ closes on convergent infinite sums of such modes. 67
565
Thus the field theory generated by the fields is a W-algebra.
W(z)
3. W-algebras and Kac-Moody algebras at * = 1
W'^..W^,dnx...„, 10>,
To show that the affine Kac-Moody coset models (1) contain W-algebras. it is useful to consider first the A-.00 limit. In this limit W becomes the space of states in the level one g representations with integral or half-integral weight which satisfy the condition •/?1)Ow = 0 .
a -n-1/2lO>=//L,//i,...//'L,^.l/2|0> ,
(16)
L/>=4.*./2-*—1/2I0),
(17)
explicitly satisfy (15). These states are of weight (n+ J) and 2/, 1 $ ; ^ n. respectively. We need to show that the three conditions for a W-algebra are satis 68
ij>iJ+l,
/y = i y + 1 = > m y = S m y + i ,
m,^-2ij,
i!,+ 1 < / i ; ^ -n-
J,
(18)
are linearly independent and span Jfa. The dimension of Jf0 at each level can be explicitly calculated [13,14] and rearranged in the form
(15)
We denote this space by Jf0- It has been shown [11] for g simply-laced, that we can find a set of states {| />} with weights A' related to the exponents of g, such that the states of the form (9) are independent and span Jf0. It is also possible to use a slight modification of this argument to show that 6„ at level one contains a W-algebra with both bosonic and fermionic fields. B„ has three inequivalent. unitary, irreducible represen tations at level one. The three level-one representa tions have as their lowest-lying states the scalar, vec tor and spinor finite-dimensional representations of B„ respectively. Together, the scalar, or vacuum, and vector representations form the Neveu-Schwarz sec tor. JPNS, and the spinor representation forms the Ramond sector, JfR. There is a free field construction of B„ at level one [12] in terms of n free bosons and one free fermion. In y NS the fermion is a NeveuSchwarz fermion and bosonic momenta take values in AR. the root lattice of B„, whereas in jfR the mo menta are in AR + t, where «is a spinor weight of B„, and the fermion is a Ramond fermion. The subspace of the representation space of 6J sat isfying (15) may be constructed entirely in JfNS and contains only states with zero bosonic momentum. Since this sector is a MCFT [9], we know that the vertex operators for all the states may be constructed from the free bosons H'(z), and the free fermion
fied. (i) is true by construction. The states (16), (17) explicitly satisfy (ii), with 11 > proportional to the conformal state. To satisfy (iii)', we need show that the states of form (9) span Jfjj. In fact, the states
Trace JP0 (, 7 ^)= f\ "fj' ( l - ^ ) X f\ I.I
i=\
..i
O-Q-"2)
xnii-^-d-t"2)-1.
(i9)
This may easily be seen to give the number of inde pendent states of the form (18) at each level. So, if we can show that the states (18) are linearly inde pendent, then they span j%>. A general state in the zero momentum sector of Jto may be written «=//£,...//:;,!?„,...!P„, 10>,
wy«-l,
ny+,<(7y<-J.
(20)
Let J?m.„,, be the subspace of Jfo spanned by states of the form (20) with in bosonic creation modes, n fer mionic creation modes and with a total fermionic contribution to the weight of — p, that is Xny= —p. Jr,„^,, contains states at level m+p and above. For states of the form (18), we introduce a gradation g, which essentially counts the maximum number of Hfields appearing in a state [11], g(W„u) = li+g{u)
, g(dmu) =
S(|0>)=0.
n+g(u), (21)
We call *„,, the subspace of states of the form (18) with gradation r, s (/-field creation modes and with a total rf-field contribution to the weight of -t. n;M contains states at levels r+ \s and above. We can con sider the projection maps
#,.,.,
•
(22)
Since the bosons and fermions used in the construc-
566
tion of Jf0 are free, the spaces X,j,.„ are orthogonal. We can introduce an ordering on the triples (r, s, t), so that 0«.,-«*; j -.,-=O, (r,s, t)> (r'.s',
{r\s\t)<(r,s,l),
(23)
G'(x) = C'(F'(x),
f)
if r>r' r=r' ,
s>s'
r=r' , i = i ' , f—ns>l— ns' .
(24)
Suppose we have a relation amongst states in differ ent *,',., at level n, then I
u,,ru,,,=0,
is invertible inside the first Weyl chamber [15]. If we consider two sets of smooth functions J(->J(". (F'(x) F"(x)) and (G'(.x),..., G"(x)), related by
a,-,-,-e *,'•.,-.,•.
(25)
(29)
£:»"l2„-,„-W'-2„-„„|0> ~e" ,l G"(r)...a m 'G"(r) . f:H,Ll.„,...H,L,
Let the first non-zero a be at (r, 5, / ) . Using (16) and the expansion
...,F"(x)),
then this map is invertible for (F) in the first Weyl chamber. We can form two maps, one from ilrs, to the space of polynomials of the G'(x), and their de rivatives, and a similar map from XmjlA to the space of polynomials of the F'(x). and their derivatives, by
(30)
_,„,|0>
H.3""F"(z)...a""/r"(r) .
(31)
The map between these two spaces of polynomials is invertible, and so we can form the commutative diagram, + terms with less//fields ,
(26)
we easily see that the only non-zero component un der the projection map 0 r J .,,„ is that in #,,,. The action of <prj,,-^ on a generic state in *, A , is
(27) where u(H) is independent of s and f and the last two terms in this state are determined by 5 and l alone. In particular, to show that the maps 0 rj ,,_„ are non-de generate on %j,n we only need to consider the space *M).o a n ( l t n e m a P 0r.o.o- This case is amenable to the analysis of Nahm [ 11 ], which we reproduce here for convenience. The tensors multiplying the modes of the fields H' in (26) are a basis for the invariant tensors under the Weyl group of B„. They give the values that the n in dependent Casimir operators C CofB„takeon an irreducible representation, in terms of the highest weight of that representation. The map from &"->3t" given by (A'
A")«(C'(A)
C"(h)),
(28)
*,;,., i ».,, •*.,,-«
f
-
«[G.ac,...] I VlF.dF,...}
(32)
Since this diagram is commutative and the map be tween the spaces of polynomials is invertible, the map from the states of the form (18) to the space of states of the form (20) is non-degenerate, and there is a Walgebra in the model generated by the fields W'(z) and d(z). The case of g simply-laced is identical to the con sideration of the spaces Wr00 and the maps 0,.o.o- In the space •#<, for g simply-laced, there is an explicit set of states, |/>, constructed in an analogous man ner to (17) from rank(g) free fields and tensors in variant under the Weyl group of g. From inspection of the characters, the dimension of each L0 eigenspace of J% is the same as the number of independent states of the form (9). Similarly one can show that these states are linearly independent by constructing maps into polynomials of the coordinates of a map 9l->8", and their derivatives. Thus there is a W-algebra for each simply-laced g in the level one repre sentation space, and Jf0 is spanned by states of the form (9) which are linearly independent.
69
567
4. Coset models are W-algebras Firstly we show that the coset models (1) are MCFTs and secondly that their Hilbert spaces are spanned to sufficiently high a level by the space of states of the form (9). We denote the generators of g' by J°i)m. The space of states for the W-algebra will be those states, u, in ihe tensor product of the vacuum representation of gk with the vacuum (g simply-laced) or NeveuSchwarz (B„) representation of g', which satisfy
(•/?.)„+./(*)«)« = 0, m>0,
(33)
We denote this space by Jr*. This is more restrictive than the usual coset model condition since we wish only to consider the meromorphic part of the coset model. All the states which satisfy (33) have integral weight (half-integral in the case of B„) with respect to the coset Virasoro algebra. These conditions may be seen to define a MCFT with local vertex operators for all the states by con sidering Jf as a restriction of the (k+1 )-fold tensor product of the level one g vacuum representation. We know that the level 1 vacuum representation of g is the Hilbert space for a MCFT since we have an ex plicitly local construction for it in terms of free fields [12]. It has been shown for g one of A„, B„, D„, E„ that we can find a set of states {10} such that the states of the form (9) or (18) are all independent and span
*a. For any state u in jf0 and for k sufficiently large, it is possible to find a state in J(k which is a deformation of » of order \/k [16]. Thus for large enough k, we can find states {|/" >} in Jfi which are O ( I M ) defor mations of {11 >}. We now consider the space of states of the form (9) formed out of the modes of the ver tex operators for these deformed states. Consider A/M the determinant of the inner product matrix of these states at level N. This determinant is a rational func tion in k. Since the k—co limit of the states (9) in Xk are those in jfi, this determinant can not be identi cally zero. The determinant has a finite number of zeros and poles in k, and so for k sufficiently large it must be non-zero. Thus the states of the form (9) in Wk art linearly independent. We know from the branching functions for the model (1), that the space of states in J?k at any par
70
ticular level has the same dimension as that in Jto, for k sufficiently large. Thus for sufficiently high k, the space of states in Jtk is spanned to level 2 max(^) — 1 by states of the form (9), and there is a W-algebra with fields of weight A' in Jfk.
5. Conclusions We have proven the existence of W-algebras in the infinite set of coset models of the form (1) based on A„, B„, D„ and E„, for k larger than some finite num ber. Although an explicit construction of the coset Walgebra fields may be too much to ask for, the range of k for which all the fields W'(z) are present, and the results in the other cases may not be beyond cal culation. It is also of interest whether the algebras constructed here are identical to those in the free field construction [7]. Certainly this is the case for WA,, WA2, WA3 and WB,, WB2, since there the field con tent determines the structure constants after the im position of the associativity of the operator product expansion [ 17 ]. It is possible that all the other alge bras are also determined by their field contents alone, but no proof is known. In a recent paper [ 18 ], a free field construction for A k„ has been used to show that the coset Virasoro algebra has the same form as the free-field case, but the other fields have not yet been considered in this manner. Finally, there is the pos sibility of the other non-simply-laced algebras, but the state counting arguments used here will have to be improved to cope with the parafermionic fields pres ent in J*o, and those used in the free-field construc tions of the level one algebras [12,19].
Acknowledgement I would like to thank the SERC for a research stu dentship, and I would like to thank W. Nahm for ex plaining his proof of the independence of states at level one for the bosonic theories, and P. Bowcock, P. Goddard, H. Kausch and A. Kent for useful discus sions concerning this work.
568
References [1]A.A. Belavin, A.M. Polyakov and A.B. Zamolodchikov. Nucl.Phys.B241 ( 1 9 8 4 ) 3 3 3 . [2]J.Cardy,Nucl. Phys. B 2 7 0 [ F S 1 6 ) (1986) 186. | 3 ) A . Capelli, C. Itzykson and J-B. Zuber, Commun. Math. Phys. 1 1 3 ( 1 9 8 7 ) I. (4) V.A. Fateev and A.M. Zamolodchikov, Nucl. Phys. B 289 (FS18] ( 1 9 8 7 ) 6 4 4 ; A.B. Zamolodchikov, Teor. Mat. Fiz. 65 (1985) 347; FA. Bais, P. Bouwknegt, K. Schoutens and M. Surridge. Nucl. Phys. B 304 (1988) 348; V.A. Fateev and S.L. Luk'yanov, Intern. J. Mod. Phys. A 3 (1988)507. (5] FA. Bais. P. Bouwknegt, K. Schoutens and M. Surridge. Nucl. Phys. B 304 (1988) 371. [6J P. Bowcock and P. Goddard, Nucl. Phys. B 305 [FS23] (1988)685. [ 7 ] V.A. Fateev and S.L. Luk'yanov, Additional symmetries and exactly-soluble models in two-dimensional conformal field theory, Moscow preprint (1988).
18 ] P. Goddard, A. Kent and D. Olive, Phys Lett. B 152 (1985) 88. [9] P. Goddard, DAMTP preprint 89-1. 110] A. Kent, Normal ordered Lie algebras, Princeton preprint IASSNS-HEP-88/4. [ 11 ] W. Nahm, private communication. [12] P. Goddard, W. Nahm, D. Olive and A. Schwimmer. Commun. Math. Phys. 107 (1986) 179. [ 13) G.M.T. Watts, Nucl. Phys. B, 339 (1990) 177. [ 14] V. Kac, Infinite dimensional Lie algebras (Cambridge U.P.. Cambridge, 1985). (15] A.O. Barut and R. Raczka, Theory of group representations and applications (World Scientific, Singapore, 1986) p. 263. [ 16] P. Goddard and A. Schwimmer, Phys. Lett. B 206 (1988) 62. [17] H.G. Kausch and G.M.T Watts, unpublished results [18] M. Kuwahara and H. Suzuki, Coset conformal models of W-algebra and their Feigin-Fuchs construction, preprint OSGE 02-89 (1989). [ 19] G.M.T. Watts, in preparation.
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Reprinted with permission from Physics Letters B Vol. 228, No. 1, pp. 57-63,7 September 1989 © 1989 Hsevier Science Publishers B. V. (North-Holland Physics Publishing Division)
THE LARGE-/V LIMIT OF EXTENDED CONFORMAL SYMMETRIES I. BAKAS ' Center for Theoretical Physics. Department of Physics and Astronomy. University of Maryland. College Park. MD 20742. USA Received 27 April 1989; revised manuscript received 14 June 1989
We study the large-A/ limit of the operator algebra W.v generated by primary conformal fields with integer spin 1, 2 S. It is shown that W x provides a representation of a certain infinite dimensional (sub )algebra of the area-preserving diffeomorphisms of the 2-plane (compactified or not). We also discuss certain applications of this result to quantum field theory.
The classification of two-dimensional conformal field theories has received considerable attention in connection with the quantum theory of strings and the critical behavior of various statistical mechanics models [ 1 ]. Recently, it was realized that a large class of conformal theories can be described in group the oretical terms as minimal models of the Virasoro and other chiral operator algebras [2]. In particular one considers extended conformal symmetry algebras W with commutation relations of the form [«„(«), ul:{m)] = X I C-'^'in, m; k
*„)
;<: :*! xu„(k,)...ujkp),
(1)
and then studies their unitary representations. The holomorphic fields {u,(z)} with Fourier modes ut(n) are chosen so that W forms a closed operator algebra (in the sense that the Jacobi identity is satisfied) and the Virasoro algebra [L„,L,„] = (n-m)L„+,„ + -hc{ni-n)6„mX>
(2)
is contained as a subalgebra in W. The identity oper ator / is also included among the generators of W and the conservation of momentum condition « + m = k,+... + kp is implicit in eq. (1). In this setting ra tional conformal field theories correspond to unitary representations of W with a finite number of confor mal (building) blocks for certain series of discrete values of the central charge c, depending on the op erator algebra W.
A detailed analysis of the problem has led to the conjecture that extended conformal symmetries can be essentially catalogued using the Cartan classifica tion of simple Lie algebras, the Virasoro algebra being the most elementary member of the conformal fam ily associated with the Lie algebra A,. This conclu sion has been reached from many different points of view that involve the quantization of three-dimen sional Chern-Simons topological field theories [3], the study of Toda field theories [4], the algebraic structures of integrable non-linear differential equa tions of the KdV type [ 5 ] and the generalization of the Goddard-Kent-Olive construction to arbitrary coset models [6]. One particular way to obtain extended conformal algebras from Kac-Moody Lie algebras is provided by the method of hamiltonian reduction employed by Drinfeld and Sokolov in their systematic description of hierarchies of integrable non-linear differential equations [7]. We consider the space of first order differential operators D,=3+/l+«(r), where /0 l
A-\
\ 1
(3)
0
... 0\
°
.
°'
:.
(4)
l' 0/
Supported in pan by the NSF grant PHY-87-17155.
57
572
/«ll
012
01* \
022
«=
(4 cont'd)
0
\
to/
i.e. A is a constant matrix and q takes values in the upper triangular matrices of the general linear alge bra gl(A0. Then it is always possible to find a gauge transformation S(z) generated by the subalgebra of gl(AT) with values in the strictly upper triangular ma trices so that S-'(z)D,5(r)
/0 ... 0
-Mr)
= 8+/l + j ; \0
(5) ... 0
-u,(z)
It turns out that the coordinate fields {u,(z),j= 1,2, ..., N) which parametrize the space of gauge equiva lence classes of the differentia] operators (3), have conformal weights 1,2 N respectively and gener ate the spin N operator algebra W* [ 8 ]. Other oper ator algebras of two-dimensional conformal field the ory can also be described in this fashion, by imposing appropriate conditions on the matrix elements of In what follows we consider only the conformal al gebra W„ and we note that the spin 2 field u2(z) (or more precisely u2(z) — j (N-1 )u\ (z)) can be iden tified with the stress-energy tensor T(z) of a two-di mensional field theory, while the spin 1 field ut(z) corresponds to an additional U ( l ) conserved cur rent that might be present in the model. The traceless condition Tr<j(z)=0 amounts to setting u,(z)=0, thus producing Zamolodchikov's spin N operator al gebra associated with the simple Lie algebra A* [2]. For N> 2 the commutation relations of W* have quadratic determining relations (cf. eq. (1)). Note that although the method of hamihonian reduction ( 3 ) - (5) provides a systematic way to formulate the commutation relations of extended conformal alge bras, the potentials q(z) are classical functions. To obtain the chiral operator algebra associated with conserved higher spin fields on the world sheet, one has to assign operators to q(z) and all the coordinate fields u,(z),7=1, 2,..., A' as well as normal order the quadratic terms that appear in the determining rela tions of the algebra [ 8 ]. However, the basic structure
58
of W„ remains the same upon quantization, as was explained in refs. [2,5]. For our purposes (and since we also normalize n = 1), it would be sufficient to use the commutation relations of W* when dealing with the chiral operator algebra of extended conformal symmetries. Motivated by the behavior of SU(N) gauge theo ries at the large-N limit (see for instance ref. [ 9 ] and references therein), we propose to study the infinite spin algebra W„. Certainly this limit arises very nat urally in higher spin theories, since one way to obtain consistent self-interacting gauge theories of massless higher spin fields is through the inclusion of an infi nite family of particles with all possible spins [10]. We shall demonstrate that as N->oo, higher spin op erator algebras of two-dimensional conformal field theory give rise to representations of certain infinite dimensional (sub)algebras of the are preserving diffeomorpbisms of 2-surfaces (e.g. ft2, S2) with nontrivial cocycles. This result might help to provide a suitable framework for studying non-perturbative as pects of string theory in the future. Let us introduce the algebra of area preserving diffeomorphisms of the 2-plane, i.e. the infinite-dimen sional algebra of canonical transformations on RJ generated by all hamihonian vector fields, HVF(R2). We' consider a pair of canonical coordinates x, y in R2 and define the Poisson bracket
among all classical functions on the plane with basis elements fm.„=xm+'y"
n, meZ.
(7)
The hamihonian vector field corresponding to/„.„ is j f . , = * r | ( « i + i ) ^ - ( » + i ) ' ■&■ fJ.
<8)
and so [Xm.m Xm „ ] is given by X.Jm,Jm ,.. Notice that/ m o form a basis for the Virasoro algebra (2) since l/;.o,/,,o} = (n-m)/, + ,„.o.
(9)
Here the central charge c=0. Sometimes it might be helpful to complexify the algebra (6) and introduce (complex) canonical coordinates z, I.
573
Having this in mind we may consider the action of the algebra (9) on the space of all HVF(R2) defined by A.o'/.,V=l/"i.oX.„}-
(10)
Clearly eq. (10) provides a centerless representation of the Virasoro algebra. It is very useful to study the decomposition of HVF(R2) under this action, in terms of primary conformal field modules of two-di mensional field theory. Wefindthat A.o-L..» = l(k+l)(n+l)-{m+l)\ft.„JI,
(11)
which implies that/„„ are basis elements (labelled by m) of a primary conformal field with weight A= - (n+1). Recall that in the holomorphic repre sentation Lk= - z * + l d/dz, the components z'"*'dzJ of a primary conformal field transform according to the rule Lk(z-+'dzJ)
= -[(m+l)+A(k+l)]zm+k
+ ,dzJ. (12)
Consequently the space of all hamiltonian vector fields on the plane, viewed as a module of the Vira soro algebra, decomposes into a direct sum of pri mary conformal field modules F (J) , i.e. HVF(R2) =r ©j./F ( J |. Results of this form have been used in the mathematics literature to study homologies of arbitrary (fixed) dimension with trivial and certain other coefficients of the Lie algebra of (poly nomial) hamiltonian vector fields on R2 [11]. We also note that HVF(R2) = HVF<.(R2)©HVP4.(R2),
(13)
2
where HVF+(R ) is spanned by /„.„ with n~z - I and the asterisk denotes the (smooth) duality operation; (13) can be easily verified using the in-out duality of primary conformal fields of weight A and 1 —A in troduced by Belavin, Polyakov and Zamolodchikov [1]. Next we focus our attention on polynomial functions (at least in the y variable) and consider the subalgebra HVF+fR2) only. Possible extensions of our results to the full algebra HVF(R2) will be dis cussed later. Using the Poisson bracket (6) we find
fields with weights A = — (n+ 1), A' = — (n' + 1) is a primary field of weight A=-(n
+ n+\)=A+A'
+ \.
