PHYSICAL REVIEW D VOLUME 39, NUMBER 2 15 JANUARY 1989
Absence of (1,0) supersymmetry anomaly in world-sheet gauge theories: A purely cohomological proof
Zi Wang Department af Physics, Utah State University, Lagan, Utah 84322
Yong-Shi Wu Department af Physics, University af Utah, Salt Lake City, Utah 84112 (Received 9 August 1988) A purely co homological proof is given for the absence of the (1,0) supersymmetry anomaly in gauge theories on a world sheet. In particular, it is shown that generalized co homological ap proaches to anomalies in supersymmetric gauge theory, either formulated in whole superconnection space or only in the Wess-Zumino-gauge surface, yield results which agree with those obtained by noncohomological field-theoretical methods. We argue that the success of the cohomological argu ments implies that there should be a generalization of (family) index theorem in the supersymmetric cases.
Anomalies in quantum theory have played a ubiquitous string-model construction arises from it. Our discussion role in particle physics, not only in unified gauge theories also verifies the consistency of generalized cohomological (the standard model and grand unified theories) but also arguments with other noncohomological field-theoretical in string theories. In the latter, it is generally believed methods in the supersymmetric cases. This not only that space-time physics has its origin in D = 2 dimension shows the validity of the cohomological approaches, but al world-sheet physics, although the connection is only also implies that there should be a generalization of the partially understood. An important link between them (family) index theorem in the space of superconnections. has been provided by anomalies in the D = 2 quantum Whether there exists such a generalization is an interest field theory which describes the propagation of a string in ing open problem. Our argument in favor of a positive certain space-time backgrounds. For example, the well answer is the following. known critical dimension and modular invariance of a The absence of a supersymmetry anomaly seems to be string theory I are both actually anomaly-free conditions a quite universal rule. If so, there must be a deep reason for the D =2 field theory. The discovery of any new for it. It might be related to the fact that a superspace (or anomaly would impose extra constraints on string-model supermanifold) is always topologically trivial in the fer construction and would provide new insight into space mionic directions, II and this topological triviality might time physics. be somehow carried over to a supersymmetry orbit in the Since supersymmetry turns out to be an important in space of superconnections. If this is true, a generaliza gredient for the construction of realistic string models, it tion of the index theorem or family index theorem might is interesting to see whether or not there is an anomaly underlie the absence of the supersymmetry anomaly. On for it. Although no supersymmetry anomaly has ever the other hand, it is well known that in nonsupersymme been found in all presently known models, a deep under trical gauge theories the validity of usual cohomology ar standing of this absence is still in demand. Several ap gument for chiral gauge anomalyl2 is assured by the fami proaches to anomalies in, say, supersymmetric gauge ly index theorem in the space of connections. 