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Global anomalies in canonical gravity

dc.contributor.authorSurya, Sumati
dc.contributor.authorVaidya, Sachindeo
dc.date.accessioned2012-05-28T03:43:57Z
dc.date.available2012-05-28T03:43:57Z
dc.date.issued1998-07
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations)en
dc.description.abstractIn this note we study the structure of diffeomorphism anomalies in 3+1 canonical gravity coupled to a chiral massless fermion. We find that when the spatial manifold Σ is S3 or a Lens space L(p,q), the first homotopy group of the related diffeomorphism group can be non-trivial and hence the question of global anomalies becomes relevant. Here we show that for gravity coupled to SU(2) chiral fermions, assuming the strong form of the Hatcher conjecture, SU(2)-induced diffeomorphism anomalies do not occur whenever Σ is S3 or a Lens space.en
dc.identifier.citationNuclear Physics B, 1998, Vol.523, p391-402en
dc.identifier.urihttp://hdl.handle.net/2289/4544
dc.language.isoenen
dc.publisherElsevier B. V.en
dc.relation.urihttp://arxiv.org/abs/hep-th/9709170en
dc.relation.urihttp://dx.doi.org/10.1016/S0550-3213(98)00286-7en
dc.relation.urihttp://adsabs.harvard.edu/abs/1998NuPhB.523..391Sen
dc.rights1998 Elsevier B.V.en
dc.titleGlobal anomalies in canonical gravityen
dc.typeArticleen

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