(15)
We are interested in representations of HVF+ (R2) which realize the infinite spin algebra (14). The sim plest one to look for is the representation in terms of (linear) differential operators defined on the space of wave functions (i/(x) such that x acts by multipli cation and y by differentiation - 8 ' « - d / d x Then the operators /„ „ associated with the basis elements (7) will be described by the (n+1 )-th order differ ential operators ( - )"* *xm* '3"*' mod 3", where the mod d" terms depend on the particular factor order ing we consider. The main motivation for being in terested in this representation is to provide a reali zation of the algebra HVF* (R2) which generalizes the (standard) holomorphic representation of the cen terless Virasoro algebra L/c=-zk* 'd/dz (though here z~x). It is the decomposition HVF,.(R2) = ©
if,.,,J„, „ } = [ ( m + ! ) ( « ' + l ) - ( m ' + l ) ( « + l ) ] x/, 1 + ,„-..»»
(14)
which means that the commutator of two conformal
*' For convenience we absorb the factor — i/fi in the definition of the Dirac commutator.
59
574
where ! = ( . ' i ) *nd s= (x,y) has been designed to suit our purposes when we order the operators/cor responding iof=f(x)y"+' a la Weyl:
'-<->~£?("r)^*-'- <»» Here the deformation parameter (~ft) has been nor malized to I. We point out that other factor ordering prescriptions give rise to different q-brackets, all sharing the property that the operator corresponding to {/„.„,/„ .„}, is represented by [/„„,/„.„ ] consis tently (see for instance ref. [14] and references therein). In all cases we find that the commutation relations of the (centerless) Virasoro and U ( l ) Kat-Moody algebras which are generated by/„ 0 and/„._, respec tively, remain unchanged. However for/„.„ with n& 1 the transformation law (11) acquires correction terms from the higher derivatives of the q-bracket (16) (or its generalization to other factor ordering prescriptions). In fact /„.„ represents the compo nents of primary conformal fields only modulo d" terms. It is relatively easy to verify that there is no consistent truncation of the (n+1 )-th order differ ential operators /„.„ which preserves the transfor mation (11), and so/„.„ will not represent confor mal fields with definite weight, if n > l . For completeness we mention that although truncations of the sum ( - ) " * xx"'* 'e" + l +0(3") terms >-/„,.„ might result to non-unitary representations of the al gebra of hamiltonian vector fields defined on the space of wave functions iy(x), this is perfectly ac ceptable in view of the problem we have in mind; clearly the (standard) representation Lk= - x ^ ' S o f the Virasoro (sub )algebra (9) is not described by selfadjoint operators on this space. It is important to re alize that by considering the algebra of area-preserv ing diffeomorphisms of the plane we are not neces sarily interested in the quantization of mechanical systems with one physical degree of freedom. In this paper we view the infinite-dimensional algebra 60
HVF+(R2) as the local symmetry algebra of field theories whose quantum properties could be de scribed in group theoretical terms by the representa tions ofHVF + (R 2 ). Before we proceed further a remark is in order. So far we have been dealing with the algebra of canoni cal transformations on the plane (14) generated by the basis elements/,, „=x m + ' y * ' , where x, y are ca nonical coordinates defined globally on R2. Instead if we consider the algebra of area-preserving diffeo morphisms of the sphere S2. we realize that the pair (x, y) is well-defined only locally and so the classical functions on S2 have to be expanded with respect to a global basis that involves spherical harmonics Y„At, 9). However the algebra of HVF(X) is (for mally) the same and insensitive to the topology of the 2-surface £ being R2 or S2. The only place where the topology makes a difference is at the group level, since not all (local) hamiltonian vector fields on S2 admit a global extension compatible with the symplectic structure. To put it differently, there is a topological obstruction to the exponentiation of all local HVF(S2) given by the second De Rham cohomology group H2(S2, R). Because our work is confined at the infinitesimal (Lie algebra) level, we intend to treat locally the canonical transformations on the plane (compactified or not) on the same footing. In the attempt to construct a suitable generaliza tion of the (standard) bolomorphicrepresentationof the Virasoro algebra (9) for the algebra (14), we en countered certain obstructions which were described effectively by the q-bracket (16) (or its generaliza tions). In more abstract terms this means that cohomologies of HVF + (R 2 ) with non-trivial coeffi cients become relevant in the representation theory of the commutation relations (14) and so we have to get accustomed to the idea of using alternative brack ets when considering field theories invariant under the algebra of area-preserving diffeomorphisms of 2surfaces. Moreover, the quantization of these theo ries (like any other field theory) requires knowledge of unitaryrepresentationsof the underlying symme try algebra, analogous to the Verma module repre sentations of two-dimensional conformal field theo ries [ 1 ]. In turn this might cause further deformation of the q-brackets we introduced earlier due to quan tum mechanical corrections of field theoretic nature: (compare eq. (9) and its q-analogue with eq. (2)).
575
For all other commutators, Schwinger terms of this type will not necessarily be (pure) c-numbers, but rather more general Lie algebra cocycles with coeffi cients in the space of local functionals of the fields F,„. We propose to use the infinite spin algebra W„ and its unitary representations for studying quantum properties of field theories which are invariant (clas sically) under the area preserving diffeomorphisms of 2-surfaces. The main driving force behind this sug gestion is the desire to take full advantage of the pri mary conformal field decomposition of the algebra HVF* (R2). Indeed the commutation relations (14) describe a higher spin operator algebra which con tains the (centerless) Virasoro algebra as subalgebra. For instance, if we define tvj (n) >-/,., we obtain {wi(n),wi(m))=(n-m)2f^„l,
(18)
which is very similar to the spin-3-spin-3 commuta tion relations of the extended conformal algebra W.v : fkA are the Fourier modes associated with spin 3 fields and fkl with spin 4 fields *2. It is quite in structive to compare (18) with the corresponding commutation relations of Zamolodchikov's W, alge bra. They are of the form [ 2 ] [w,(n), w-i(m)] = (n-m)2wl(n
+ m)
+ 755C«(n ! - 1 )(n 2 -4)<S„«.,„ 0
+ (n-m)[-h(n+m
+ 2){n + m + 3)
- i ( n + 2)(m + 2)]Z.„+„„
(19)
where w4(z) is a (composite) spin 4 field ~:7"2(z):, the regularized square of the stress-energy tensor. To avoid confusion we note that the leading term in eq. (19) is a purely composite field only when N=2. For N^A there is a primary conformal field with spin 4 among the generators of the W* algebra, whose Fourier modes can be taken to represent/, 2In fact the spin-3-spin-3 commutator of W /v>4 is of the form (18) plus other terms associated with local functions of T (e.g. T1 and derivatives of T) as well as cocycles, analogous to eq. (19) [2,5]. Including all other spin fields we find that the (maximally) ex tended infinite spin operator algebra W^ provides a * : Recall that fields of weight A and I - A are dual to each other. i.e. quadratic differentials are dual to vector fields, etc.
representation of HVF+ (R2). This statement is to be understood in the following sense: for large N, the commutation relations between any two generators of W.v with spin s and s', differ from the correspond ing relations (14) of the algebra HVF + (R 2 ) only by local functionals of conformal fields with spin less than 5+5' - 2. Since both infinite-dimensional alge bras satisfy the Jacobi identity, it is natural to think of W^ as an extension (in mathematical terms) of the classical Poisson algebra HVF<. (R2). However, it is crucial to realize that cohomologies of the algebra HVF+ (R2) with non-trivial coefficients (in general) become relevant in this representation and account for the central (cocycle) terms ~ <5„+,„ 0 as well as the contributions of lower spin fields (and their deriva tives) in the commutation relations of W„. The representation of area-preserving diffeo morphisms of 2-surfaces (e.g. R2, S2) we obtain this way, has the advantage of maintaining the primary character of the generating conformal fields, i.e. [Ln,wk(m) ]=[(k-
l)n-m]w„(n
+ m),
(20)
as opposed to the "holomorphic" representation we considered earlier. Here wk(m) represents the basis elementX,<.j_2.*_2 for all different spins k. More over, it makes it possible to use two-dimensional conformal field theory techniques for studying field theories invariant under HVF + ( I ) , with I=;R2 or S2. In particular highest weight (Verma) module rep resentations of W* for large N, could provide infor mation about the quantization of membrane (or other) reparametrization invariant theories whose evolution preserves (locally) the area element of I. We point out that the unitaryrepresentationsof ex tended conformal symmetries can be constructed ex plicitly. It is known that fundamental weights of sim ple Lie algebras determine the roots of their (generalized) Kac determinants [2]. In the present approach the "master" symmetry is the affine Kac-Moody algebra of GL(N) (and its subalgebrasSL(iV), etc.), since the spin operator al gebras W* are obtained from it by applying the method of hamiltonian reduction [ 8 ]. At the large-/V limit, the GL(oo) Kac-Moody algebra seems to be come relevant for the quantum theory of (possibly higher dimensional) HVF*(R2)-invariant models. Incidentally we note that the loop group of GL(fc), QGL(&). can be embedded in GL(oo) for all values 61
576
of k (see for instance [IS]). Then two-dimensional non-linear o-models with values in the infinite di mensional space flG, where G is an appropriately chosen subgroup of GL(fc), could be used effectively to describe properties of higher dimensional field theories. Recent results of Atiyah in instanton phys ics justify such expectations in principle (16]. How ever, as far as various membrane models are con cerned, further work is required showing whether indeed quantum field theory selects W^ to be the rel evant quantum symmetry algebra. It might be inter esting to construct W*-string theories, where W* is assumed to be the basic symmetry on the world sheet [17], and study their quantization for large N. Per haps the behavior of W^-strings can be formulated in membrane theoretical terms in analogy with the description of SU(oo) gauge theories in terms of conventional string models. We point out that there are two distinct ways to approach the A'—oo limit of GL(/V) by considering either semi-infinite (in both rows and columns) or purely oo x oo matrices. In the first case, denoted by GL (oo)+, the method of hamiltonian reduction (and its quantum counterpart) give rise to the representa tion of HVF + (R 2 ) we considered above. We expect that generalization of our techniques to the full GL(oo) will yield the entire algebra of area-preserv ing diffeomorphisms. However, it is not quite clear at the moment how the gauge fixing procedure (4), (S) has to be modified in this case or what is the meaning of it in the context of conformal field theories. In this framework it is also interesting to study minimal models of extended conformal algebras at the large-N limit. In particular we may consider conformally invariant solutions of two-dimensional quantum field theory possessing a global ZN symme try, e.g. ZA Ising models at their critical point. They are associated with unitary representations of Zamolodchikov's spin N operator algebra with central charge [2]
c= 2 y.
(2.)
At the limit N-*oo the resulting theory has an infinite number of conformal (building) blocks and c=2. It is conceivable that conformal field theories with Z . symmetry have an alternative description in terms of
62
the symmetry algebra of area-preserving diffeo morphisms of 2-surfaces. More generally we think that a better understanding of the large-^ limit of confor mal symmetries will provide us with some non-perturbative information about string theory. These problems are under investigation and results will be reported elsewhere. Finally we mention that other authors have used membranes to describe a new type of gauge principle for SU(oo) Yang-Mills theories and higher spin (Fradkin-Vasil'ev) algebras in (2+1) dimensions [18]. Since our work is based on techniques of twodimensional conformal field theory, the results we have obtained are quite different. Moreover, the present framework could be used for developing a conformal field theory approach to the quantization of certain membrane theories which is different (in nature) from that of ref. [19]. Further details will be presented in ref. [20]. Note added. Recently it was shown that for Ar-»oo the Poisson bracket computation of W* yields the same result as the complete quantum computation of the commutators [21]. References [ 11 A.A. BeUvin, A.M. Polyakov ind A.B. Zamolodchikov, Nucl. Phys. B 241 (1984)333. | 2 ) D . Friedan, Z. Qiu ind S. Shenker, Phys. Rev. Lett. 52 (1984)1575; A.B. Zamolodchikov and V.A. Fateev, Nucl. Phys. B 280 (1987)644; V.A. Fateev and S.L. Lykyanov, Intern. J. Mod. Phys. A 3 (1988)507; D. Kastor, E. Martinet and Z. Qiu. Phys. Lett. B 200 (1988) 434; J. Batter, D. Nemochansky and S. Yankidowicz, Phys. Rev. Lett. 60 (1988) 389; G. Moore and N. Seiberg, Phys. Lett. B 212 (1988) 451. (31E. Wittcn, Princeton preprint (1988); C. Moore and N. Scibert. Princeton preprint (1989). [4] A. Bilal and J.-L. Gervais, Phys. Lett. B 206 (1988) 412. [5)1. Bakaa, Phys. Lett. B 213 (1988) 313; Texas preprint, to appear in Commun. Math. Phys.; P. Mathieu, Phys. Lett. B 208 (1988) 101; K. Yamatishi. Phys. Lett. B 205 (1988) 466. 16) P. Goddard, A. Kent and D. Olive, Phys. Lett B 152 (1985) 88; F.A. Bais, P. Bouwknegl, M. Surridfe and K. Schoutens, Nucl. Phys. B 304 (1988) 348, 371; M.R. Douglas, Caltech preprint (1987).
577
17] V.G. Drinfeldand V.V. Sokolov. J. Sov. Math. 30 (1985) 1975. [8 ] 1. Baku. Phys. Leu. B 219 (1989) 283: M Bershadsky and H. Oogun, Princeton preprint (1989). [9]A.A.Migdal. Phys. Rep. 102(1983) 199. [10) M A Vasil'ev and E.S. Fradkin, Ann. Phys. 177 (1987) 63; FA. Berends. G.J.H. Burgers and H. Van Dam. Nucl. Phys. B 260 (1985) 295. (111 D B. Fuks. Funct. Anal Appl. 19 (1985) 305 (12] R. Abraham and J.E. Marsden, Foundations of mechanics, 2nd Ed. (Benjamin/Cummings. MenloPark. 1978). [ 13] J. Moyal, Proc. Camb. Phil. Soc. 45 (1949) 99. (14] G. Agarwal and E. Wolf, Phys. Rev. D 2 (1970) 2187 [15] V.G. Kac and A.K. Raina. Highest weight representations of infinite dimensional Lie algebras (World Scientific, Singapore. 1987).
[ 161 M. Atiyah. Commun. Math. Phys. 93 (1984) 437. 1171 A. Bilal and J.-L. Gervais, LPTENS preprint (1988). [18]J.Hoppe, Phys. Lett. B 215 (1988) 706; E. Floratos, J. Uiopoulos and G. Tiktopoulos. Phys. Lett. B 217(1989)285; D.B. Fairlie and C.K. Zachos. Argonne preprint (1989); E. Bergshoeff. M P. Blencowe and K.S. Stelle, Imperial preprint (1988). [19)1. Antoniadis. P. Ditsas, E. Floratos and J. Uiopoulos, Nucl. Phys. B 300 (1988) 549; E. Floratos and J. Uiopoulos, Phys. Lett. B 201(1988)237. (20] I. Bakas, in preparation. [21 ] A. Bilal. CERN preprint (1989).
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Reprinted with permission from Nuclear Physics B Vol. 339, pp. 191-221,1990 © 1990 Hsevier Science Publishers B. V. (North-Holland)
W„ AND THE RACAH-WIGNER ALGEBRA C.N. POPE and X. SHEN Center for Theoretical Physics, Texas A&M University, College Station, TX 77843-4242, USA L.J. ROMANS* Department of Physics, University of Southern California, Los Angeles, CA 90089-0484, USA Received 16 January 1990
We examine the structure of a recently constructed W„ algebra, an extension of the Virasoro algebra that describes an infinite number of fields with all conformal spins 2,3,..., with central terms for all spins. By examining its underlying SLX2, R) structure, we are able to exhibit its relation to the algebras of SL(2, R) tensor operators. Based upon this relationship, we generalise W^ to a one-parameter family of inequivalent Lie algebras WJ/x), which for general fi requires the introduction of formally negative spins. Furthermore, we display a realisation of the Wj(/i) commutation relations in terms of an underlying associative product, which we denote with a lone star. This product structure shares many formal features with the Racah-Wigner algebra in angular-momentum theory. We also discuss the relation between W„ and the symplectic algebra on a cone, which can be viewed as a co-adjoint orbit of SL(2, R).
1. Introduction The WN algebras are extensions of the Virasoro algebra containing fields of conformal spin 2,3,...,N (see e.g. refs. [1-4] and references within). These are not Lie algebras for any finite TV > 2, owing to the presence of non-linear terms in the commutation relations, which rapidly increase in complexity as N increases. However, it has been argued that the structure of these algebras should become much simpler in the limit N -* oo [5]. The process of taking the N -» oo limit is not uniquely defined; one can in principle arrive at different algebras depending upon how one first rescales the generators and structure constants of the finite-TV algebra. One particular limit that has been discussed recently [6] takes the form K'W]
= ((; -1)»« - (<• - I)«)H£':'„- 2 \
(i.i)
where wf£ is a generator of conformal spin i. This algebra, which we shall refer to ♦Supported in part by the U.S. Department of Energy, under grant DE-FG03-84ER40168.
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as y/a, can be represented by the Poisson bracket of functions on a two-dimensional phase space, with wj? = qm+'~1p'~l. Although the Ww algebras have central terms for each conformal spin, the limit (1.1) admits a central term only in the Virasoro (i = 2) sector. One might suppose, therefore, that there should exist some different limiting procedure in which all the central terms of the Ww algebra are retained in the N-KX> limit. From a physical point of view such a limit would probably be of greater interest, since it would presumably allow the existence of unitary represen tations with non-trivial dependence on the higher-spin generators. In a recent paper [7], we examined the construction of such an algebra, which we refer to as W,,,, that can be viewed as a deformation of the w,,, algebra (1.1). Our starting point was to demand that the algebra admit central terms for all conformal spins, and then derive the form of the structure constants by imposing the Jacobi identities. The form of the resulting algebra is unique, up to an arbitrary constant c which sets the scale of the central terms. The algebra w„, can be easily obtained as a particular contraction of our W„ algebra, in which most of the structure constants are sent to zero, as well as all of the central terms for spins higher than two. It is consistent for W,,, and its contraction w„ to both be obtainable as two different N -* <x> limits of WN, since the algebra contraction can be implemented in the limiting procedure. The purpose of the present paper is to elucidate the group-theoretic structure that underlies the W,. algebra. In the following section, we begin by presenting the complete expressions for the structure constants, including central terms, essen tially as we have given them in ref. [7]. We then observe that the structure constants of the W„ algebra may be neatly expressed as products of Clebsch-Gordan coefficients and Saalschutzian 4 F 3 generalised hypergeometric functions. The latter may in fact be formally written in terms of Wigner 6-j symbols. These results suggest that one might seek an interpretation of the W^, algebra within the context of SU(2) angular-momentum theory (or, more precisely, algebras of SL(2, R) tensor operators). In subsect. 2.2 we give the operator-product expansion for W«, corresponding to our structure constants. The W„ algebra contains an anomaly-free subalgebra, comprising subsets of generators of conformal spins 2,3,4,... in the 3,5,7,... representations of SLX2, R). The adjoint 3 representation at the base of this "wedge" of generators corresponds to the usual anomaly-free S1X2, R) subalgebra of the Virasoro algebra. In sect. 3, we study the algebras ^(fi) of SL(2, R) tensor operators, which are parametrised by the value fi of the SL(2,R) Casimir operator, and show how to realise the wedge subalgebra WA as the special case fi = 0 of these algebras. Furthermore, we display explicit expressions for the structure constants of J7"(/x) for general /x. The algebras y~(/x) have been considered before in the mathematics and physics literature, though to our knowledge the structure constants have been previously given in closed form only for the special value /x = - -jj (the so-called "symplecton," corresponding to the higher-spin theory of Fradkin and Vasiliev [8D.
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The full W,,, algebra corresponds to an extension of WA outside the wedge, where for each conformal spin the finite-dimensional SL(2, R) representation is extended to the infinite set of Fourier modes of a two-dimensional conformal field. We show in subsect. 33 how to extend the general SL(2,R) tensor algebra ^"(/i.) outside the wedge. For generic values of fi, the resulting Lie algebra Wjt/t) requires the introduction of an infinite set of extra generators with formally negative spin. Motivated by the existence of a standard multiplication law for SL(2, R) tensor operators, we show in sect. 4 how to extend this multiplication consistently outside the wedge (for general /i) to obtain an associative product law defined on Wjt/i). This product, which we denote with a lone star * , appears to be of a type rather unfamiliar in the context of conformal field theory, though it bears some formal resemblance to the so-called Racah-Wigner algebra in the theory of angular momentum (as discussed in refs. [9,10]). As an example, the product of two Virasoro modes (in the case fi = 0) takes the form Lm*Ln-Wm+H
+ \{m-n)Lm+Ht
(1.2)
where the Wm +n are modes of a spin-3 field and the antisymmetric component of eq. (1.2) reproduces the (c = 0) Virasoro algebra. In sect. 5, we discuss a geometrical interpretation of the algebra in terms of the co-adjoint orbits of SL(2, R). In particular, from the form of the wedge subalgebra WA, we find that the relevant orbit is that of the cone. We present some concluding remarks in sect. 6. Finally, in an appendix we summarize our notational conventions and collect several useful mathematical results involving generalised hypergeometric functions.