13 Without theories have been suggested and worked out in higher the latter, the usual cohomology argument only provides dimensions (D ~ 4) (Refs. 2--4). But no two results look us with a solution to the Wess-Zumino consistency condi alike, so usually we do not know whether or not they are tion,14 but we are not sure that this solution is the right consistent with each other. A principle for comparing one, since solutions to the consistency condition may not the results in different approaches has been suggested by be unique. The family index theorem guarantees that the us some time ag05 (see also Zumin06 and Hwang7); never solution provided by the usual cohomology argument is theless it is difficult to practice it in D ~ 4 except for a few indeed the right one. The existence of this theorem may cases. In D = 2, the situation is much simpler: the re have been indicated by the fact that the result from a per sults7- 9 do not look very involved. So we feel it is possi turbative calculation 15 or path-integral derivation 16 coin ble to directly compare various approaches by applying cides with the solution provided by the usual cohomology our method,S and we expect to gain some insight into the argument. Namely this coincidence of the results ob problem from such comparison. tained by apparently different methods should not be con Here we report on a recent study on 0,0) world-sheet sidered as purely accidental; there must be something supersymmetric gauge theories which have been lately deep and fundamental hidden behind it. Now we can re explored in the construction of consistent string models. 10 peat this line of reasoning for the supersymmetric cases: Our study confirms again that there is no supersymmetry if once again a generalized cohomology argument can anomaly in these theories and, therefore, no constraint on reproduce the results obtained by other field-theoretical
39 509 © 1989 The American Physical Society 510 ZI WANG AND YONG-SRI WU 39
methods, there should be a sort of generalized family in A G [ A ;A]=8G (A)Weff[ A] , dex theorem which makes the generalized cohomology (5) argument valid. This is why we are interested in a new As[A ;E]=8S (E)Weff[A] . proof of the known absence of a (1,0) world-sheet super In Ref. 9 the gauge anomaly is obtained by a generalized symmetry anomaly8 from a cohomological point of view. cohomology argument in (l,0) superspace as follows: In this paper, we restrict ourselves to gauge theories with (1,0) global supersymmetry. [Our treatment applies AdA ;A]=c f d 2x dOTr[AW_ Ae-DeA-)] (6) also to (p,q) supersymmetric theories which can be writ ten in terms of (1,0) superfields by projecting into (1,0) su (where c is a constant depending on the representation perspace.] We hope to discuss the locally supersym content of matter superfields) with no mentioning about metric cases (supergravity) in later publications. Results the supersymmetry anomaly As[ A ;E]. We note that the of this study have been briefly announced in Ref. 17. integrand in Eq. (6) is the e - ee component, as it should For closed strings, the simplest world-sheet supersym be, of lU~( A,F) == Tr[A(F - A 2)]. Here lU~( A,F) is one of metry is (1,0) supersymmetry.18 For our notation we are the quantities appearing in the usual descent equations 12 going to use the flat superspace used by Ovrut and his in D = 2, but now with A and F being superforms. collaborators. 19 (For other references on the same sub Again, it is the descent equation satisfied by lU~( A,F) ject, see Ref. 20. Although the notations in the first pa which guarantees that the right-hand side of Eq. (6) per of Ref. 20 have more indices, they are convenient for satisfies the Wess-Zumino consistency condition for the keeping track of the Lorentz transformation property.) anomaly AG in superconnection space.9 The superspace coordinates are z M = (x ±, 0) where 0 is a To check this result and prove that it implies the ab Weyl-Majorana spin or. The (1,0) supercharge is sence of supersymmetry anomaly, we use a technique we Q=da/aO-iOa/ax+), satisfying !Q,Q}=2ia/ax+. invented before,s i.e., first study the anomalies in the The supercovariant derivatives are given by Wess-Zumino (WZ) gauge in the way Itoyama, Nair, and DM=(D±,De); D±=a/ax±, De=a/aO+iOa/ax+. In Ren4 did in D 2: 4 and then compare them with the above (1,0) superspace, one can define scalar superfields Ad A ;A] [Eq. (6)] by the method we suggested in Ref. 5.