2. The structure of W^ In our previous paper, we presented a complete set of structure constants for an algebra of generators V^, corresponding to the mth Fourier mode of a field of conformal spin (i + 2); thus m ranges over all integers and i = 0,1,2,..., with the usual Virasoro generators given by Lm = V%. Our starting point was an ansatz of the general form
+ ...WY2is(m,n)V^-^
+ q2ici(m)Si'Sm+ni0.
(2.1)
In ref. [7] we took the polynomials appearing within the central terms to be simple monomials; that is, of the form c^m) = cim2i+3. It is more useful, however, to take
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C.N. Pope etal / Racah-Wigneralgebra
the central terms to have the canonical form determined by c,(m) = {m-i-
l ) ( m - i ) . . . ( m + j)(m + i' + l)cl-;
(2.2)
the difference between these two alternatives is "trivial" in the sense that it may be absorbed into a linear redefinition of the generators. (This fact is well known for the Virasoro sector: the linear component of the anomaly term may be altered at will by simply shifting L 0 by a constant.) Taking into account the modified definition (2.2) for the central terms, the structure constants of ref. [7] become
with .,
' * A-O
(2/-3)(2/+l)(2r-2/ + 3)(r-/+l)
/-1 l(2i ~ 2l + 3 ) ( 2 / "
2/
+ 3 H 2 ' + 2/ - 4r + 2/ + 3) '
(
}
2r+l
^('",«) = 2LL 1 ( - i ) * ( 2 7 1 ) k=0
(2i -2r+l+k) !(2; + 2 - k)!(i + 1 + m)!(; + 1 + n)! (2i - 2r + 1) !(2; - 2r + 1) !(i - 2r + m + it)!(;' + 1+ n - k)! 2r+l
E X (2i + 2 - 2r)»[2j + 2 - *] 2 r + 1 _J« + 1 + m] 2 r + 1 _ J ; + 1 + n]*, (2.5) where the Pochhammer symbols (a)„ and [o]„ are defined in eq. (A.la,b) of appendix A, and as usual a product over an empty range of indices is taken to be unity. The coefficients appearing in the central terms are determined to be
C,=
2 2, ' _3 /!(i + 2)! (2i+l)!!(2i + 3)!! C '
(2 6)
'
where c is an arbitrary overall constant. In the Virasoro sector, eq. (2.6) becomes c0 = c/12, which identifies c as the usual central charge.
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C.N. Pope et al. / Racah-Wigner algebra
195
If the deformation parameter q in eq. (2.1) is set to zero the algebra reduces to eq. (1.1), with w^ +2) identified as V^. The expressions N£(m,n) (and hence the g'jr(m, n) themselves) are in general polynomials in m and n of degree (2r + 1). The integer s appearing in eq. (2.1) is equal to the integer part of (i +/)/2, so in general the commutator of a V generator with a V' generator gives a sequence of generators of the form V'+J, Vi+>~2,..., terminating with either V1 or V° accord ing as (i +j) is odd or even. In fact it is not necessary to terminate the sequence of terms "by hand," since it turns out that the functions
(2.7)
the structure constants are transformed according to , q2rg'l{m,n)^
Z(i,m)Z(j,n) , . \ . ' ' .q*&{m,n),
(2.8)
Z(i +j - 2r,m + n) while for the central terms we have while for the central terms we have rt(m)the-zeroth-order Z ( i , m ) Z ( i ,component -m)q2icl{m)(corresponding . (2.9) In particular, to maintain to the w„ In particular, to maintain the zeroth-order component (corresponding to the w„ algebra) unchanged, one is restricted to simple scalings of the form Z(i, m) = A'i>m, where the vm component simply expresses the fact that the mode number is additive. As mentioned in ref. [7], this class of transformations has the sole effect of taking q->\q, demonstrating that the algebras (2.1) for all (non-zero) q are isomorphic. We have taken advantage of this freedom by taking q2 -» \q2 with respect to ref. [7]. Fixing a particular value of q amounts to fixing a convention for the relative sizes of the fields V^. In order to agree with the conventions of Zamolodchikov [1], for example, we should take q2 = ^. 2.1. DIVERS EXPRESSIONS FOR THE W„, STRUCTURE CONSTANTS
The coefficients
V
(-h)k(\)k(-r-\)k(-r)k
*lr £o*>H-a(-;-a0+;-2r + §)/
(2 10)
-
Note that the summation is automatically cut off at k = r, since the factor (—r)k
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C.N. Pope et al. / Racah-Wigneralgebra
vanishes for k > r. Comparing eq. (2.10) with the definition of the generalised hypergeometric function (A.3), we immediately see that _I
1 - r - l
2 > 2 >
^ = 4 ^ 3
—I
'
2'
-r
'
(2.11)
5,-/-5.'+;-2r+§'
Owing to the particular values of the arguments, this is a terminating saalschiitzian 4 Fj(l) series (as defined in appendix A). For the special case i = 0, it turns out that the coefficients
_
i-j-2),(-j+r), (2 12)
* * ~ (-/-*),(-;■ + ' - § ) , '
"
which can in turn be expressed in terms of gamma functions, if desired. One thus obtains a relatively simple expression for the commutator of any Virasoro genera tor with an arbitrary generator in W... The fact that the quantities
Z(i)Z(j) 4> 'I =
z{i+j_2r)
xy2(-l)y
, («' + J " 2 r + §) 4 (i + 1,; + 1, i + / - 2 r + 1)
sin IT/
,,.
..
5
. . .
i
i > (2- 13 )
where Z(/) = V'!(' + 2 ) ! / ( / + 2 - ) !
(2.14)
and the function A(a, b, c) is defined in eq. (A.2). The factors involving the Z(i) can clearly be absorbed into a rescaling of the generators, as in eq. (2.7).
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C.N. Popeetal. / Racah-Wigneralgebra
197
Several comments are in order concerning eq. (2.13). Under usual conditions one does not tend to encounter 6-j symbols with quarter-integer arguments; however, there is in principle no obstruction to defining such objects, and in fact 6-j symbols with continuous ranges for their arguments have received a certain amount of attention in the literature (see, e.g., ref. [11]). A more serious point is that the expression on the r.h.s. of eq. (2.13) is only defined through a limiting process: since ;' is an integer, sin vj is zero, while it turns out that the 6-j symbol is formally infinite. Although it is possible to make sense of the formal expression given in eq. (2.13), we have so far found the representation of the structure constants in terms of 6-j symbols to be neither calculationally useful nor indicative of specific underlying structures. Therefore, for now we shall view the form (2.13) as an interesting curiosity, and continue to consider the coefficients <£2;r as defined through the unambiguous formula (2.11), equivalent to eq. (2.4). With a little manipulation one can also write the polynomials N{[(m, n) as given in eq. (2.5) in terms of generalised hypergeometric functions: A#(#i!,n) = [i + l + m ] 2 r + , [ 2 / + 2]2 r + i,F 2
2/ + 2 - 2r, -j — 1 -n, -2r 1 ;i — 2j - 2, i + 1 + m - 2r (2.15)
There is in addition a formal representation of N£(m, n) in terms of Clebsch-Gordan coefficients. To see this, we first apply the transformation (A.7) of terminating 3 F 2 (1) series, yielding NiHm.n) = [i + 1 +m]2r+1[j+
1
-n]2r+liF2
-i— \+m,—j—\—n, — 2r - 1 i + 1 + m - 2r, j + 1 - n - 2r ; i (2.16)
which can then be turned back into a summation 2r+l
k 2r 1 "ii(m,n)=2r E£\-l) ( Z ) * =0
(i + 1 + m) \(i + 1 - m)!(/ X
(i + m - 2r + k)!(i + 1 - m - k)\{j
+ 1 + n)!(;' + 1 - n)! + 1 + « - & ) ! ( ; - 2r-n
+ k)
E(-iW2'+1 X[i + 1 + m]2r+i_k[i
+ I -m]k[j
+ I + n]k[j + 1
-n]2r+l_k. (2.17)
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C.N. Pope et al. / Racah-Wigner algebra
This is precisely the summation appearing in the van der Waerden expression for the Clebsch-Gordan coefficients (see, for example, eq. (3.170) of ref. [9]). We find (2r+l)! N¥r(m,n) = — — — : —^ 2(i +j -2r+ | ) ' A(i +\,j+l,i
+j - 2r + 1)
K(i,m)K(j,n) v w
i j2,+ 1, i+j ' ' ' i:ii+ p i + 1, x „ . . . '' \yi.^ci:\\ - +\
K(i+j
:
(2-i8)
- 2r + 1
-2r,m+n)
where K(l,m) = •/(/ + 1 + m)!(/ + 1 - m ) \ .
(2.19)
Note that the Clebsch-Gordan coefficients which appear in eq. (2.18) vanish outside the "wedge" of generators defined by \m\ < (i + 1), whilst the K(i,m) are singular there. Thus although eq. (2.18) is apparently defined only within the wedge, it may be formally extended by analytic continuation to eq. (2.17), which is well-defined everywhere. In the next section, we shall be concerned with the algebra W„ restricted to within the wedge, i.e. WA. Since the factors of K(l,m) appear in precisely the form (2.8), it will be possible to work with rescaled generators for which those factors are removed from the structure constants. A fair amount of simplification occurs if one combines eq. (2.13) with eq. (2.8) to give an expression for the structure constants g'2{(m,n) in "angular-momentum language." Upon performing certain rescalings of the type (2.7), we find
\f/2C^:l^'-^'
gZ(m,„)^(i+j-2r+
. V ( - 1)
sin7ry '
•(i-y-i)
H<+y) + i
- '
-!(<+;)+'•-!
-2U+J)-r + \
-W (2.20)
Because of the aforementioned complications in handling the 6-j symbol, however, we prefer not to emphasize this approach. The Clebsch-Gordan coefficients satisfy a useful identity, which can be used to recast the Jacobi identities for our algebra in a considerably more tractable form, at least for the component not involving the central terms. The identity reads (see eq. (2.67) of ref. [10]) Ctt,n+pC£n+p,m+n+p=U-iy+'+k+'y/(28+l)(2h
^'m,n,m+n'-'m+n,p,m+»i+p •
+ l)
i k
j I
(
h\ gj
g
V^-^^7
586
C.N. Pope et al. / Racah-Wtgner algebra
199
Using this identity (or the relevant analytic continuation) the factors involving the N£(m,ri) may be stripped off the Jacobi identity that the structure constants g'Jr(m, n) must satisfy. One finds that the Jacobi identity
[Ki.[^''^*]]+ KM K /> K ™]] +
W»[KJ.^']]
=0
( 2 - 22 )
(modulo central terms, which may be handled separately) is reformulated as the condition
mW-f'" (2i + 2; - At + 3)
=
£ /' + * J + l
i+j-2t + l
,j -_0 0 \ * + l
j + k - 2s + I
i+j + k-2r+l
+ («*♦/).
\Mk^j^k-2s
r2sV2r~2s
(2-23)
where $% is defined by
n
=
4(i + l , ; + l , « + ; - 2 r + l ) '
(2-24)
The result of this manipulation is that the dependence of eq. (2.22) on the mode numbers m,n,p has been completely factored out, considerably reducing the number of identities which must be verified. (Note that the 6-j symbol appearing in eqs. (2.21) and (2.23) is perfectly regular and well-defined, unlike the singular 6-j symbol occurring in eqs. (2.13) and (2.20).) 2.2. THE OPERATOR-PRODUCT EXPANSION FOR W„
It is often useful for studying extended conformal symmetry to represent the algebra in terms of an operator product expansion. To do this, we define a set of conformal fields Vi(z)=l2VJ,z-n-i-2-
(2-25)
m
It is convenient to introduce the quantities flHm,")*
**
M&(m,n),
(2.26)
where ^ r ( m , n ) = 2 E 1 ( - l ) * ( 2 r + 1 ) ( 2 / - 2 r + 2),[2; + 2 - * ] 2 r + 1 _ , m 2 - 1 - V (2.27)
587
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C.N. Pope et al. / Racah-Wigner algebra
and <j>'{r is given by eq. (2.11). The M%r(m, n) contain just the terms of total degree (2r + 1) in m and n of the polynomials N£(m,n). Conversely, the full N^r(m,n) may be obtained from the M£(m, n) by replacing each monomial manp by the expression [m + i + 1 ]a[n +j + l]p, which then generates the proper terms of lower order in m and n. The two alternatives may be formally related through a simple change of variable in the definitions of the conformal fields V'(z). In fact, fiiim, n) would replace the g'2'r(m, n) in the commutator (2.1), if one were to make the field redefinitions for which the central terms become pure monomials, as we did in ref. [7]. In the present context, however, we are concerned with the algebra (2.1) for which the central terms take the standard form (2.2), and we only introduce the f^r(m,n) as a formal device in order to express the corresponding OPE most economically. In terms of the polynomials f^r(m, n), the OPE corresponding to the algebra (2.1) reads V'(z)V'(w)
~ -9 2 , 'c,* , 7 (3,) 2 , ' + 3 -^- - E g 2 7 m , a J K ' ' Z
(W
° - (2-28)
r
In the Virasoro sector this gives In the Virasoro sector this gives c
1
V°(w) 2
4
2(z-w)
1
2
\(z-w)
z-w
dw\v°(w),
(2.29)
as required, recalling that V°(z) is simply the energy-momentum operator T{z). For the operator product of the conformal-spin-3 field Vl(z) with itself, eq. (2.28) gives q2c
€
V2(w)
1
4o2 x V°(w) - -j- (2dt - 3d? dw + 3d2 dl - 2dl) ^ - ^ 8q2c (z-w) Aq2 I
/
4
2
\(z-wy 60
5 \(z-w)A
\ ,
z-w 30
3
(z-w)3
d
w
w
+-
_fl2+_—-
(z-w)
3
3|
K
0
( w ) >
w (2.30)
588
C.N. Pope et al. / Racah-Wigner algebra
201
One may verify by inspection that this precisely coincides with the OPE for the W3 algebra as presented in ref. [1], with the identifications q2 = j ^ , Vl(z) = W(z) and V\z) = \b2 A(z). The fact that V2(z) is not a primary field (for q * 0) is seen in the OPE V2(w) z-w /
4
\(Z-H»)
1 z-w
32q2 5
V°(w) z-w \92q2
\ , /
5(z
—w)
The final term involving V° would be absent if V2 were a true spin-4 primary field. 3. The "wedge" algebra, SL(2, R) tensor operators and WJ[JI,) In this section we focus attention upon the "wedge" of generators V^ for which \m\ < (i + 1). One can verify that the commutator of any two generators within the wedge only involves generators within the wedge. The resulting wedge subalgebra of W„, which we denote WA, has the feature that it is anomaly free; that is, the central terms vanish for all commutators, as may be seen from eq. (2.2). The algebra WA is the natural generalisation of the SL(2, R) subalgebra of the Virasoro algebra, generated by L„ L 0 and L_,. 3.1. ALGEBRAS OF SU2.R) TENSOR OPERATORS
Our algebra WA is not the only example of an algebra that can be constructed involving the generators within the wedge. In fact, there is a family of similar algebras that has been discussed previously in the literature, obtained by consider ing the set of all polynomial tensor operators in the enveloping algebra of SU(2) or SL(2, R). As we shall now describe, our algebra WA is in fact a special case of the family of SLX2, R) tensor-operator algebras. The tensor-operator algebras may be constructed in the following way. We begin by considering the SL(2, R) generators L ±= L ± , and L 0 , which satisfy [L±,L0]=±L±;
[L + ,L_] = 2L 0 .
(3.1)
The Casimir operator may be written as Q = (L0)2-±(L+L_+L_L
+
).
(3.2)
The three generators themselves transform as the 3 of SLX2.R). Higher-tensor operators r j , ( - / < m < / ) , transforming in general as the (21+ l)-dimensional
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C.N. Pope et al. / Racah-Wigneralgebra
representation of SL(2, R), are constructed from appropriate polynomials of degree / in the L's. Specifically, we start with the highest-weight state T,' = (L+)', and then construct the lower-weight states in the usual way, by (/ — m) successive applications of L_:
7l = ^ i
(-2/),.
[L_,[L_,...[L_,
(L + )']...]]
m .
/ - m times *
(-21)
•
\l-m
(AdLy-m(L+y,
0.3)
l-m
where Adx(Y) = [X,Y]. The operator L'±m (for m > 0 ) may be expressed as a polynomial in L 0 , with coefficients involving the Casimir operator Q, multiplying Lm±. With our normalisation, the leading coefficient is always unity: T'±m = ( L ' 0 - ± \m{l~m)L'0-m-'
+ ...)Lm± .
(3.4)
This is not the standard normalisation, but will prove to be the most convenient for purposes of comparison with the algebra WA. Acting upon a Hilbert space in which the quadratic Casimir takes on a definite value Q = ft, the operators T[m close into an infinite-dimensional algebra (para metrised by fi), which we may label S7~(ii). Equivalently, ^"(^.) is the quotient of the enveloping algebra for SL(2,R) by the ideal generated by (Q -/x). From the consideration of SL(2, R) covariance, we would expect that this is the most general family of algebras for tensor operators in this set of SL(2, U) representations. In particular, we would therefore expect that our wedge algebra WA should coincide with J?"(/x) for some specific value of fi. To determine the value of p. corresponding to the algebra WA, it is sufficient to look at the commutator of Tj with Ttx. These operators are given by T/ = (L + Y,
r!, = ( L 0 - i ) L _ .
(3.5)
As one verifies by a straightforward calculation, they commute to give [T/,T2_l]=\j(6(L0)2 =3
^-i+
+ 6(j-\)L0
2(2/+D
+ (j-l)(2j-l)-2Q)(L
-727nriF1
+
y~1
(3 6)
-
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C.N. Pope el al / Racah-Wigner algebra
203
(modulo Q — n). On the other hand, we have from eq. (2.1) that [V/-l.Vl-i]
-3;^
1 +
8^
( ;
^1.)}(
+ 1 ) )
^.
(3.7)
Comparing these two expressions, we see that they agree provided that one makes the identifications V^ = rj, + 1, q2 = -^ and in addition fi = 0.
(3.8)
Thus the wedge subalgebra WA contained in W„ is determined to be the SL(2, R) operator algebra y~(0), specified by the value fi = 0 for the quadratic Casimir. (Note that although one might be accustomed to thinking of a n = s(s + 1) representation of SU(2) or SL(2, R) as being (2s + l)-dimensional, we are not restricted to considering this discrete set of finite-dimensional representations. In particular, for any value of the parameter fi, we can allow the representation to be infinite dimensional. For present purposes, the representation space can remain unspecified.) By examining the hermiticity properties of the tensor operators Tlm, it is rather straightforward to see that the operator algebra is a real form of A„ of the type SL(oo,R). (Alternatively, by sending Tlm - > ( - l ) ' / 2 J ^ , one gets another non-com pact real form of A,,, namely SU(°°,«).) This conclusion holds, of course, for all values of the parameter /JL; in particular, we see that our wedge algebra WA is isomorphic to the p = 0 version of SU«>, R). Note that versions of SL(oo, R) for different fi are not isomorphic to each other. This does not contradict the well-known classification by Kac of infinite-rank Lie algebras, in which he obtains only A„ and A+m as N -»°° limits of AN [12]. To realize this limit, Kac considers a very specific type of construction which is perhaps natural if one is attempting to prove a classification theorem, but does not appear appropriate in a context such as ours. The commutation relations for the SL(2, R) operator algebra ^"(/i) for general ji may be written in the form [Ti+\T,!+l]
=gi'(m,n; M )r;V„ + 1 + qhK™^-^)^'^ +
...WgUm,n;n)T£;l->°,
+
q'g^m^^)^'^ (3.9)
where the structure constants reduce to those given in sect. 2 when /J. = 0. For general /i, the structure constants can be written as gyr(w,W;M)-2(2r+1),^(w,n),
(3.10)
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where A^(m,/i) are still given by eqs. (2.5) or (2.17), and the 4>'^r(fi) are polynomials in L/A of degree r. Thus in particular $J/(/LA) = <£(0) = 1. For general r, the result is a relatively minor modification of eq. (2.4): ' * [(27-3)(2/+l)-16M](2r-2/ + 3)(i-f+l) * _ 0 / - i / ( 2 i - 2 / + 3 ) ( 2 / - 2 / + 3)(2i + 2 / - 4 r + 2/ + 3) ' *
'
We have arrived at this formula by a combination of analytic calculation and conjecture. For example, eq. (3.6) can be used to rigorously obtain ^ ( M ) f° r all ')• We have checked the general result (3.11) extensively by using algebraic computing techniques, and we claim that it is correct for all r. If we parametrise fi in terms of a variable s according to M= 5(5 + 1),
(3.12)
the expression in brackets in eq. (3.11) factorizes: (2/ - 3)(2/ + 1) - 165(5 + 1) = (2/ - 3 -
4J)(2/
+ 1 + 4s) ,
(3.13)
and it is straightforward to see that the expression (3.11) for general /A continues to be expressible as a saalschiitzian 4F3(1) generalised hypergeometric function, with a simple modification of the expression (2.11): - j - 2 s , f +25, -r
\,~r
-'-£,-;'-5.'+/-2r+§'
(3.14)
(Note that this is invariant under the involution s -» -s - 1, as required for a function of /LA.) 3.2. ^ ( / i ) FOR OTHER SPECIAL VALUES OF M
An explicit realisation of the SL(2, U) operator algebras for arbitrary fi is provided by using the so-called Jordan map to write the SL(2, U) generators as L + = iaxa2,
L_ = ia2a1,
L0 = Ka2<*2— a i^i) >
(3.15)
where aa and aa are boson operators satisfying [aa,ap]=Sap,
[aa,ap] = [aa,ae] = 0
(see e.g. ref. [9]). For the special value /x = - ^ , it is possible to replace (3.15) by L + = -{ia1,
L_=\ia2,
L0= -j(aa +aa),
(3.16)
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C.N. Pope et al. / Racah-Wigneralgebra
205
where a and a satisfy [a, a] = 1. This non-standard boson realisation of the generators of SU(2) (or SL(2, R), in our case) is due to Biedenharn and Louck ([13] and ch. 5, topic 3 of ref. [10]), who coined the term "symplecton" to describe it. For IJL = - j£, which corresponds to s = - 5 or s = - f in eq. (3.12), one easily sees that the hypergeometric function in eq. (3.14) collapses to simply 1 for all values of i, j and r. This precisely agrees with the computation of the algebra of tensor operators for the symplecton by Biedenharn and Louck [10,13], providing further non-trivial checks on the correctness of our general expression (3.14). More recently, the symplecton algebra has arisen as the symmetry algebra in a higher-spin theory Fradkin and Vasiliev [8]. The construction of this higher-spin algebra in terms of tensor operators was described in ref. [14]. It was also shown in ref. [14] that the ii = oo case of the SLX2, R) operator algebras corresponds to the area-preserving algebra of a two-dimensional hyperboloid. In fact the ii -»oo limit of the operator algebra ^(fi) has a relatively simple form, for which the structure constants can be given explicitly in closed form. From eq. (3.11), one can see that as fi tends to infinity only the k = r term in the sum is important. After making an appropriate rescaling of q in eq. (3.9) to absorb the parameter ft, and other rescalings of the generators T'm -» T'm to simplify the expression, we find that the operator algebra in this limit assume the relatively simple form r _.
\T
_., ^ y[2k+~\{i+j + k + 2)A2(\i,\j,{k) TJ] = Y —V2 2
.t ' riik
Tk
(3 17)
where the summation is over all values of k such that i+j + k is odd and the Clebsch-Gordan coefficients are non-zero, and the function A is defined in eq. (A.2). A whole class of finite-dimensional tensor algebras has been discussed exten sively in the angular-momentum theory and related mathematical literature [9,10], corresponding to Wigner operators (which are just rescaled versions of our 7J,) acting on the finite-dimensional space of spin-s states. For any given finite s, there is precisely one algebra, namely the standard A 2 j algebra. (Various real forms are possible, corresponding to different scalings of generators by factors of v ' - 1 •) When s = oo, however, one can have many inequivalent A„ algebras, as we discussed earlier. By taking the limit 5 -»oo for the Wigner tensor-operator algebras, one obtains a specific infinite-dimensional algebra. By construction, the value of the quadratic Casimir /A, given by eq. (3.12), will be infinite for this algebra. Thus we should be able to rederive the algebra (3.17) (i.e. the ft = oo special case of our family of wedge algebras parametrised by (i) by taking the 5 -»oo limit of the operator algebras given in refs. [9,10]. For finite s, the
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Racah-Wigneralgebra
finite-dimensional operator algebra takes the form
[T^.TV] = -2E(-1)V(2/+ l)(2y+ 1) {j I
k
s)c^m+nT^+n,
(3.18)
where the summation is over the same range as in eq. (3.17). To take the s -* oo limit, we first use eq. (A.14) to express the 6-j symbol in terms of a saalschiitzian 4 F 3 (1) hypergeometric function. Expanding the coefficient of the resulting 4 /" 3 to leading order in 1/s, we find ii \s
J s
i-iy+jk\A(ij,k)
k\ s)
y/2s~(k-i)\(k-j)l(i+j-k)\ x4F3
-i-j
k - 2s, k - i -j, - i, -j -2sl,k-i + l,k-j + 1 ;i
(3.19)
It is now necessary to evaluate the 4 F 3 symbol in the 5 -» a> limit. To leading order, it reduces to a well-poised 3 F 2 (1) function which can be re-expressed as a Clebsch-Gordan coefficient (as in eq. (A.15)); however, for the values of i, j and k relevant here, all the Clebsch-Gordan coefficients will be zero. (Alternatively, this follows directly from Dixon's theorem (A.9), which evaluates the general well-poised 3 F 2 (1) series.) Thus we must look at the next term in the 1/s expansion. We find
4^3
k — 2s, k - i —j, — i, —j -i-j-2s-l,k-i+l,k-j-l (i+j +
: 1
k+l)(k-i-j)ij
2s(k-i+
!)(*->+1)
k-i-j 3^2
k-j
+ 1,-i + 1, - ; ' + 1 ;i + 2,k-i + 2
+ 0(l/52). (3.20)
The operator algebra in the 5 -> oo limit then takes the form r 1
\j'
,
"'
T'n J
_ * ! ( / + / + * + 1)«V(2« + 1)(2; + 1) 4 ( 1 , ; , * )
=y
X
(k-i
+
X3f2
k-i-j+\, k-j
\)\(k-j+l)\(i+j-k-l)\
+ 2,k-i
-i+l,-j+\ ; i C%n,m+jLn> +2
after rescaling the generators to absorb the (2s) constants.
3/2
(3-21)
factor in the structure
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207
The 3F2 function in eq. (3.21) is nearly poised of the first kind (see the appendix A for the definition of this term); it can be summed to give a closed-form expression, using eq. (A.10), in our special case where i +j + k is odd. Using this, and the freedom to rescale the generators Tlm by arbitrary functions as in eq. (2.7), we finally see that the s -* <» limit of the SL(2, R) tensor-operator algebras indeed reduces to the previous expression (3.17) which had been obtained directly from our general formula (3.11)*. 3.3. THE ALGEBRA WJ,i) OUTSIDE THE WEDGE
We have seen in subsect. 3.1 that there is a one-parameter family of SL(2, R) operator algebras that includes, for the special case /A = 0, the wedge subalgebra WA of our W,, algebra. Thus we know that the ft = 0 operator algebra can be extended "beyond the wedge" to give the full W., algebra, which can then be augmented with a central extension. It is natural to enquire whether the SL(2, R) operator algebras can be extended beyond the wedge for other values of the parameter ft. As we remarked in sect. 2, the structure constants in the W„ algebra (2.1) have the property that they vanish for all i, ;' and r such that i +j - 2r < 0. This has the effect of automatically terminating the descending sequence of terms on the right-hand side with either V1 or V°. In a formal sense, one can continue any of the SL(2, R) operator algebras beyond the wedge, provided that one introduces extra generators V^ for all i < 0. For any value of fi, the structure constants given by eqs. (3.10) and (3.14) will then give an algebra Wj/i) that satisfies the Jacobi identity both inside and outside the wedge. However, for generic values of /i one cannot consistently truncate the theory to the i > 0 sector, since the Jacobi identities will only be satisfied provided that one does not artificially terminate the sequence "by hand". For example, we have seen that for the special value n = - fg, the coefficients
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C.N. Pope et al. / Racah-Wigneralgebra
From the general structure of the central terms (2.2), which, to leading order, are proportional to m 2 , + 3 for the generators K^, it would seem that the inclusion of generators with i < - 1 in the algebra is likely to preclude the possibility of finding a non-singular central extension for general /A. As we mentioned in ref. [7] for the usual W^, = W„(0) algebra, the truncation to the even-spin generators forms a subalgebra W„/2 (corresponding to WD„ as opposed to WA*,, following the notation of the authors of ref. [2]). This property also holds for Wj(p.)> yielding a subalgebra W00/2(/x) of even spins, positive and (possibly) negative. It is instructive to consider the commutator of two Virasoro modes in the general Wj/x) algebra. It turns out that the polynomials /v*2°°(m, n) and N£°(m, n) vanish identically, a fact which is of course independent of the value of /i, so the corrections to the commutator begin with K -6 (with formal spin - 4 ) . Explicitly, we have [Lm,Ln] = (m-n)Lm+n
+ 0V-2+n + 0V-tn
+ q6g?)(m,n;»)Vm
+ ...
(3.22)
where g™(m,n;n) = 2(m 3 - m ) ( n 3 - n ) ( m -n)
(3.23a)
- Imn + 2/z2 + 16)4>°V) (3.23b)
with 2 io
4>6°°(M) = T M 2 ( l + 4 * ) ,
^
( M ) =
9X25X11M2(1
(3.24a)
+ 4M)(71 + 12M)
*
(324b)
As required, the corrections vanish for fi = 0, and for general fi the negative spins do not appear when Lm and Ln are within the wedge. Furthermore, the expres sions (3.24a,b) reduce to 1 for the symplecton (/x = - ^ ) . It is interesting to note that there is one other value besides /i = 0 for which the negative-spin generators decouple: /t = — 5, corresponding to s= — \. This property persists for other cases we have checked, and we conjecture that the algebra W„(- j) may be consistently truncated to the spin > 1 sector (one needs to include the spin-one
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C.N. Pope et al. / Racah-Wigner algebra
209
field V~1 if one includes any generators of odd spin). We intend to investigate the special significance of the value fi = — j in a separate work. 4. An associative product underlying W^ The structure of a Lie algebra (such as W^) is completely specified by giving the Lie bracket [x, y] for each pair of algebra elements x and y. In the Lie theory this object is viewed as a fundamental bilinear product, subject to certain requirements (antisymmetry and the Jacobi identities) which are necessary for consistency of the Lie algebra. One need never refer to an explicit realisation of the bracket [x, y] as an commutator xy-yx.U such a realisation should happen to exist (in terms of an associative product xy defined on the algebra), the Jacobi identity for the commu tator is then identically satisfied. In this section we discuss a realisation of the WJ/J.) commutation relations (for c = 0)
[KW\=
E?2^'","^)^2'
(4.1)
r-0
as the antisymmetric component of an associative multiplication:
Guided by the expression (4.1), which should correspond to the difference (4.2) of two star products, we are led to propose the form
K*K = \ L q'g^m,n;n)V^-'
(4.3)
a=-l
as a natural candidate for a lone star product (LS product). The functions constituting the coefficients of the various generators in the product (4.3) are direct generalizations of the functions appearing in (4.1) (as defined in eqs. (3.10), (3.11) or (3.14) and (2.5) or (2.17)), with r replaced with \a. Note that the resulting expression for
+l
N>i(n,m),
(4.4)
as can be seen by reversing the order of summation in eqs. (2.5) or (2.17), or equivalently by applying eq. (A.13) to (2.15) or (2.16). This means that the terms with even a appear in the commutator as in eq. (4.1), while the anticommutator is
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C.N. Pope et al. / Racah-Wigner algebra
given by the terms with odd a:
E« 2 , _ 1 ^-i('«.«)Kiv„- 2 r + 1 ■ (4-5)
{Ki.K/} = K * yj+yi*yj.=
/=0
We display a few examples of LS products for yt, = 0. The LS product of two Virasoro modes contains a spin-3 component, as well as the usual Virasoro mode in the antisymmetric component: Lm * K = (l/4*)^ + „ + i{m-n)Lm+n
.
(4.6)
Other LS products involving spin-2 and spin-3 fields read
Lm * V: = j-qV^n
+ | ( 6 m 2 - 3mn + n2 - 4 ) L m + „ ,
+ \{2m-n)V^+n
(4.7a)
V^ * Ln = — Km2+/I + \(m - 2n)Vj,+„ + | ( m 2 - 3mn + 6n2 - 4 ) L m + „ , (4.7b)
VJ, * V„l = ^ K n 3 + „ + (m - /z)Km2+/, + y (2m 2 - 3m« + 2* 2 - A)Vj,+n 2q2 + —(m
-n)(2m2
- mn + 2* 2 - 8 ) L m + n .
(4.7c)
This is more than enough information to compute the LS product of three Virasoro modes, which read
Lm*
1 Ln* Lp= —-IV2+n+p V2 + ] 6
1 + — —{m-p)Vj,+n+p
2 m+n+P 2
4
2
+ -jL(3m - 2n + 3p2 + mn - Amp + np - 2)Lm+n+p.
(4.8)
Already in this simplest case, the associativity condition provides rather non-trivial checks upon the forms of the LS products. In the ju.-deformed lone-star algebra, which we may denote by LSA(/i), the product of two elements involves (for generic ix) an infinite sum of generators whose spins are unbounded below. However, it is still feasible to verify associativity of the product, since the coefficient of a given generator in any multiple product only involves a finite number of terms. (This is related to the analogous property for the Jacobi identities of WJ/x).)
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211
It is interesting to note that LSA(/x) contains an identity element, given by the zero mode of the spin-field, multiplied by 4
= K*V^
= JjV^-
(4-9)
As an illustrative example, we consider the LS product of two Virasoro modes in LSA(ji); since the commutator is considered in subsect. 3.3, we need only examine the symmetric component here. We find that N$°(m, n) vanishes identically, so that the anticommutator has the form {L m ,L„} = — V:+n+qgr(m,n;n)V-ln + q5g?(m,n;fi)V^n
+ OV-ln
+ q7g<*>(m,n;n)Vmln+ ... .
(4.10)
The first few terms are given by g°°(m,n;n)
= H"i2-mn
+ n2-l)4>?'(n),
g™(m,n;ri
= -Hm3-m)(n3-n)4>?>(n),
g?{m,n;iL)
= - f (m 3 - m)(n 3 - n)(m2 - 5mn + n2 -
(4.11a) (4.11b) 4)4>°°(M)
(4.11c)
with
>5°V) = i x 2 V ( l + 4 M ) , (4.12a), (4.12b) 2
( 1
+ 4M)(57 + 4 M ) .
(4.12C)
As required, the corrections to eq. (4.6) vanish for /i. = 0, and the <j>™ are all equal to one for /i = - ^ . Just as for the antisymmetric component discussed in subsect. (3.3), we find that the negative-spin fields decouple for the special value fi= — \, as well as for /i = 0. The LS product represents an extension outside the wedge of the standard product of SIX2, R) tensor operators in ST(\i), just as Wjji) is determined by the extension of the commutation relations of y(n) outside the wedge. Whenever H ¥= 0, one must adjoin the unit operator to ^"(p.) in order for the multiplication to close. (This is in contrast to the commutator algebras within the wedge, for which the SL(2,R) singlet generator always decouples, yielding the overall product algebra GU<»,R) = R X SL(<»,R). As in subsect. 3.1, one should identify Vj, with
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T„+l and set q = \; this means that the new generator T° at the tip of the wedge is then precisely the identity element AqV^x. An example of eq. (4.10) applied within the wedge reads {r01,r01} = 2702 + fM,
(4.13)
consistent with the definition (3.3), which gives 7"02 = (rj) 2 - 5Q. Another applica tion of eq. (4.10) reads {7/,ri 1 } = 2r 0 2 -f M ;
(4.14)
eliminating K02 from eqs. (4.13) and (4.14) simply gives the condition Q = ft. The product of operators described in this section is analogous to the product of Racah-Wigner operators that defines the Racah-Wigner algebra [9,10]. Indeed, the operators within the wedge coincide, up to normalisation, with the so-called special Wigner operators [9,10], which form a subset of the Racah-Wigner operators for which the spin-changing parameter is set equal to zero. The formal lone-star product is also evocative of the fusion rules of rational conformal field theory [16], which in some sense form the quantum analogues of the (classical) Racah-Wigner algebra.
5. Towards a geometrical interpretation of W^ The relationship between area-preserving algebras of two-dimensional surfaces and the W^ algebra has received a certain amount of attention [6,17]. In light of the group-theoretic picture that has emerged in the preceding sections, we further reveal this very interesting relationship. In particular it is the co-adjoint orbits of SL(2, R) on which the area-preserving algebras are relevant to the class of tensoroperator algebras in the previous section. It is well known in the literature that the co-adjoint orbits of any finite, semi-simple, Lie group naturally define a symplectic manifold. The symplectic structure inherited from the group can be used to yield a Poisson bracket, which leads to a geometrical approach to quantization. From algebraic point of view, the Poisson bracket is the classical limit of the quantum commutator. However, by extending the Poisson bracket to the Moyal bracket [18], the essence of the full quantum algebra is captured in a classical construction. In particular, one can reformulate our previous tensor-operator algebras in terms of Moyal brackets of functions on the co-adjoint orbits of SL(2, R). In the three-dimensional vector space R3 of the Lie algebra of SL(2, R) the co-adjoint orbits are defined by the invariant quadratic Casimir. We associate the coordinates (x,y,z) with the generators (L + , L_,L0). Thus the co-adjoint orbits
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C.N. Pope etal. / Racah-Wigneralgebra
213
are the two-dimensional surfaces given by z2-xy = n.
(5.1)
If fi < 0, fi = 0 or M > 0, the orbits consist of either a hyperboloid of two disconnected sheets, a cone or a hyperboloid of one sheet, respectively. In particular, we see that our wedge algebra WA corresponds to the case where the co-adjoint orbit is a cone. Defining x"; a = 1,2,3 to be (x, y, z), we obtain the following Poisson bracket on the co-adjoint orbit: {F,G}nmcc"'xcdaFdbG,
(5.2)
where indices are raised and lowered using the indefinite-signature metric of SL(2,IR). The Poisson bracket (5.2) is induced from U3 by restricting the functions F(x") and G(x") to lie on the two-dimensional surface defined by eq. (5.1). It is easy to check that substituting x" for F and xb for G, we recover the SIX2,R) algebra {x",xb)=ecabxc.
(5.3)
The tensor operators that we discussed in subsect. 3.1 will now be represented instead by tensor harmonics constructed as homogeneous polynomials in x" in the usual way rm-^.,....,*"'-*"',
<5-4)
where the Aa a are symmetric traceless tensors. By defining an appropriate Moyal-type bracket, which arises in the deformation theory of the Poisson bracket, one will then recover the SL(2, R) operator algebras of subsect. 3.1 in terms of these tensor harmonics. We already noted in the introduction that the leading-order terms in the W^ algebra (i.e. the w,, algebra) can be obtained from the Poisson-bracket algebra of functions
KW+m+y+i
(5.5)
on a two-dimensional phase space. Thus the association of (L+,L_,L0) (x, y,z) now corresponds to x = q2p,
y=P,
z = qp.
with
(5.6)
Thus xy =z 2 , and so again we recover the result / t = 0 for this algebra. By
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rewriting eq. (5.5) in terms of x and y, we obtain yi —x0+l-m)/2
(i+\+m)/2
(5 7)
and from eq. (5.2) the Poisson bracket becomes
(^--(^qTf-if-lr-ir)-
<">
By redefining x -»x 2 and y ->y2, this becomes, after a constant rescaling,
(5 9)
("-••«>--hf-^-if-if •
-
where now the functions V^ are given by I/i
„i + 1 — m.,i+ 1 +m
(5.10)
It is interesting to note that if one replaces the Poisson bracket in eq. (5.9) by the standard Moyal bracket, then one obtains expressions on the right-hand side that precisely reproduce the N{'r(m, n) part of the structure constants g'Jr(m, n) of the W^ algebra (2.1). Specifically, the Moyal bracket acting on a pair of functions / and g takes the form oc { / > #}Moyal =
E {/'S/Moyal.r 7--0
(5-H)
where (-l)r
/ d
d
d
d
"2r+l
{/.s}Moyu=7Trr7T7| — — " — —g I (2r+i)!\a^^r"a^a7
%■
(5-12>
Identifying / with V„ and g with K„', as in eq. (5.10), and comparing the result of expanding the expression (5.12) with the expression (2.17) for N^r(m,n), one finds
{Kl. K / W , =
(-1)'
( 2 r + 1},
mm, n)V^-2r.