(2) [We have used little g and s to distinguish the (usual) gauge transformation (7) and the (combined) supersym a where A==Aa(z)UT ) is an infinitesimal scalar superfield metry transformation (8) in the WZ gauge from the (gen taking values in the Lie algebra of G. The gauge and su eralized) gauge transformation (2) and the (usual or persymmetric invariant action is genuine) supersymmetry transformation in superspace
2 which are labeled by capital G and S.] It is easy to work S = f d x dO[ -TrF -e:DeF _e+1Je
(usual) gauge orbit of A in the WZ gauge, which acts on Now we expand w~( A +v,F) into terms of different de the parameters t; of the gauge functions a( x ; t I' ... ) in grees in v, e±, and ell: transformations (7): w~( A +v,F)= ~ W;,q (v, A ,F) , (32) 8 A=-dv-[A,v], 8v=-v2 . (22) p +q +k =3 where k =degree of v, p =degree of e±, q =degree of ell. Then we identify, following Borona, Pasti, and Tonin,3 Substituting Eq. (32) into Eq. (31) and equating forms with same (p,q, k) degrees, one obtains the descent equa 1= f d 2x 8( ... ) , tions which are the supersymmetric generalization of the (23) usual ones in Ref. 12. However, we point out a special 1= f d 2x i.D ( ... ) feature of the D = 2 (1,0) supersymmetrical case: namely, one has the identity as the coboundary operators along the gauge and super TrF2 =0 in D =2 (1,0) superspace . (33) symmetry orbits, respectively, for a local functional of A This follows from the constraint Fell = 0 and the Bianchi and F in the WZ gauge. Here the definition of i. which identities, since they together lead to acts on a super m-form F +11=0, F +_ =iDIiF -II . (34) (24) (Note that in the supersymmetric case a pnon a super four-form in D = 2 may not be zero, since dx + dx - d (J d (J is given by does not vanish. Similar identities have been noticed by 3 Borona, Pasti, and Tonin in D:::: 4 cases. ) U sing the (25) identity (33), the descent equations derived from Eqs. (31) and (32) take a simpler form. Among others one has
A 0 0 with EA=(O,O,E). 8g and 8s satisfy the relations dWI,2+Dw2,[ =0,
(26) 8W?,2+ dwL+Dwi,0=0, (35) 8wi,0+dwlo=0. Therefore, for the gauge and supersymmetry anomalies in the WZ gauge . From these equations we immediately see that if one identifies the anomalies in the WZ gauge by the cohomo (27) logical ansatz
Ag [ A ; v ] = c f w1 0 I ' we have the consistency conditions x ' 11=0 (36) As [ A ; E] = c i .w~ I I ' (28) f x ' e=o then they automatically satisfy the consistency conditions which is the cohomological form of our previous con (27). A straightforward calculation shows that sistency conditions (0). Ag[A;v]=cfd2xTr[vW_V+-D+V_)] , (37) To obtain the solution to Eq. (28), we follow a cohomo logical procedure, which can be viewed as another gen (38) eralization of the usual one12 to the supersymmetric case. Let us consider TrF 2. Here Tr acts on the matrix (or Lie Namely, they coincide with Eqs. (12) and (13) we have algebra) part as before. Similar to the nonsupersym obtained before; but now they are deduced from a coho metric case, one has mological ansatz (36). In conclusion, we have applied both a field-theoretical version of Itoyama, Nair, and Ren4 and a modified ver sion of Borona, Pasti, and Tonin's cohomological ap We introduce proach3 to study the gauge and supersymmetry anomalies in the WZ gauge in world-sheet (1,0) supersymmetric (30) gauge theories. We find that the results from the two ap proaches coincide with each other. Also by using a tech and derive from d 2=8 2=d8+8d =0 and ~2=0 that nique we suggested before,s we have compared this result 8 ;J=F. Thus, with the result obtained by Ovrut and his co-workers with a co homological procedure in superconnection space; and we confirm the absence of (1,0) supersymmetry TrF 2=Tr;J2= ~w~(.A,;J) in superconnection space, which has been proved in =(d +D +8)w~( A +v,F) . (31) the literature by noncohomological field-theoretical 39 ABSENCE OF (1,0) SUPERSYMMETRY ANOMALY IN WORLD- ... 513 methods.8 Therefore, we have checked the consistency of existence, at least in D = 2, of a generalized (family) index the results from several different approaches for theorem in the space of superconnections which underlies anomalies in supersymmetric gauge theory in the D =2 the co homological approach. 0,0) case. Moreover, as we argued at the beginning of the paper, the coincidence or consistency of these results Y.S.W. was supported in part by NSF Grant No. from field-theoretical and cohomological methods not PHY-8706501. Z.W. thanks Professor V. G. Lind for en only verifies the validity of the latter, but also implies the couragement.
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