(5.13)
Thus the W„ commutation relations may be written
[vlvi]
=E r= 0
tt-q2y
(5-14)
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C.N. Pope et al. / Racah-Wigneralgebra
215
Thus a Moyal-type expression encodes much of the structure of the W„ algebra, barring the
6. Discussion The WN algebras, hence presumably also W,,, arise as the symmetry algebras of certain two-dimensional conformal field theories. Even though it describes a system with an infinite number of higher-spin fields, the fact that W,,, unlike W^, is a linear algebra may mean that such systems are more accessible to explicit calculations. The starting point for investigations of this kind would be to study the representation theory for W.,. One natural suggestion is to look for an extension to W^ of the series of minimal model representations constructed by Friedan et al. [19] for the Virasoro algebra (the simplest W-algebra W2), which have central charge
where k = 1,2,3,... labels the particular model. In ref. [2] an analogous series of models is proposed for the general WN, having central charges c(N,k) = (N-l)\l-= 2k + 0(l/N),
(6.2)
where again the label k ranges over the positive integers. This suggests that if a corresponding series of minimal model representations for W„ can be constructed, the central charge should take on the simple and suggestive values c(°o, &) = 2k. One might expect that the general representation theory for W., will be a rich subject; it may turn out that the underlying algebraic structures discussed in the preceding sections might make this a more manageable problem than one might at first suspect. Whether the corresponding field theories might go beyond the class of rational conformal field theories is not clear. Another way of constructing a field theory based on the W,, symmetry is to make use of the method of co-adjoint orbits to build an invariant action. When applied
603
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C.N. Pope etal. / Racah-Wigner algebra
to the case of the Virasoro algebra, this yields the action for Polyakov's two-dimen sional gravity [20]. It seems natural to expect that by taking W„ as the starting point instead, one should obtain a two-dimensional theory in which an infinite number of additional fields are coupled to Polyakov gravity. It may be that this theory would admit of a more elegant three-dimensional interpretation. In fact this raises the general question of whether W^ might more appropriately be thought of as a symmetry algebra for a (2 + l)-dimensional theory rather than a (1 + l)-dimensional one. So far all our discussion has been concerned with algebras of purely bosonic symmetries. It is natural to enquire whether supersymmetric extensions of W„ can exist. We have as yet been unable to construct such an extension, although for the contracted algebra w„ they certainly exist [17]. One might perhaps have expected to encounter some difficulties here, since already at the level of WN algebras for finite N there are qualitative differences between the bosonic and supersymmetric cases. In particular, whereas for the bosonic cases the central charge parameter can take arbitrary values, it is known for the W5/2 super-algebra that only one specific value (namely, c = - jf ) is possible [1]. This sort of restriction appears rather unnatural in an approach such as ours, in which the conditions upon the central terms tend to be insensitive to a simultaneous overall scaling, as in eq. (2.6). It would be interesting to study in more detail the family of Lie algebras Wj/i), obtained in subsect. 3.3 by extending the S1X2, U) operator algebras ^~(fi) beyond the wedge. As we discussed earlier, for generic values of n this algebra requires the introduction of further generators with all negative conformal spins, in addi tion to the familiar positive-spin generators of the W. algebra. If it turns out that the class of Wj/x) algebras could be implemented as symmetries of (2 + 1)dimensional theories, one might find that the inclusion of fields with negative conformal spin (from a two-dimensional viewpoint) is actually desirable. The process of extending the SL(2, U) operator algebras beyond the wedge raises another interesting question. As described in subsect. 3.1, an operator algebra y~(/j.) is constructed from the enveloping algebra of SL(2, R) by (roughly speaking) setting the Casimir operator of SIX2,R) to the specific value fi. It would appear natural to attempt an analogous construction of LSA(/i) (or Wj/i)) outside the wedge, starting with the enveloping algebra for the full Virasoro algebra. However, it is not clear to us how this might work, especially for a generic WJ/x) requiring negative-spin fields. In ref. [2] a free-field construction of WN is given, in which the higher-spin fields are realised (through a Miura transformation) as normally ordered polynomials in the elementary currents. It might appear that this construction should be related to the algebra of SL(2, R) tensors and its extension outside the wedge to the LS product structure (as discussed in sect. 4), but upon closer examination it becomes evident that any such connection would have to be rather indirect. For example,
604
C.N. Pope et al. / Racah-Wigner algebra
217
in the WN construction, the normal-ordered product of two conformal-spin-2 generators yields a conformal-spin-4 generator, whereas in the corresponding multiplication within the SL(2, R) wedge algebra, the product of two SL(2, R)-spin-l generators gives rise to SLX2, R)-spin-2 generators, associated beyond the wedge with conformal-spin 3. Evidently the notions of conformal and SL(2, U) spin are very different. The general issue of how to interpret the LS product structure within the context of conformal field theory remains quite mysterious to us. For example, it remains an open question whether an associative LS multiplication can be defined whose antisymmetric component includes the central terms expected in a commu tator of conformal fields. The new perspectives presented herein have only begun to be investigated, and we may yet have a lot to learn about how to deal with W„, and related algebraic structures. We are grateful to R. Gustafson for several discussions, and for bringing refs. [9,10] to our attention. We are also indebted to C.J. Isham for extensive discus sions relating to the material in sect. 5. At numerous points throughout our work we benefitted from use of the algebraic-computing program MATHEMATICA [21]. One of the authors (L.J.R.) would like to thank the other authors and the Center for Theoretical Physics at Texas A&M University for their Texas-style hospitality during the course of this work.
Appendix A In this appendix we collect a number of mathematical definitions and results, most of which are standard in the relevant specialized field, but may not be familiar to the general reader. Throughout this section, n denotes a general non-negative integer, unless stated otherwise. The rising and falling Pochhammer symbols (also known as rising and falling factorials) are defined by (a) n = a{a + 1) ... {a + n - 1) = (a + n - 1) !/(a - 1)!,
(A.la)
[a]H = a(a-l)...(a-n
(A.lb)
+ l)=a\/(a-n)\,
respectively, with (a) 0 = [a] 0 = 1. It is easy to see that they are related by [a]n = (a -n + 1)„ = ( - l ) " ( - a ) „ , and that both are polynomials in a of degree n. Analytic continuation in n may be effected through the expressions involving factorials.
605
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C.N. Pope et al. / Racah-Wigner algebra
It is convenient to introduce the notation ,/
,
A{a c)
^
,
Aa+b-c)\{b 3
1/
+ c-a)\{c
+ a-b)\
(a + b + c + iy.
•
(A 2)
-
This particular combination of factorials arises quite often in the theory of angular momentum. The generalised hypergeometric function mFn(z), with m upper arguments a,, n lower arguments 6, and variable z, is defined as the series
F bu...,bn
y
'
(gl)jt(«2)f-(Ofc
^_
( A 2
{
h(^)k(b2)k...(bn)k'k\'
,
■)
generalising the standard hypergeometric function 2F, of Gauss. This expression is manifestly symmetric under separate permutations of the upper arguments and the lower arguments. The series terminates if any of the upper arguments is a negative integer or zero. If a numerator and a denominator argument coincide, their contributions to each term of the series cancel, leaving an m.lFn_l series. The functions mFn have received a great deal of attention by mathematical analysts; our basic guide to this body of work (and general reference for quoted results involving the mFn) has been the book by Slater [22]. We give here some standard definitions and results which we have found useful. The series (A.3) is called "saalschiitzian" if
I>,- = 1 + Efl,-
(A.4)
A series of type m + 1Fm is "well-poised" if there is a permutation of the upper arguments such that l+a1=bl+a2
= b2 + a3= ...=bm+am
+ l.
(A.5)
If this equality is violated by only one of the (m + 1) expressions, the series is "nearly poised." After a permutation of the arguments, the unequal expression can then be taken to be either the first one (1 + a,) or the last one (bm + am + l); one then speaks of a nearly poised series of the first kind or the second kind, respectively. These definitions may appear rather arbitrary at first, but are amply justified by the existence of numerous theorems involving series satisfying conditions of these types [22]. For example, Saalschiitz's theorem gives the sum of a terminating
606
C.N. Pope et al. / Racah-Wigneralgebra
219
saalschiitzian -iF2(l) series in closed form: a b
F \
>>
3 2
{c,l+a
~n
•1
+ b-c-n'
=
.
(c-a)n(c-b)n (c)n(c-a-b)n
(A.6)
As we saw in sect. 2, this identity allows one to simplify the commutator of a Virasoro generator with an arbitrary generator in W„. A useful transformation of terminating 3F2(1) series is
3F2
a,b, —n ;i c,d
(d-a)n (d)n
3^2
a,c — b, — n . ;i c,l +a -d — n
(A.7)
Identity (A.7) allows us to transform the expressions N£(m, n) appearing in our structure constants into Clebsch-Gordan coefficients, as described in sect. 2. Note that Saalschutz's theorem (A.6) is easily obtained as a special case of eq. (A.7), using the fact that (1 - x - n)n = ( - 1)"(JC)„ and recalling the celebrated theorem of Gauss evaluating the general 2 ^i(D :
2^1
[..»„]_ r(c)r(c-a-b) r(c-a)r(c-b)
(A.8)
Dixon's theorem evaluates the general well-poised 3F2(1) series: p\ 3' 2
2a,b,c + 2a-b,l + 2a-c'
a\(2a -b)\(2a
i l Jl - „.A.,_ ",. (2o)!(a -b)\(a
-c)\(a
-b
IL -c)!(2a
-c)\
\.-bL - c ) !
(A.9)
In subsect. 3.2, we also require the following summation formula which holds for a terminating, nearly poised 3F2(1) series of the first kind: F \ 3 2
-2a, -b-a,-c-a .A [ b-a + 2,c-a + 2 ' l\ ( - l)"(2a) !(b - a + 1) !(c - a + 1) !(a + b + c + 1)! , alblc\(b + c + l)\(a+b + l)(a+c + l)
(A.10)
where a, b and c are non-negative integers. We have arrived at this result, as well as at eq. (A.7), by algebraic-computing techniques; we have not encountered either of them in the literature.
607
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C.N. Pope et al. / Racah-Wigneralgebra
There are several further results which we have found of some use. A general 3 7 2 (l) series may be transformed into another one: r
3r2
a,b,c d,e
rje)r(s)
;i
r(e-a)r(s
+ a) 3 * 2
a,d — b,d — c . 1 , d,s + a '
where ssd + e - a -b -c. A terminating saalschiitzian transformed into another one:
4^3
(e-a)n{f-a),
a,b,c, —n ;i d,e,f
(e)n(f)n
4 F 3 (1)
(A.ll)
series may be
a,d - b,d - c, - n
provided that d + e +f=a + b + c — n + 1. By reversing the order of summation, any terminating generalised hypergeometric series can be straightforwardly transformed into another. The form of this transformation relevant for our purposes reads al,...,am,-n
= (-1)
m+1 m
* m + 1 *»
1 -bx-n,...,\ -bm-n, - n . (A.13) 1 -a,-/i,...,l -am-n ; i
The representation of a 6-y symbol in terms of a terminating saalschiitzian 4F3(l) series is discussed in ref. [10]; the basic result, appearing as eq. (5.11.4) there, reads la \d ld
b
c
c
( - ! ) * ' ( j 3 , + l)\A(a,b,e)A(c,d,e)A(a,c,f) A{b,d,f) e\_ /fj/ " ( / 3 2 - ^ 1 ) ! ( / 3 3 - / 3 1 ) ! ( / 3 l - a 1 ) ! 0 1 - a 2 ) ! ( ^ 1 - a 3 ) ! ( ^ 1 - a 4 ) ! «i
_
/3,, a 2 - /315 a 3 - /3,, a 4 - /3[
x 4 F 3 -p -l,P -p l 2 i
+ l,fi3-pi
+l
;i
(A.14)
where the parameters (/3,,/32,/33) are identified with a permutation of the threetuple (a+b
+ c + d,a +d + e +f,b + c + e + / )
with /3, assigned to the minimum of the three (other choices being related by analytic continuation), and (0^02,01^,04) taken to be any permutation of the
608
C.N. Pope et al. / Racah-Wigneralgebra
221
four-tuple (a+b
+ e,c + d + e,a + c+f,b
+
d+f).
The representation of the Clebsch-Gordan coefficients in terms of terminating 3^2(1) series is also discussed in ref. [10]; up to analytic continuation, one has
m)\(j-n)\(k+p)\(k-p)\]l/2A(i,j,k)
[(2k + l)(i +
X3^2
—i - n, +m k 1 ++k m, — i-j- n, 1 +- ki -j—j +
(A.15)
Here, of course, n is a standard angular-momentum label, not assumed to be a nonnegative integer.
References [1] A.B. Zamolodchikov, Theor. Mat. Fiz. 65 (1985) 347 [2] V.A. Fateev and S. Lykyanov, Int. J. Mod. Phys. A3 (1988) 507 [3] A. Bilal and J.-L. Gervais, Phys. Lett. B206 (1988) 412 [4] F. Bais, P. Bouwknegt, M. Surridge and K. Schoutens, Nucl. Phys. B304 (1988) 348, 371 [5] A. Bilal, Phys. Lett. B227 (1989) 406 [6] I. Bakas, Phys. Lett. B228 (1989) 57 [7] C.N. Pope, L.J. Romans and X. Shen, Phys. Lett. B236 (1990) 173 [8] E.S. Fradkin and M.A. Vasiliev, Ann. Phys. (N.Y.) 177 (1987) 63 [9] L.C. Biedenharn and J.D. Louck, Angular momentum in quantum physics (Addison-Wesley, Reading, MA, 1981) [10] L.C. Biedenharn and J.D. Louck, The Racah-Wigner algebra in quantum theory (Addison-Wes ley, New York, MA, 1981) [11] J. Reynal, J. Math. Phys. 20 (1979) 2398 [12] V.G. Kac, Infinite dimensional Lie algebras (Cambridge University Press, Cambridge, 1985) [13] L.C. Biedenharn and J.D. Louck, Ann. Phys. (N.Y.) 63 (1971) 459 [14] E. Bergshoeff, M.P. Blencowe and K.S. Stelle, Area-preserving diffeomorphisms and higher-spin theories, Imperial preprint TH/88-89/9 [15] J. Hoppe, MIT Ph.D. Thesis (1982) [16] G. Moore and N. Seiberg, Commun. Math. Phys. 123 (1989) 177 [17] C.N. Pope and X. Shen, Higher-spin theories, w„ algebras and their superextensions, Phys. Lett. B236 (1990) 21 [18] J.E. Moyal, Proc. Cambridge Philos. Soc. 45 (1949) 99 [19] D. Friedan, Z. Qiu and S. Shenker, Phys. Lett. B151 (1985) 37 [20] A. Alekseev and S. Shatashvili, Nucl. Phys. B323 (1989) 719 [21] S. Wolfram, Mathematica (Addison-Wesley, Reading, MA, 1988) [22] L.J. Slater, Generalized hypergeometric functions (Cambridge Univ. Press, Cambridge, 1966)
609
Reprinted with permission from Physics Letters B Vol. 242, No. 3,4, pp. 401^06,14 June 1990 © 1990 Hsevier Science Publishers B. V. (North-Holland) A NEW HIGHER-SPIN ALGEBRA AND THE LONE-STAR PRODUCT C.N. POPE*,L.J. ROMANS"' andX. SHEN■ ■ Center for Theoretical Physics. Texas AiM University. College Station. TX 7784S-4242. USA " Department of Physics. University of Southern California. Los Angeles. CA 90039-0484, USA Received 31 December 1989
In two recent papers, we constructed a new N-oa limit of the If* algebras, which we denote Wx having generators of conformal spins 2, 3 with central terms for all spins. In this paper, we construct another new algebra, which we denote H^l+0o, with generators of conformal spins, 1,2,3 again with central terms for all spins. The requirement that the algebras be closed requires that one include the spin-1 generators in W,+m and prohibits their inclusion in Wx. Paralleling our analogous construction for Jfoo, we show that the new algebra can also be realised as the antisymmetric part of an associative "lone-star" product, which also closes on the set of generators with conformal spins * I.
The recent discovery [ 1 ] of a W„ algebra with central terms for all integer conformal spin > 2 has uncovered an exciting new landscape of infinite-di mensional algebraic structures. The process of eluci dating the underlying framework of the W„ algebra (2] has suggested various directions for further de velopments. Included in these are, for example, the inclusion of fermionic generators to form a super- W^ algebra; the study of the representation theory of the algebras; and the construction of field-theoretic models that realise this symmetry. Solving these problems will help achieve the classification of all conformal field theories. Another issue that naturally arises in tackling these problems is the question of whether one can include conformal-spin-1 genera tors in the algebra, just as one may adjoin Kac-Moody generators to the usual Virasoro generators to form an extended algebra involving spins one and two. This may facilitate the construction of the higher-spin al gebras in terms of conformal-spin-1 currents in a manner analogous to the construction for the WN al gebras for finite N (3). Furthermore, spin-1 genera tors are known to play a crucial role in the superconformal algebras with extended supersymmetry.
1
Supported in part by the US Department of Energy, under grant DE-FG03-84ER40I68.
Specifically they induce the rotations amongst the su persymmetry generators. The W„, algebra constructed in ref. [1,2] cannot be augmented to include conformal-spin-1 genera tors. To be more precise, if one includes spin-1 gen erators in the algebra, one is then forced by the re quirement of closure to add further generators with all conformal spins sj 0, which presumably does not make sense in the context of two-dimensional con formal field theory. In this paper, we construct a new algebra, which we denote W, +00 , in which the inclu sion of conformal-spin-1 generators is not only pos sible, but required in order to satisfy the Jacobi iden tities. The W,+0O algebra contains generators of conformal spins & 1 with central terms for all spins. Both W^ and Wi+oo can be viewed as extensions of the SL(2, R) tensor algebras z(n), where the pa rameter n is the value of the quadratic Casimir Q of SL(2, R). As discussed in ref. [2], the generators of these tensor algebras may be associated with modes V'„ of conformal fields, restricted to the "wedge" |m| < ( / + l ) . We showed in ref. [2] how the algebra r(/i) for general n could be extended "beyond the wedge" to an algebra W„{ji), in general requiring the addition of fields of negative conformal spin. Owing to the presence of non-trivial zeros among the struc ture constants for the n=0 algebra, the particular ex tension W^OJcan be consistently truncated to a 401
610
closed algebra containing only those generators with conformal spins > 2. This is the algebra W^, con structed in ref. [ 1 ]. The W\+^ algebra is the analo gous truncation of the extension W„( - 1 ) of T( - j) beyond the wedge when//= - J. In this case, the con sistent truncation retains all generators with confor mal spins > I. In ref. [2], we showed that the algebras W„(n) could be realised as the antisymmetric part of an un derlying associative product, which we denote with a lone star *. As we shall discuss presently, the lonestar product also givesriseto a closed algebra for gen erators of conformal spins 5 1 at the special value ft= - \. This product is reminiscent of the fusion rules characteristic of rational conformal field theories [ 4 ]. The algebras that we shall be considering all take the general form
=gUm, n;n) VZi„ + q2g'{{m, n\u) V'+iS q'gUm,n;»)V+l-t+...
+ 2
+q 'gUm,n;fi)V*ii,1'
+ ...
2
+ ? 'c1(m;/i)<5«rf„+,.o.
(1)
the ipt.in) can be expressed as
where the right-hand side is a Saalschiltzian «/"3(l) generalised hypergeometric function [ 2 ]. (Note that this is invariant under the involution *-»—*-1, as required for function of/;.) For generic values of/;, the sequence of terms on theright-handside of (1) will continue indefinitely, so that generators of all conformal spins from - oo to + oo are present in the algebra. When ft=0, the struc ture constants g<j, (m, n; ft) turn out to be zero when ever i+j-2r is less than zero. This has the effect of terminating the sequence of terms at conformal spin 2, givingriseto the fP«, algebra that we described ear lier. Some of the zeros of gi,(m, n; 0) occur because of "obvious" zeros of N'j,(m, n), whilst the remain der occur because of non-trivial zeros of #J,(0). As discussed in ref. [ 2 ], the functions $
The generators V'„ correspond to the mth Fourier mode of a conformal spin(/+2) field; g'i,(m, n; n) are the structure constants; c,(m;n) are the central terms and q is a parameter. The structure constants are given by [2]
gUm,n;n)=^^NUm,n),
(2)
where the N'i,(m, n) are given by
X [ / + l - m ] 4 f j + l + n]»[y+l-B]j, + 1 _ t >
(3)
and the
(4)
c,(m; O ) s ( m - i - l ) ( m - / ) . . . X(m+/)(m+(+l)c,(0),
(6)
where the charges c,(0) are given by [2) c,(0) =
2*- 3 i!(i + 2)! ( 2 I + 1 ) ! ! ( 2 I + 3)!!<
(7)
and c is an arbitrary constant. For general values of ft, the algebra (1) without central terms still makes formal sense, provided that one includes generators of all negative conformal spins. However, one might expect that there would be difficulties in adding a central extension to the algebra for generic ft; for ex ample, it is not clear that (6) admits a sensible con tinuation for / < - 1 . In fact, one can easily see by examining some spe cific Jacobi identities that the central charges for neg ative spins must all be zero. For example, the Jacobi identity [ V\ [ V, Vk] ] + cyclic=0, with i=nj=0 and k= -n, n>0, establishes a relation between c0
611 and f -1. for n » 1. Together with the relations that one can derive amongst the c, with i positive, this shows that the c.n must be non-zero if the c, are non-zero. On the other hand, taking i = - 2n,j= - n, k= - n, or i3s-2n-\J=-n, k= -n, again with n>0, estab lishes that c _„ must be zero for n? 2. Thus if genera tors with conformal spins ^0 are present in the al gebra, all the central terms must be zero. It follows that if the algebra W„(ji) is to admit central terms, it must be the case that the structure constants (2) possess zeros, by virtue of the functions <M,(n) and tl],(m,n) having zeros, such that all generators with conformal spins < 0 may be consistently truncated from the algebra. We observed in ref. [2] that there is another spe cial value of the parameter fi (besides p=0) for which tbe functions^, (//) have many zeros, namely for the case/i=-l. In fact it turns out that $'{,(-J) has ze ros at almost all the same values of /, j and Ir as does 4'{,(0). The only zeros of the latter that do not occur in the former are when /' +j—2r is equal to - 1 . Thus one can see by examining (1) and (2) that when jjs - 1 , the sequence of terms on the right-hand side will terminate with V -1 „. We therefore obtain a new closed algebra of generators with positive conformal spin, corresponding to W ^ f - D - Since generators with all conformal spins > 1 are present here, we de note this algebra Wx+0O, in contrast to the algebra W^ that has generators with conformal spins > 2. By examining the contributions of the central terms of the Jacobi identities for the algebra (1) with li= - J, we find that the m-dependence of c,(m; - J) is the same as in (6), i.e. c,(m;-i)a(ffi-i-l)(m-i)... X(m+i)(m + ; + l ) c 1 ( - l ) -
(8)
The values of the central charges c,( - J) may be ef ficiently fixed by looking at the central-term contri bution to the Jacobi identity involving KJ,, V'n and y'-m-n- From this, one finds the recursion relation c,*A-\) c,(-J)
4Q + 2)' (2/ + 3)(2, + 5 ) '
22i-2\(i+lY\2
Symplecton«-»5= - J,
Sdiff(//)~j=oo. K
whence we derive the general result
^-> )= (L.^'IJ)!! C -
where c is an arbitrary constant. Since (10) reduces to c0=-hc >n 'he Virasoro sector, the constant c may be identified as the usual central charge. At this stage, it is perhaps worth summarising what is known about the algebras that arise for special val ues of the parameter /i. In ref. [ 2 ], we discussed the "wedge" algebras J[fi) of SL(2, R) tensor operators T'm, where 8 is the SL(2, R) spin, - x < m < { , and/i is the value of the quadratic SL(2, R) Casimir oper ator Q. The operators 7"i, are the three SL(2, R) gen erators themselves, while the higher operators are built up from higher powers of the SL(2, R) genera tors, modded out by the ideal generated by ( 2 - / 0 [21We noted in ref. [ 2 ] that when n = - & the algebra J[fi) is the "symplecton" algebra of Biedenharn and Louck [ 5 ]. This has also arisen more recently in the context of the higher-spin algebras of Fradkin and Vasiliev [6,7]. Another special case of &[n) arises when fi=oo. This algebra is isomorphic to the algebra of area-preserving diffeomorphisms Sdiff(H) of a two-dimensional hyperboloid H [8,7,2]. To our knowledge, ref. [2] contains the first explicit closedform expression for the structure constants for this case. When the parameter /i is equal to zero, we showed in ref. [2] that the algebra &[/i) could be extended "beyond the wedge," to the algebra W„ where one makes the association V'„~T'£' and now allows the index m to range over - o o < m < o o for each t>0. Now, in this paper, we have shown how to construct another algebra, Witab, by extending &{-{) "be yond the wedge." In this case i> - 1 , and again -oo<m
(l0)
(11)
Note that Wi+a> corresponds to the "symmetric point" of eq. (4); the value 5= — s-\ = - j is the one that minimises the value n of the SL(2, R) Casimir operator. For general values of s, we may, without loss of generality, assume that s> - j . When s= - J, cor403
612
responding to the symplecton algebra, one can see from eq. ($) that all the functions
(12)
m
The results presented there generalise in a straight forward manner to our new algebra W^oo- Rather than presenting the general case, we refer the reader to ref. 12], and instead here we give some example operator-product expansions. For convenience, we shall refer to the spin-1 field V~'(z) as;'(z), with modesy„= V-'. The current-current operator prod uct reads
404
^W-TeSS) 3 -
(13)
Thespin-2fieldV°(z) is simply the energy-momen tum tensor 7"(z), with OPE given by ^)7"(w)~2U^p
Hu^ + r ^ H -
(U)
The OPE
^ w w - f e ^ + rb*-)'*"0
(l5)
is the statement that j(z) is a primary spin-1 field. The OPE between the spin-2 and spin-3 fields
+ r 7 ^- ri y
(16)
3(z-H>)
however, shows that the spin-3 field V2(z) is not a primaryfield,owing to the presence of the extra term involvingy'(z) on the right-hand side. This is a prop erty of all thefieldsof spin > 3. Just as in the case of the WN algebras discussed in ref. [ 3 ], it is convenient to work withfieldsthat do not, in general, have defi nite conformal spin. However, for the sake of brevity we usually speak of thefieldK'(z) as having confor mal spin (< + 2), it being understood that this refers to its leading-order behaviour in the OPE with T(a). In ref. [2], we also showed that the Lie bracket in the algebra (1) for the case c=0 can be realised as the antisymmetric component of a suitably defined multiplication law for the generators, which we de note by a lone star *. Thus [V'm,V>n] = Vlm*V'„-V'„*V'm-
(17)
One can regard the lone-star product of generators as a more fundamental concept than the antisymmetric part (17). The * product of generators forms an as sociative algebra, which we call LSA (p), which takes the form [2]
613
V„*y* = l I am-
Q'gUm,n;H)V£r.'.
(18)
I
where the summation runs over both even and odd values of a in the stated range. The functions g'i(m, Kfi) with a odd are defined by (2)-(5), with r re placed by \a. As in the commutator algebra W^, it turns out that the zeros of g'i(m, n\ ft) at n=0 are ,uch that LSA(0) closes on the set of generators with />0 (2). For generic values of fi, one must include an infinite number of generators with negative conformal spins too. If we now examine the algebra LSA(/0 for^= - J , we find that as in the commutator algebra IV,+0O, the lone-star algebra closes on the set of generators with i> - 1 . In other words the structure constants g'l {m, n; - J) have zeros both for even and odd a such that the infinite sequences of terms on the right-hand side 0 f (18) terminates with V^\.„-jm^n. Some exam ples of the lone-star product of generators in LSA(-})are
+£q{6m2-3mn
yX
"*L'= j-qy~+* +
/„*£„= j-Lm+„ + {mjm+n, *""*A==4o L"*'-\n)-+"-
(20a) <20b)
Note that, as pointed out in ref. [2), the operator Aqj0 plays the role of the identity element in the * algebra. Further examples of * products, which can be con trasted with the corresponding ones for LSA (0) given in section 4 of ref. [2J, are the product of two Vira soro generators
+ \q(m2-mn
(22a) + H»>-2>>)V'~.+.
2
fiq(m -3mn+6n2-4)L„.n
-j«2(»J-nW»+».
(22b)
The * product of three Virasoro generators may be computed from (20)-(22) to be Lm*L„*Lp= -^-j K;L+„+(,+ — ( m - p ) K ^ + „ , + ^(im2-2n2
+ ip2 +
mn-9mp+np-l)
X *—m + n + p
+ {q[2m, + m2(n-p)-m(n2
+ 2) (23)
(19)
for two spin-1 modes, while for a spin-1 mode and a Virasoro generator
Lm*L,,= ±V!...
n2-4)Lm+„
+ W(m>-m)jm.„,
-(m"p)\jm+ntp. J-*J"= 4qjm+"
+
+
Hm-n)L„„
+ n2-l)j„+„,
(21)
Verifying the associativity property for even this sim ple example of a triple product is not completely trivial. In this paper, we have presented a new higher-spin algebra, W^^, containing generators with all conformal spins > 1, and show how it may be realised as the antisymmetric part of an associative product al gebra. Together with the algebra W, for generators of all conformal spins > 2 that we obtained previ ously, this new algebra exhausts the possibilities for constructing positive-conformal-spin algebras as ex tensions beyond the wedge of SL(2, R) tensor-oper ator algebras. This may be seen from eq. (3.24a) of ref. [ 2 ], in which it is evident that for any value n of the SL(2, R) Casimir besides 0 or - J, the commu tator of two Virasoro generators in W„(/i) contains a component with spin formally equal to - 4 . It would be nice to have a more direct understanding of why these particular values of the SL(2, R) Casimir are singled out.
and products of Virasoro generators and spin-3 modes
405
614
References [ l ] C . N . Pope, L.J. Romans and X. Shen. Phys. Lett. B 136 (1990)173. [2) C.N. Pope. U Romans and X. Shen. Wm and the RacahWigner algebra, preprint CTP TAMU-72/89, USC-89/ HEP040. [3) A.B. Zamotodchikov, Teor. Mat. Fiz. 65 (1985) 347; V.A. Fateev and S. Lykyanov, Intern. J. Mod. Phys. A3 (1988)507. [4) G. Moore and N. Seiberg, Commun. Math. Phys. 123(1989) 177.
406
(5) L.C. Biedenham and J.D. Louck, Angular momentum in quantum physics (Addison-Wesley, Reading MA, 1981); The Racah-Wigner algebra in quantum theory (AddisonWesley. Reading. MA, 1981). [6] E.S. Fradkin and M.A. Vasiliev, Ann. Phys. 177 (1987) 63. [ 7 j E BerfthoetT, M.P. Blencowe and K.S. Stdte, Area-preaervia| difTeomorphisms and higher-spin theories, Imperial preprint TH/88-89/9. (8] J. Hoppe, MIT Ph.D. Thesis (1982).
615
Reprinted with permission from International Journal of Modem Physics A Vol. 7, Suppl. 1A, pp. 55-81,1992 Proceedings of the RIMS Research Project 1991, "Infinite Analysis" © 1992 World Scientific Publishing Company
B E Y O N D THE LARGE N LIMIT: NON-LINEAR Woo AS SYMMETRY OF THE SL(2,R)/U(1) COSET MODEL*
IOANNIS BAKAS+ Center for Theoretical Physics Department of Physics and Astronomy, University of Maryland College Park, MD ZOUZ, USA
and ELIAS KIRITSIst Department of Physics, University of California and Theoretical Physics Group, Lawrence Berkleley Laboratory Berkeley, CA 947S0, USA
Received
September 24,1991
ABSTRACT We show that the symmetry algebra of the SL(£,R)h/ U(l) coset model is a non-linear deformation of W^, characterized by k. This is a universal W-algebra which linearizes in the large k limit and truncates to WN for k =—N. Using the theory of non-compact parafennioos we construct a free field realization of the non-linear W„ in terms of two bosons with background charge. The (^characters of all unitary SL(S,R)/U(1) repre sentations are computed. Applications to the physics of 2-d black hole backgrounds are also discussed and connections with the KP approach to c=l string theory are outlined. Keywords: Conformal Field Theory, W algebras.
1. Introduction There has been considerable interest in the construction of a universal W-algebra which unifies all types of extended conformal symmetries in 2-d quantum field the*This work was supported in part by the Director, Office of Energy Research, Office of High Energy and Nuclear Physics, Division of High Energy Physics of the U.S. Department of Energy under Contract DE- ACO3-76SFO0096 and in part by the National Science Foundation under grants PHY-85-15857 and PHY-87-17155. + Address after September 16, 1991: School of Natural Sciences, Institute for Advanced Study, Princeton, NJ 08540, USA. T Address after October 1, 1991: Lab. de Physique Theorique, Ecole Normale Superieure, 24 rue Lhomond, F-7S231, Paris, CEDEX 05, FRANCE.
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/. Baku & E.
KiriUit
ory. The existence of such master symmetry could be advantageous for developing a non-perturbative formulation of string theory and exploring its vacuum structure. Originally it was thought that the large N limit of Zamolodchikov's Ws algebras,1,2 interesting as it may be in its own right, plays a prominent role in this direction. However, since W^ is a linear algebra,3,4,8 it is very difficult to invent a mechanism which effectively truncates the spin content of Woo to a finite set 2,3, • • •, N and produces the non-linear features of WN algebras for N > 3. To put it differently, since W)v is not a subalgebra of Ww for N < N' (unless N = 2), the large N limit is not defined inductively. In this paper we show that the resolution to this problem lies beyond the large TV limit! The method we employ here is based on the standard relation be tween W-algebras and parafermions. Recall that the ZN parafermion coset models SU(2)N/U{\) have a Wjv symmetry and central charge,6 cN = ——--1=2——-. (1.1) v N+ 2 N +2 ' For large values of TV, CN approaches 2 from below and the underlying Wp/ algebra linearizes in the limit N —* oo. 5 One way to penetrate the c = 2 barrier and go beyond the large N limit of SU(2) parafermionic models is to consider the noncompact coset models SL(2, R)k/U(\),7,6 whose central charge is
* - & — *&:
™
Then, it is natural to expect that the W-algebra of the SL(2, R)k/U(l) coset models reduces to the WN algebra of SU(2)N/U(1) for k = -N. The idea to make the transition from the compact to the non-compact models is motivated by well known results in the representation theory of the N = 2 superconformal algebra. In this case, for central charge c < 3, there exists only a discrete series of unitary representations with c = 3N/(N + 2), for all non-negative integers N.9 These can be obtained from representations of the SU(2)N current algebra by subtracting and then adding back a free boson (alternatively stated by changing the radius of the torus boson).10 For representations with c > 3, the SU(2) parafermion method is not adequate and further generalization is required. Lykken introduced a new type of parafermion algebra for c > 3, 1 1 which corresponds to SL(2, R) and contains an infinite number of parafermions, unlike the compact case. It was subsequently shown that all unitary N = 2 superconformal representations with 3 < c = 2k/(k — 2) can be obtained from representations of the SL(2, R)k current algebra by the same method of appropriately subtracting and then adding back a free boson.7 Our main result is the construction of the W-symmetry of the SL(2, R)k/U(l) coset model. As we will demonstrate later, this is an extended conformal algebra which for generic real values of k has an infinite number of generators with integer spin 2,3, • • •. Although the spectrum of generators is identical to that of the Woo
617
Beyond the Large N Limit
57
algebra, in this case there are non-linear terms which depend explicitly on k and cannot be absorbed into field redefinitions. We will denote the W-algebra of the 5L(2, R)k/U(l) coset model by Woo(ib) and note that the non-linearities disappear in the limit k —* ±00, where the ordinary Woo algebra is recovered. Also, for all integer values of k — —N < —2, it turns out that Woo(fc) truncates to the finitely generated Ws algebras. In this sense, the non-linear deformation of W^ we construct here is a universal W-algebra for the .A-series of extended conformal symmetries. Similarly, one may consider higher rank non-compact coset spaces and obtain further generalizations of our results. We will comment on this possibility at the end. The W-symmetry of the SL(2, R)k/U(\) model (and its parafermionic exten sions that we will also consider for rational values of k) are also important for study ing properties of the conformal field theory governing the 2-d black hole solution to string theory discovered by Witten, 12 (see also Ref. 13). In this case k = 9/4 (c = 26) and the Woo(k) symmetry is non-linear. However, since the number of its generators is infinite, the 2-d black hole background carries an infinite number of independent quantum numbers, one for each W-generator. We will propose a recursive method for their construction. Another problem related to the recent developments in non-perturbative 2-d quantum gravity, 14 is the connection (if any) between Woo(fc) (for k = 9/4) and the underlying Wi + 0 0 symmetry in c = 1 string theory. 15 It has been demonstrated recently that the bi-Hamiltonian structure of the full KP hierarchy can be described in W terms as follows: Wi + 0 0 , 1 6 provides the first Hamiltonian structure, 1 7 1 8 while the second one is a non-linear deformation of Woo , 19,20 (in both cases the central charge is zero). It is reasonable to expect that Woo(ik) is a quantum version of the second Hamiltonian structure of the KP hierarchy. From the point of view of the KP approach to the theory of multi-matrix models,21 the relation between the 2-d black hole solution and the c = 1 matrix model could be elucidated and lead to a deeper understanding of these string models. We will present some thoughts in this direction later. The material in this paper is organized as follows. In section 2 we review the basics of parafermion algebras with emphasis on the SL(2, R) case and motivate the introduction of Woo(Jk) • In section 3 we adopt the free field realization of 51,(2, R)k current algebra and obtain expressions for the generators of Woo(k) in terms of two bosons with background charge. We also present the results of some explicit calculations for the commutation relations of Woo(fc) , which are sufficient to demonstrate the universal features of the algebra. In section 4 we derive the character formulae for all unitary highest weight representations. In section 5 we discuss the implications of our results to the theory of 2-d gravity and finally in section 6 we present our conclusions.
618
58
/. B*Ut & E. KiriUu
2. S L ( 2 , R ) / U ( 1 ) Parafermion Algebra Parafermion algebras are generated by a collection of currents ipi(z) and their conjugates ip]{z) = *l>-i(z) with V"o(*) = V"o(2) = 1- A. priori there are no restric tions on the range of / = 0,1,2, • • • and generically, the conformal dimension Aj of the parafermion currents is fractional. The algebra assumes the form, 11 l M * ) i M t i / ) = Cil,h(z-w)*>>+»-*<>-*»
M*)4>hw)
= (* -
U,
) " 2 A ' I1 + — (
z
[4nl+h{w) + 0{z-w)]t
(2.1a)
- *)2TA">) + 0((x - w)3)] ,
(2.16)
where T^, is the stress tensor of the parafermion theory with central charge c^,. The structure constants (?{,,<, are determined by associativity and the conformal dimensions At are constrained to satisfy the recursion relation Ai+i -I- Aj_i - 2A, - A 2 + 2Ai = n« , n t € Z$ .
(2.2)
Parafermions arise naturally in the context of N = 2 super conformal algebra. 10,11 Its generators, J(z), T(z) and G ± (z) can be constructed in terms of one scalar field
• T{z) = -\(dM*))2
G*(*) = y y e ^ v T ^ ^ W .
+ ?*(*) ,
(2.3a)
(2.36)
This realization determines c^ and Ai in terms of the central charge of the N = 2 superconformal algebra, c* = c - l
,
AX = 2 ( ^ L H
(2.4)
and the operator product expansion (OPE) of the / = 1 parafermions generates V>±2 with conformal dimension A, = «
.
(2.5)
It is clear that the spectrum of the parafermion algebra depends crucially on c. In particular, for c < 3, using the parametrization c = 3N/(N + 2), the recursion relations (2.2) (due to zeros in the OPE coefficients Cj,,ij) generate only a finite number of independent parafermion currents with dimensions ^ . f f i ^ f l . o s . s w - l N
(2.6)
619
Beyond ike Large N Limit
59
These correspond to the ordinary ZN parafermions of Fateev and Zamolodchikov,6 described by the coset model SU(^)N/U{\) , with central charge c^, given by Eq. (1.1). On the other hand, for c > 3, using the parametrization c = 3k/(k — 2), Lykken pointed out, 11 that the parafermion algebra does not truncate. In this case the parafermion currents form an infinite family of fields with dimensions Ai = ^ , l 6 ?
+ 0
.
(2.7)
For completeness we include the formulae for the structure constants Q, ,i, in both cases. For the ZN parafermions, r
'*•''
.[
r(AT-/ 1 + i)r(AT-./ a + i)r(/ 1 + /a + i)
1*
Lr(/i + i)r(/2 + i)r(^ + i)r(N-/ 1 -/ 2 + i)J '
{
while for the Lykken family, n
f r^ + ^ + hjrwrtii-rb + i) 1* r(/i + i)r(/3 + i)r(* + /i)r(* + h)\
(2.9)
We also have C-j,,/, = Ci,,»,_«, for h > h- Notice that Eqs. (2.6), (2.8) are analytic continuations of Eqs. (2.7), (2.9) respectively for k —* —N. The parafermion algebra (2.1) can be converted into a current algebra using an additional free scalar field x( z )> 6 m analogy with the N = 2 superconformal algebra. To do this, we define the currents J\z)
= -\[\dtX{z)
, J±(*) = V i b r ^ x M ^ * ) ,
(2.10)
which transform the parafermion algebra into the current algebra J*(z)J~(w)
= —±—-2^^+0(1), (z — w)* z—w
(2.11a)
J3(z) J±{w) = ± ^ M + 0 ( 1 ) , z—w
(2.116)
J3(z)J*(rv) = - T J ^ I + 0(1) .
(2.11c)
Here we consider the case of Lykken parafermions with c^, > 2 (i.e., k is any real number > 2). The symmetry of the non-compact parafermions is Z^. The OPEs (2.11) define an SL(2, R)k current algebra and the corresponding coset model is SL(2, R)it/U(l) with central charge c^, given by Eq. (1.2). If we had taken k = —N, we would have obtained the SU(2)N current algebra description of the ZN parafermions.6 The free field representation of ZN parafermions was derived in Ref. 22. The corresponding one for the non-compact case was given in Ref. 23.
620
60
/. £•*•« » E. KiriUis
It is well known that parafermion coset models have a W-symmetry whose gen erators appear on the right hand side of the OPE (2.1b). In particular, it is suf ficient to consider Vi(*)V'-i( w ) an< l g° beyond the most singular terms in order to extract the W-generators. In Eq. (2.1b) we have only displayed explicitly the stress tensor T^ which is the lowest spin field of the underlying W-algebra. For SU(2)N parafermion models the corresponding W-algebra is WTV, 1,2 generated by chiral fields with integer spin 2,3, • • •, N. For finite N > 3, the parafermion currents acquire fractional dimensions ~ \/N and the Wft algebra is non-linear. However, as N —► oo, the parafermions become mutually local fields with integer dimension Aj = 1,2, • • • and Woo linearizes.5 Then, by formally interchanging N to — Jfc in the large TV limit, we access the non-compact coset region which lies beyond the c = 2 barrier. For c > 2, the SL(2, R)k/U(l) model has the same number of parafermion currents as SU(2)oo/U(l) and makes sense for any real Jfc > 2. In order to understand qualitatively the main features of the SL(2,R)k/U(l) W-algebra, notice that although the number of parafermions is independent of Jfc, their conformal dimension A| = / + ^ acquires a non-integer contribution ~ 1/Jfc for finite Jfc. Therefore, it is natural to expect that the underlying W-algebra has the same spectrum of generators as Woo , but it develops non-linearities depending on Jfc. In the next section we construct the W-algebra of the SL(2,R)k/U(l) coset model, Woo(k) and demonstrate its universal features. In section 4 we show that the character of the Woo (Jfc) vacuum module (as well as the rest of the characters) for Jfc > 2 are independent of Jfc. This rigorously proves that the spectrum of the algebra is the same as that of the usual Woo ■ Thus, for any k > 2, the generators are chiral fields with integer spin 2,3, • • •, each with multiplicity one. 3. The Chiral Algebra
W^k)
We adopt the free field realization of the 5L(2, R)k current algebra, which rep resents the two parafermion currents ip±\(z) in Eq. ( 2.10) as, 2 2 , 2 3 rP±1(z) = - - L [ q F v T ^ c W z ) -(- tVife dz
,
(3.1)
using two free bosons with (4>i(z)*j M > = -Sij \og(z - w) .
(3.2)
It follows immediately from the OPE (2.1b) that the stress tensor of the theory is
W2(z) = T^z) = -\(dz
9
*Vi •
( 33 )
All other generators of Woo (Jfc) appear in the less singular terms of ipi(z)tp_l(w) and it is just a matter of computation to extract their form in terms of 4>\,4>2. We will present the results of the calculation up to spin 5, since for the higher
621
Bejoni
tke Large N Limit
61
spin generators the expressions become considerably more involved and we have no closed formulae for them in general. It should be stressed, however, that the OPEs of the W-algebra can be computed without the use of the free-field formulation, directly from the parafermion correlation functions. In several occasions we did the computations with both methods as an independent check. We define the primary higher spin generators Ws(z) of the algebra, using the bootstrap method, by the OPE*
+
h (? + 5*"*) "««>" i > «
- W^TT'' : * *
+0{e6)
:
«+
.
(3.4)
For the primary spin 3 field we obtain the expression W3(z) = a(d<j>2)3 + 0&
(3.5)
where 2i (3fc - 4) / 2 c
„.(A:-2)
.
i [2
Ik-2
6 = 21^-L^J-j-
n.(*-2)
„. Ik-2
, e = -2i}J —
[2 ,
•
x
(3.6)
Then, the OPE of W3 with itself yields W I, + , W f,* - 16(fc + l)(* + 2)(3fc-4)
16(fc + 2)(fc-2)(3fc-4) / 1
where ^ ( z ) is the primary spin 4 field which was defined implicitly in Eq. (3.4). Its explicit form is given in appendix A. Before we proceed further a remark is in order. The requirement that a spin 3 field of the form (3.5) is primary with respect to the stress tensor (3.3), imposes a
Norrnal ordered products of operators are defined, as usual, by subtracting the singular terms plus the finite terms that are total derivatives of lower dimension operators appearing in the corresponding OPE. In general, they are not symmetric.
622
62
/. BtUt & E. Kiriitit
three conditions on its numerical coefficients. Since the overall normalization is a matter of convention, one is left with one undetermined parameter. Then, if we consider the OPE Wa(z + e)Ws(z) and demand that the t~4 term is proportional to Wi(z), we obtain a quadratic equation for the ratio x = y/e. The two solutions are
x+ =
_^p2) ^ ^ = _ | ^ _ _
(3 g)
In our case the expression (3.6) corresponds to the first branch, which also gives rise to a non-zero primary field W4. For the second branch, the only quasiprimary operator that appears to order e~2 is : W% : and there is no primary spin 4 field present. In this case we are dealing with Zamolodchikov's W3 algebra in its free field realization in terms of two bosons.1 We return now to the Woo{k) algebra and perform the next OPE. We find „ , ,_ ,
A w
,_i _ 3 • 2 7 (* + 3)(2fc - l)(2fc - 3) / 1 l ^ . w / x
+
5(3* - 4 ) / l
Id,
Id2
2fi,\„,/x
39 • 2*(k - 2)(fc + 3)(2fc - l)(2k - 3) / 1 2 d.\ * 2 (16* - 17)(64* - 107) \t* + 5 1 ) ' 3^(k + 3)(2k-3)(k-2):(dW2)W3:(z) fc2(16Jb - 1 7 ) ~e +VW>
2
3
' K> Vy)
where W^z) is the spin 5 primary field computed directly from the expansion (3.4). Its explicit form is also given in appendix A. The expressions for : W$ :, : W2W3 : and : {dWzjWa : are given in appendix B. We may iterate the procedure above to obtain expressions for all higher spin fields of the algebra and compute their commutation relations. The strategy is obvious, but the derivation of the formulae for all the higher spin fields in closed form is a very difficult task. As far as the commutation relations of Woo(k) are concerned, one may compute its central terms (i.e., {W,(z)W,i(w))) directly from Eq. (3.4) by considering the parafermion four-point function
L*12*14*34223j
[*i2*34 \
+ (*2~*4) •
K*24*23/
(3.10)
The coefficients of all other terms that appear in the singular part of the OPE W,(z+i)WB>{z) can also be computed directly, using Eq. (3.4) and the parafermion six-point function (^IV'JVIV'I V'lV'IY A general property of Woo(k) is already obvious from (3.7), (3.9). The alge bra is invariant under the transformation Wt —♦ ( - l ) ' W , , where composite fields
623
Beyond tke Large N Limit
63
transform multiplicatively. This is a reflection of the rpi —* V»-i invariance of the parafermion algebra and corresponds to the Weyl reflection in SL(2, R). We note that the closure of the Woo(*) algebra is guaranteed by the closure of the charge zero sector of the enveloping algebra of the SL(2, R)k current algebra (c.f. the re alization (2.10) in terms of ^ I . V"i and the additional scalar field \)- It would be very interesting, though, to have the complete structure of Woo(*) m closed form. For all real values of k > 2, the Woo(fc) algebra is non-linear and has an infinite number of higher spin generators (one per spin). One might wonder that the algebra, although non-linear at first sight, might linearize by appropriate change of basis. This was the case with the standard Woo ■ For example, one might consider the field redefinition
which linearizes the singular part of the OPE (3.7) and still maintains the linearity of the W2W4 OPE. In order to verify that such field redefinition does not remove all the non-linearities from Woo(*) , it is sufficient to look at the OPE W4W4 and in particular to order e~4, where both W4 and : W 2 : terms appear. We find that
2io(t+ (t
" :ff t + - 3 ff" )(3t ' 4) -
w«+.ww. 1+
f^(
+
5*** + B^)^"
+
(k?W*-iiS
9* 2 (4ib 3 +15fc 2 -33ib + 4) <4W4(z) + 0(€ 5 ) 16(* + l)(Jfc -I- 2)(Jfc + 3)(2Jfe - 1)(3* - 4)
'■W' ■■W+ (3.12)
Then, if we compute W4W4, we find to order e 4 that the coefficients of W4 and : W 2 : do not combine to give only W\. It turns out that the remaining term is 160(fc - i)(fc - 2 ) 2 (* + 2)(3fc - 4) . 3Jk2(2Jk - 3X18*3 + lb2 - 117* + 116) '
2 2
_ ' K> '
(6
'
which establishes the non-linear nature of Woo(fc) • Next, we discuss properties of Woo(*) for some special values of k. (i) Recovering Wppi In the limit ifc —► 00, the W-symmetry of the SL{2, R)k /U(l) coset model is the standard Woo . since as we argued earlier the compact and non-compact parafermion algebras have a common limit. In both cases the algebra contracts to a £/(l) 3 current algebra6 by a suitable rescaling of its genera tors. Passing to the coset model, one effectively removes one of the U(l) currents 'In the SL(t,R)
case two of the »h»K»»i current* are non-compact.
624
64
1. B*kf
& E.
Kiriitu
and the resulting parafermion algebra is the enveloping algebra of the U{\)7 cur rent algebra.5 The first parafermion currents can be identified with the two C/(l) currents, which when written in terms of a free complex boson are
(314)
tfi(«) = W(z) , 4>U*) = ***(*) • All higher parafermions are composite operators, fh(z) =: tf : (z) , *l(*) =■■ ( r f ) k : W •
(3-15)
In the large ft limit, the free field realization of Woo (ft) in terms of two bosons with background charge should reproduce the results we have obtained for Woo with c = 2. 5 This can be readily verified using the identification fc(z) = ^ W ( z ) -I- d$(z))
, fc(z) = ^ g ( W * ) - d$(z)) ,
(3.16)
which yields W2(z) s Wt{z) = -d
(3.17)
at ft = oo. Similarly, Ws(z) becomes W3(z) = W3(z) = -2(840*4 -■d74d$)(z)
.
(3.18)
For the higher spin fields we proceed along similar lines. We note, however, that Woo is usually written in a quasiprimary basis, while all our Woo (ft) generators are by construction primary. In order to make the comparison for s = 4, we should consider W4 instead of W4. Using Eqs. (3.10), (A.l), (A.2) and (B.l) we obtain at ft = co W4(z) = -^(.d4>dP4> - 3d2
(3.19)
These are exactly the formulae we have given elsewhere,5 for the Woo algebra and they generalize for higher spin too. The general expression for the appropriate W, can be obtained from the following expansion ^i(* + e)tf_i(*) = - j
mS + n l)l 1 +^f*( * - 2 ()-! 12)2V' - 4 ^Tn ! ( (2S c"d»W(z)+ 0 w z s-l)!(25+n-l)! * * >+
+*(£)
(3.20)
The linearization of the Woo(ft) algebra at k = oo can also be seen explicitly in the example we gave earlier, since the difference (3.13) vanishes in this limit. (ii) Woo (ft) at k = 2: So far we have been mostly interested in WTO(ft) for real ft > 2. There is no a priori reason not to extend the range of ft to all real numbers.
625
Beyond the Large N Limit
65
The value ib = 2 is special because the central charge of the Virasoro subalge bra becomes infinite. Nevertheless, it is interesting to see what happens to the jy-symmetry there. In the examples we have already given, all non-linear terms disappear and there no need to make any field redefinitions. Moreover, the stress tensor and its composites do not appear in the commutation relations of higher spin generators which are well defined with no infinities involved. This can be eas ily understood by looking at the free field realization of W3(z), W4(z), Ws(z), etc. For k = 2, all terms involving the field 4>\{z) vanish and therefore the remaining field
T h e quantum version of these algebra* k described in Ref. 24.
626
66
I. Baku
« E.
KiriUit
in the sense that the OPE of any operator with a null operator will produce only null operators. Thus, WN is of cohomological nature, defined as the original algebra modulo the null ideal. This point of view is also adopted by Narganes-Quyano,22 while discussing the free-field realization of Wjv algebras in terms of two bosons. In the region —1 < k < 2, where the central charge is negative, we also observe a reduction of the Woo(k) algebra for some fractional values of k, like 1/2,4/3, • • • etc. The identification of the resulting W-symmetry is beyond the scope of the present work. Likewise, the relevance of Woo(k) to non-unitary SU{2) coset models with fractional level will not be considered here. We only note that for fractional k < — 1, there is no evidence that Woo(k) truncates to a finitely generated algebra and this might have implications to non-unitary conformal field theories of fractional type (see for instance Ref. 25 and references therein). (iv) Extension of Woo(k) for Rational k: When k is rational and positive**, the chiral algebra of the theory is larger. To see this, recall that the dimension of the parafermion operator ^j(z) is Aj = l + l2/k. Let us parametrize k as k = r/t, where r € Z+, t £ ZQ and they are relatively prime. It is obvious that the parafermion operators (and their adjoints) with / = nr, n G Z, have integer dimension A n r = nr(l + nt). Thus, we may consider a larger algebra, *££, which is an extension of Woo(k) by the parafermion operators VVw- The complete description of a basis in this algebra is given by W?(z) , where n€ Z labels the Zoo charge sector (the Zoo charge is nr) and s = 0,2,3, •• •. The dimension of W?{z) is nr(l + nt) + *. W°(z) are the Woo(k) generators with W§(z) = 1 and WQ(Z) = il>nr(z). The remaining generators are obtained from the parafermionic OPE and the fusion rules implied by the Zoo symmetry are [W?1] ® [W?'] = £[W7,' + ">] .
(3.21)
m"
When r is even, we can define a local algebra even larger than W£f, by including parafermions with half-integer spin as well. For r = Ir1, the parafermions \pnr' have dimension nr'(2 + nt)/2 and they form an algebra *|^ •*, where some of its generators are fermionic. Since we have assumed that r and t are relatively prime, t is always odd and r' can be even or odd. If r1 is odd, then, ipnr' with n odd will be fermionic. If r' is even, then, the algebra * ^ •* will contain bosonic generators of integer spin only. We also note that if r is proportional to the square of an integer, then *£,' can be extended further. We will encounter this generalization later for k = 9/4. 4. S L ( 2 , R ) / U ( 1 ) Characters In this section we are going to derive the characters for all unitary Woo(k) representations obtained from the SL(2,R)k/U(l) model. Their derivation relies on the intimate relation between the SL(2, R) current algebra and the N = 2 For k < 0 most of the parafermion operators have negative spin.
627
Beyond the Largt N Limit
67
superconformal algebra with c > 3. 7 In section 2 we gave a brief description of this relation at the level of the algebra. As shown in Ref. 7, for any state in the base of an 5L(2, R) current algebra representation, there exists one highest weight (hw) N = 2 superconformal representation. Let $£,(z) denote an operator* of the SL(2, R) WZW model with J3(z)Vm(w) = m ^ 4
, 7±(z)*i,(ii/) = C±U,m)^m±l{w)
+ 0(l)
Z — IV
+ 0(1) ,
Z — W
(4.1) where C 2 . = m(m ± 1) — j(j — 1). Using Eq. (2.10) we can factorize this operator
♦£, = try/I**)^ where $£, is an operator in the SL(2, R)k/U(l) ZL = '-**
(42)
t
theory. If we now define
^^«x)Vm(z)
.
(4.3)
then, Zh is an N — 2 primary operator with dimension A and U(l) charge Q given by
A
=
- j ( j - 1) + m 2 7
*- — F ^ ) — '
_ Qjm
2m (44)
"^2 •
The character of an N = 2 hw representation J2 is defined as XR = Trn[qL°wJo]. We are going to use the results of Ref. 26 where the characters of all unitary hw representations of the N = 2 superconformal algebra were derived from an analysis of the embedding structure of the null Verma modules'. The unitarity restrictions on these representations (viewed either as SL(2, R)k /U(l) or TV = 2 representations) are as follows: All the continuous series repre sentations are unitary. The trivial representation is also unitary. From the £)* representations only those satisfying 0 < j < Jfc/2 are unitary 8 . Thus, there are four different cases to consider corresponding to analogous SL(2, R) representations. (i) Trivial Representation, j — 0, m = 0: This corresponds to the vacuum representation of the N = 2 algebra, A = 0, Q = 0. For c > 3 there are two independent generating null vectors at relative charge ±1 and level (mode number) 1/2. The character in this case is* Xo(«,«0 = F
N S
( q , ^ ^ / i ^ ^ - i )
(45)
-
where FNS »S the unrestricted partition function FNS(q,w)
= /(<,)" 2 f[{l+
+ f-iw-1)
= f(q)-3
£
qn*'2wn
(4.6)
r»6Z
'Only the chiral part is important in this discussion. f The characters were also derived independently in Ref. 27 and for minimal representations in Ref. 28. 8 A n analysis of non-unitary SL(t,R)k/ U(l) representations will be presented elsewhere. It is enough for our purposes to consider only the NS sector.
628
68
/. B*k*$ & E.
KiriUu
811(1
oo
/(«)=II( 1 -« n )-
(4J)
n=l
(ii) Positive Discrete Series (D%): For the positive series we have j = n + e, where 0 < e < V and m = j + r, r e Z$. These are lowest weight (lw) 5L(2, R) representations. Here we have to distinguish two cases. (iia) j ^ Jb/2: There is one generating null vector in the corresponding N = 2 representations at relative charge —1 and level r + I. 2 6 The character is
xUlM^'^-/"'^^
(4-8)
(iib) j = Jb/2: In this case, apart from the charged null vector discussed above, there is also an independent one at relative charge zero and level 1. Consequently, the character is
*u» ■> ■«-—»»- (.+X-w+X-^ ■
(49)
(iii) Negative Discrete Series (!?„): For the negative series we have j = n—e, where 0 < £ < 1 and m = - j - r , r 6 Z 0 + . These are hw SL(2, R) representations and likewise we distinguish two cases. (iiia) j ^ Jb/2: There is one generating null vector at level r + | and relative charge 1. The character is Xj,m(q,w)
=
q
^ ^ - ^ ^ - .
(4.10)
(iiib) j = Jb/2: In this case there is also an extra null vector at relative charge zero and level 1. The character is
(iv) Continuous Representations: These correspond to the principal and com plementary series of SL(2, R) representations. In this case j(j — 1) < e(e — 1) and the representations are neither hw nor lw. In the principal series, j = ^ + ip, p € R, m = mo + n, n G Z, \mo\ < 1/2. In the supplementary series j is real with 0< | j - l | < £ + l , m = m o + n , n e 2 , | m o ± l | < | j - | | . These give rise to N = 2 representations with irreducible Verma modules. Consequently, the character is Xlm(q, «/) = qA'"WQ'">FNs(q,
w) .
'c=0 corresponds to SO(t,l) representations, while e=0 or J to SL(2,R)~SU(l,l) A general c corresponds to the universal covering group.
(4.12) representations.
629
Beyond (Ac Ltr/e N Limit
69
To go from N = 2 characters to SL(2, R)k/U(l) characters is rather straightfor ward. At the representation level, one has to decompose the N — 2 representations into U(l) representations and keep only the hw state of each U(l) representation. This is done by expanding the N = 2 character in a power series in w. The contribu tion of any given C(l) hw representation of charge Q appears as a factor multiplying u)Q. To factor out the U(l) representation, but its hw state, we must divide by the [/(l) multiplicity function f(q). One also needs to correct the dimension of a given U(l) hw state of charge Q by subtracting a factor ^fj?Q2. This way we can obtain the characters of the parafermionic SL(2, R)k/U(l) model, ipj,m(q), which define the non-compact analogue of the string functions c£,(g) via lfc.m(«)=/(«) *£,(«) ,
(4-13)
where f(q) was defined by Eq. (4.7). Another point to be stressed is the following. In the N = 2 case, starting from a hw state with a certain U(l) charge and acting with the supercharges, one moves to states that correspond to SL(2, R) states with different JQ eigenvalue compared to the initial one. Thus, for fixed j , starting with a certain m and decomposing the N = 2 character, we can obtain the characters of the whole coset module generated by the representation labeled by j . We summarize the results for the non-compact string functions.J (i) Trivial Representation: (-l)"g
c^Ofa) m
W
3
f(q)
Tl
'T —
(l + , H )
,m£Z.
(4.14)
n=l
(iia) D± j * fc/2: c>m(D;q) = *
-iV-n + u-tr)' oo —53 ^ - l ) " * * ^ .
M
meZ.
(4.15)
n=0
(iib) D±, j = k/2: ckJ2(D;q)=c£°(q). (iii) Continuous
(4.16)
Representations:
c3m(c;q) =
jT-73
, m = mo + n , n£Z
.
(4.17)
We should remark that the identity (4.16) also holds in the compact SU(2) case. Using the above we can write the following decomposition formulae for the N = 2 characters, which are generalizations of the compact case.30 For the D± representations we obtain ^±0+r)(9.^)=E^(n"r"2^fi)^,>"r"2^^(I?:) J
•reZo±
The character* in cases (iia) and (iii) have been calculated previously in Ref. 29.
(4-18)
630
70
I. BtUt
& E. Kirii$u
respectively. For j = 0 we obtain the result for the trivial representation, while for the continuous series,
XL(9, «0 = £ « * ( - * * ) > - » c>m_n(c; q) .
(4.19)
nez The relations above differ from the compact case (N = 2 minimal models) , where the string functions are periodic with period 2k, due to the Z* symmetry . This turns the infinite sum into a mod 2k sum and produces the 51/(2) ^-functions,30,31 X«™P°<*=
k
£
Jm){q)dmW)_^Mk+2)(^*\
I
m'=-fc+l m'=-fc+
^
( 4. 2 o) ''
where tfm>fc(T> z) =
£
,*» ,«*» , ? = e 2 ™ , u; = e 2 ™
(4.21)
n€Z+m/2k
is the standard t?-function. We can now compute the characters of ail SL(2, R)k representations which give rise to unitary SL{2, R)k/U{\) representations. We summarize the formulae for the affine characters, defined as Tr[qLowJ«]. (i) Trivial Representation:
where
»(«,«») = A (1 - qn)(l - Qnw)(l - qnw~l) .
(4.23)
n=l
(ii) D+ Representations,
j ^ k/2:k
X f *(«,») = J
'" „ , ■ (1 - tw)7r(9, w)
(4-24)
For the D+ representation with j = k/2, the Verma module is reducible because there is a null vector at level one. This is the only hw representation embedded in it, since it transforms as a j ' = | — 1 representation. Consequently, the character is
x^^i-^flVT'1'
<4-25)
(1 — w)ir(q, w)
Formulae (4.24) and (4.26) were obtained in Ref. 32 where questions of modular invariance were addressed.
631
Beyond tke Large S Limit
(iii) D~
71
Representations: SLj *J
"to,-«0
SL
U.
,'**. ^ U V - J ( 1 - t u - l M«,'« " ) '
(4.26)
" J ( l - qw)
\— V
i — u/
(4.27)
y«\«f, u//
For the continuous series the characters converge nowhere in the complex w-plane. The SL(2, R)k characters above are related to the non-compact string functions via a generalization of the Kac-Peterson formula,33 x f *(«,«;) = £
q~U±^^+mcin(D;q)
.
(4.28)
mGZ
The string functions cPm are the characters of Woo{k) representations with Zoo charge m l . In particular, the string functions associated with the trivial (j = 0) representation are the W^k) characters of the parafermions ipm(z), with m > 0 and their adjoints, with m < 0. c 0 is the character of the vacuum module of the Woo(k) algebra. It is obvious that the state multiplicities in all Woo(k) characters are independent of k. Consequently, the counting of independent states, null states and generators is the same for all Jb > 2 and in particular, it coincides with that of Jfc = oo. The number and structure of null states of Woo(k) representations can be obtained from the explicit realization of Woo in Ref. 5. From Eq. (4.28), we can obtain for j = 0 the non-trivial identity £ & ( « ) = /(9)-3 + 0 ( l / * ) .
(4-29)
m€2T
which describes the decomposition of the vacuum representation of the current algebra into Woo representations. 34
U(l)xU(l)
5. Applications to 2-d Quantum Gravity The presence of the Woo{k) symmetry in the SL(2, R)k/U(l) coset model sug gests the existence of an infinite number of conservation laws for all A; > 2 and in particular for Jb = 9/4, which corresponds to Witten's black hole solution. Let us introduce the following charges Q.=
IdzW.{z),
«>2,
(5.1)
Sometimes string functions are referred to as parafermionic characters. This is not correct. A parafermionic representation whose moduk is generated by the action of the parafermionic currents decomposes into a finite sum of W-representation* in the SCf(B) case and into an infinite sum of WOO(IE) IT'l'"!■■+»»ion? in the SL(l,R) case. Parafermionic representations are in one to one correspondence with SL(t,R) representations.
632
72
1. Baku, & E.
KiriUit
which by definition are identified with the — s+ 1 Fourier mode of the W,(z) fields, i.e., Q, = W$—+l) • (5.2) Clearly, in order to insure that all Q, are in involution, W.,O.»J = 0 , V * y > 2 ,
(5.3)
the W-generators of the algebra must satisfy the condition I dz I dw W.(z)W.>(w) = 0 .
(5.4)
At this point one might think that the non-linear terms of the Woo(k) algebra violate the condition (5.4). This condition is certainly valid in the limit k —* oo, after introducing the standard quasiprimary field basis of Woo - 4 ' 5 Eq. (5.4) will be true in general, iff the coefficient of (z — w)~l in the OPE W,(z)Wa>(w) is a total derivative. It follows from the results we have already presented that the OPE for s = 3, s' = 4 does not enjoy the desired property. Hence, the question arises whether there are appropriate redefinitions of the JV-generators which can give rise to infinitely many charges in involution. Our attitude is that this is indeed the case, although we cannot provide a complete proof because the commutation relations of Woo(k) are not yet known in closed form. Later we will reformulate this conjecture in a language which is analogous to the conservation laws of the KP hierarchy and suggest an alternative way for interpreting the charges Q, in involution. We also note that the field redefinitions we are searching for s > 4 should yield the quasiprimary field basis of Woo in the limit k —► oo, for which Eqs. (5.3) are automatic. Let us now sketch the basic steps for constructing a new spin-4 generator which is compatible with Eq. (5.4). Apart from the OPE (3.9) we also have »r /
+6^
\ .,/2 / x
+
48/1
Id2
Id
1 ^ , , , , ,
H): W2W3 : (,) + <-WVn:U
+ 0{1) f
m
which can be computed directly, using the free field realization of the W-generators, or more easily using the general formulae
(■.Wi:{zl)W.(z2)WM)=s(s+l_£r) (W.(z2)W.(za)) <: W2W, : (zi)W.(z2)
: Wj : (z3)) _
~ f
(56fl) v
'"5'*?2zk
2s(8s-5)1
z\2
(5.66)
633
Beyond tke Large N Limit
(: {dW7)W. : (*i)ty,(z 2 ) : Wj : (z 3 )) <W,(n)W.(z 2 )>
-
4s(s - 1) 5+ 2
|
(5-2)(3«-l)1
73
z12
s+ 1
J z[zz-a ' (5.6c) Here c is the central charge of the Virasoro algebra and W, are Virasoro primaries. Then, the combination
WT-M = W,W + « ( * + 2(ite"_ 3) ^" 2) : * ? : W
(5.7)
has an OPE with W-i, W3 with single pole that contains only total derivatives, as required. We point out that the spin 4 field (5.7) is different from W^z) introduced earlier (cf. Eq. (3.11)). They both coincide, however, in the the limit k —► oo, according to the general expectation we mentioned. Carrying out this procedure for other higher spin fields is straightforward, but cumbersome and it will not be dealt with here. It would be interesting to describe the complete structure of W^k) , not in terms of primary field generators, but in a basis which makes the conditions (5.4) manifest. Whether this is possible in practice or a formidable calculational task remains to be seen. Before we proceed further, two remarks are in order, with emphasis on Witten's black hole solution. First, for k = 9/4, the parafermion fields xpi(z) with / = 3n, nE Z, are local operators with integer dimension A, = n(4n + 3) .
(5.8)
Therefore, as we explained earlier, one might consider enlarging Woo(k) by includ ing {V^n(2)} >n ' n e spectrum. This extended W-algebra governs the physics of the 2-d black hole solution and we expect it to be the maximal symmetry of the model. It would be very interesting to analyze its structure in detail and study the algebra of charges associated with the V^n generators. Of course, similar questions can be raised for arbitrary (but rational) values of k. As for the 2-d black hole, it would be interesting to know whether there is any relation between the parafermionic exten sion we are considering here and the algebra of volume preserving diffeomorphisms of the 3-d cone introduced by Witten in his recent study of 2-d string theory. 35 Second, the existence and explicit construction of an infinite family of inde pendent charges in involution is very important for understanding the physics of 51.(2, R)k/U(l) coset models, in general. For the black hole solution, in particular, the set {Qs} could be responsible for the maintenance of quantum coherence in the Hawking evaporation process (see for instance Ref. 36 for some preliminary results in this direction). It is an interesting problem to find the target space interpreta tion of the Woo(k) symmetry (and its parafermionic extensions for fractional k) and examine whether the quantum mechanical states of the theory can be completely classified by the corresponding conserved charges. We hope to address these issues elsewhere.
634
74
/. Bmktt & E.
Kirittu
Next, we present some thoughts aiming at a deeper connection between the conservation laws of the SL(2, R)k/U(l) coset and those of the KP hierarchy. The basic idea here originates in the recent works of Yu and Wu, 17,19 who studied the bi-Hamiltonian structure of the KP hierarchy (see also Refe. 18,20). We review their main results for the completeness of our presentation. The interpretation we will put forward for the charges Qt is essentially a quantum mechanical version of the classical KP integrals. Recall that the KP hierarchy can be formulated as a Lax pair, using the pseudodifferential operator oo
L = dz + ^2ur(z)d:r-1
(5.9)
r=0
(for details see Ref. 37 and references therein). For the Hamiltonian description of the KP hierarchy we introduce the following quantities Ht = -resL'
, s € Z+
(5.10)
and consider the corresponding charges, H, = jdzH,{z),
(5.11)
as Hamiltonian functional for the various flows. The first Hamiltonian structure of the KP hierarchy is given by the commutation relations of W\+00 with zero central charge, which in terms of the {u r (z)} variables assume the Watanabe form, 38 {ur(z),u.(w)}{1)
= K£Hz)6(z-w)
Kg>(z) = £ ( - 1 ) ' (f}ur+.-i(z)tf. 1=0
- £
^ '
,
(fjSiur+t-i(z)
(5.12a) .
(5.126)
1=0 ^ '
The appropriate change of variables that establishes the isomorphism with Wi+oo is given by
It also follows from the integrability properties of the KP hierarchy that the charges (5.11) are in involution, i.e.,
{«.,«.'}(») = ° •
(5-14)
If we change basis from (5.13) to (5.10), the commutation relations of Wi+00 will assume a non-linear form, which Yu and Wu related to the second Hamiltonian structure of the KP hierarchy as follows, j> dw {H.(z), H.,{w)}m
= jdw
{H.(z), H..+1 (ti;)} (1) .
(5.15)
635
Beyond the Large N Limit 75
The second structure of the KP hierarchy is non-linear, given by the commuta tion relations {«,.(*), ti.(u>)}(2) = K$(z)6(z - w) , (5.16a) where
«S>M = D - 1 ) ' ( r t ' W - n - K ^ - £ (s! 1)al«.+r+1-1(2)+ J=0
^
'
1=0 ^
'
+£[E TVi^^r.v^ 1=0 Lm=r+1 "
£
m=»+l
V
fc=0
>
(-l)'(m"f"1)|«m-J-lWaillr+.-mW
^
•
(5.166)
'J
Change of basis to the variables (5.10) maintains the non-linear features of (5.16) and gives rise to a non-linear deformation of the centerless Woo • denoted by Woo in Ref. 19. The Woo algebra of Yu and Wu is classical with zero central charge, but it resembles the general structure of Wao{k) , provided that H,(z) is identified with Wt+i (z) (* > 1). For comparison we also have to introduce appropriate redefinitions which transform Woo(k) to a non-primary field basis. The recursion relations (5.15) are sufficient to insure that the charges Q«+i = 7i, of Woo are all in involution. This follows by integrating Eq. (5.15) with respect to z and noting that its right hand side subsequently vanishes, thanks to Eq. (5.14). Therefore, although the relation between the classical algebras W\+00 and VVoo is indirect and valid only in the integrated form of the commutation relations (5.15), the implications for Woo are substantial and not at all obvious without the KP point of view. The most important point for us is the identification of the Woo charges with the conserved quantities of the KP hierarchy and their explicit construction in terms of W\+oo generators, as dictated by Eq. (5.13). We are now in the position to state our proposal for the conservation laws of the 2-d black hole solution, after choosing a suitable non-primary basis for the gen erators of Woo(k) . The charges Q, are the conserved quantities of a quantum deformation of the KP hierarchy. In the theory of quantum integrable systems, usually only one of the two Hamiltonian structures survives,39 and therefore recur sive relations of the form (5.15) cannot be used to prove complete integrability. The latter is established by explicit computation case by case, which is a very cumber some procedure, as the one we encounter for the black hole. Quantum equations of KdV type are naturally defined by means of their quantum second Hamiltonian structure. The obvious candidate for our problem is Woo(k) with c* ^ 0 and this is the essence of the proposal.
636
76
/. B«i«» & E.
KiriUit
The quantum deformation of the KP hierarchy we advocate for interpreting the black hole charges is rather speculative at this point and further work is required to illuminate it. If it exists, however, it would have important consequences on the relation between SL(2,R)k/U(l) coset models and the ordinary KP approach to non-perturbative string theory via matrix models. In this framework, it will be also interesting to examine whether recursive relations between Woa(k) and Wi+oo with non-zero central charge still exist for some miraculous reason, for certain values of Jb. We also hope to address these issues elsewhere. 6. Conclusions and F u r t h e r Remarks In this paper we studied the generic chiral symmetry of the 51,(2, R)k/U{\) coset model. It is described by the non-linear algebra Woo{k) with an infinite number of generators of spin s = 2,3, • • •. This is a universal W-algebra (for the ^-series of extended conformal symmetries), since at Jb = —N with N = 1,2, • • •, it truncates to the usual Zamolodchikov Wp/ algebras. As k —» ±oo, one recovers the usual Woo algebra, which is linear in a quasiprimary field basis. We have investigated the general structure of Woo(k) , using its relation to compact and non-compact parafermions. We have also constructed a free field realization of the algebra in terms of two bosons with background charge. For Jb = 2, the central charge of the Virasoro subalgebra is infinite, but as we argued, the generators with spin s > 3 form a well-defined closed linear subalgebra. Several other truncations seem to be possible for certain special values of Jb < 2. For rational values of Jb = r/t, the chiral algebra Vv*oo(Jb) can be enlarged further by including all parafermionic operators with integer (or even half-integer) spin. This yields a double graded algebra which definitely deserves more attention, in particular for Jb = 9/4. The complete structure of Woo(k) in closed form remains an open problem. The spectrum of the SL(2, R)k/U(l) coset model is built out of hw representa tions of Woo(k) . We computed the characters (generalized string functions) of all unitary representations of JVoo(Jb) , using the relationship between SL(2,R)k/U(l) and the N = 2 super conformal representation theory with c > 3. The characters for the vacuum module provided crucial information on the spectrum of Woo(k) . which is the same and infinitely generated for all Jb > 2. As a byproduct, we also obtained the SL(2, R)k characters for representations in the discrete series. Woo(fc) is related to various approaches to 2-d gravity in two possible ways. First, it is a symmetry of the black hole solution (for Jb = 9/4). The existence of an infinite number of integrals in involution will characterize the structure of string theory in the black hole background. This could have important implications on questions of loss of coherence during black hole evaporation. We conjectured the existence of such integrals in involution, based on explicit calculations up to s = 4 and their existence for all s in the large Jb limit. This algebra also seems to be a quantum version of the second Hamiltonian structure of the KP hierarchy. Due to the importance of the this hierarchy to matrix model approaches to 2-d quantum gravity, it is reasonable to expect that Woo(k) could help illuminating the KP-like
637
Bcfoni
ike Large N Limit
77
integrable structure of 2-d string theory. Finally, we conclude by discussing some further generalizations of the W sym metry of 51/(2, R)ie/U(l) to higher rank coset models. In Ref. 5 we constructed a "colored" generalization of the usual Woo algebra, denoted by Wg,, which is linear and contains W^ as a subalgebra. W^ arises as the N —<• oo limit of the chiral algebra of the Grassmannian coset models SU(p+ 1)N/(SU(P)M X (7(1)). One may consider the non-compact version of these models, SU(p, l)k/(SU(p)k x (7(1)) and examine whether the corresponding non-linear chiral algebra has the same spectrum as Wgo. Again, when k becomes a negative integer, the algebra should truncate to the finitely generated chiral algebra of the compact coset. It would be interesting to investigate this generalization of Woo(k) , since it also qualifies as a universal Walgebra for the A-series of extended conformal symmetries, but for a wider range of values for the central charge. It also remains a challenging question to find a framework for constructing the most universal W-symmetry that contains all possi ble chiral algebras of 2-d CFT. Such master symmetry could play a prominent role in the non-perturbative study of string theory. Acknowledgements This work was initiated while both of us were attending the "Infinite Analysis" workshop at the Research Institute for Mathematical Sciences in Kyoto. We are grateful to Prof. T. Miwa and all other members of RIMS for their kind invitation, generous financial support and Japanese-style hospitality, which provided us with a very enjoyable and stimulating environment. Special thanks are due to Prof. T. Inami for the hospitality extended to us at the Yukawa Institute for Fundamental Physics. We are also grateful to Prof. L. Alvarez-Gaume and all other members of the Theory Division at CERN for their hospitality and financial support during the last stages of this work. E. K. would also like to thank the organizers of the Aspen Summer Institute and the Ecole Normale Summer Institute for hospitality and financial support, during the course of this work. N o t e Added After the completion of this work we received Ref. 40, where the parafermionic characters discussed in section 4 were independently obtained. References 1. A. B. Zamolodchikov, Theor. Math. Phys. 85 (1985) 1205; A. B. Zamolodchikov, V. A. Fateev, Nuel. Phys. B280 [FS18] (1987) 644. 2. V. A. Fateev, S. L. Lykyanov, Int. J. Mod. Phys. A3 (1988) 507. 3. I. Bakas, Phys. Lett. B228 (1989) 57; Comm. Math. Phys. 134 (1990) 487; "Area Pre serving Diffeomorphisms and Higher Spin Fields in Two Dimensions" in the Proceedings of the Trieste Conference on "Supermembranes and Physics in 2+1 Dimensions", eds. M. Duff, C. Pope and E.Sezgin (World Scientific, 1990), p. 352. 4. C. Pope, L. Romans, X. Shen, Phys. Lett. B236 (1990) 173; Sucl. Phys. B339 (1990)
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/. B*ktt & E. KiriUis
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Beyond tke Large N Limit
79
34. S. Odake, T. Sano, Talk given at the KEK Workshop on Superstrings and CFT, Dec. 1990. 35. E. Witten, IAS preprint, IASSNS-HEP-91-51, Aug. 1991. 36. J. EUia, N. Mavromatos, D. Nanopoulos, CERN preprints, CERN-TH-6147/91, Jun. 1991, CERN-TH-6229/91, Sep. 1991. 37. G. Segal, G. Wilson, Publ. Math. IHES 61 (1985) 5. 38. Y. Watanabe, Lett. Math. Phys. 7 (1983) 99; Ann. Di Mat. Pur. Appl. 137 (1984) 77. 39. R. Sasaki, I. Yamanaka, Comm. Math. Phys. 108 (1987) 691; Adv. Stud. Pur. Math. 16 (1988) 271; B. Kupershmidt, P. Mathieu, Phys. Lett. B227 (1989) 245. 40. J. Distler, P. Nelson, Pensylvania preprint, UPR-0462T, Aug. 1991. Appendix A In this appendix we give the free field realization of the primary W4(z) and Ws(z) generators. Normal ordering is implicitly assumed.
W4(z) = -
6
^_1?) [ a ^ )
4
-1- a2(d
+ <* 5 (dVi) 2 + <*6 d
+ as d*4>x + a 9 d2
+ a10d2
(Al)
where a i = (Jfe-2)2(6Jfc + 5) a 3 = 6(Jk-2)(2Jfe2-13Jfc + 8) a 5 = -2(ik - 2)(6* 2 - 12fc + 1) a8 = -|(ib2-Jb-»-l)v/2(Jb-2) a 1 0 = -2(Jb - 2)(6Jb + 5) v/2(Jfe-2)
Ws(z) =
16» 5Jfe2(64Jfc - 107)
a 2 = (fc-12)(2Jfe-l)(3fc-4), a 4 = -2(3Jk - 4)(2Ar2 + 2k + 3), a« = a7 = 8(Jb - 2)(Jk2 - it + 1), a 9 = - 2 ( 2 * - 3)(19fc-8)y/2(fc-2), a n = 4Jt(16Jk- ll)y/2(k-2). (A.2)
m 0x(d
4
2
+ 0A(d
+fe{d2
+ ,/2(k-2)(il(d
+ 72 d2Md
+ f3(d
+ 7s dPfa&fa + 76 #4>i&4*+
+ 77 d*
3
>2)
l
(A3)
+
640 80
I. Btkas & E. KiriUis
where A = 6(2* - l)(5Jb - 24)(5* - 8) 03 = 60(* - 2)(2* - 3)(5* - 8) /?5 = 1 5 ( 5 * - 8 ) ( 6 * 2 - 7 * + 8) 07 = *(* 2 - 3Jfc + 5) 09 = - 3 0 ( * - 2)(38* 2 - 63* - 2) 7 i = - 1 5 * ( * - 2 ) ( 1 0 * + 7) 73 = 1 5 ( * - 2 ) ( * - 4 ) ( 1 0 * + 7) 7 5 = - 1 5 ( 2 * - 3 ) ( 2 * 2 + * + 8) 77 = 1 0 ( * - 2 ) ( * 2 - 3 * + 5)
02 = 3O(k-2)2(lOk + 7), 04 = -15(Jb - 2 ) ( 2 * 2 - 71k - 16),
& = -30(5*-8)(4* 2 + * + 6),
& = 180(*-2)(3*2-4), 0io = 30(* - 2)(16Jb2 - 31* + 16), 72 = 15(5* - 8)(2* 2 - 33* + 12), 74 = - 1 5 * ( 5 * - 8 ) ( 2 * - 2 5 ) , 76 = 15(4* 3 - 10* 2 + 13* - 16), 78 = - 1 0 * ( * 2 - 3 * + 5).
(A4)
Appendix B In this appendix we give the free field realization of the composite operators appearing in the OPEs (3.7) and (3.9). • Wi : (z) = i ( 0 ^ ) 4 + l-(d
- \
d
+ ^l _ 2) Qt #*i - &Md
W2W3 : ( z ) =
8i*\/!
(B.i)
- 2 8 ( 3 * - 4)(d
- 56(3* - 5 ) ( a ^ 0 2 ( 5 ^ 2 ) 3 + 2(17* - 1 8 ) ( 3 ^ i ) 2 # V 2 - 12(19* - 24) S ^ i A V i S 2 ^ + 2(65* - 96)(5^ 2 ) 2 5 3 ^2- 72(3* - A)d
+ 12(* - 2)(d7
+ * &
+ 2 U N / ^ _ 2 ) "7(3*2 " 18* + 2°)
^W+
+ 2 1 * ( * - 2)(d
+ 48)d2
(5.2)
641
Beyond tke Large N Limit
: (dW2)W3 :(z) = y ^ ^ f
- eid^fd^dfc
?(* - 2)(d
81
6(d4>2)2d*^-
+ Hdfaf&fo) + (3k - 4) (-ib(d2
- 42d<j>id2
Wd
- (13* - 66) d
\5ky/k(k-2)
(it - 2)(d*4>1d22 -
ls&faidttfdfa +
+ \2d24>l{d4>i)2d24>2 + 24d