Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/6215
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dc.contributor.authorMERULIYA, VIRAJen_US
dc.contributor.authorMUKHI, SUNILen_US
dc.date.accessioned2021-09-01T05:07:45Z-
dc.date.available2021-09-01T05:07:45Z-
dc.date.issued2021-08en_US
dc.identifier.citationJournal of High Energy Physics, 2021(8), 98.en_US
dc.identifier.issn1029-8479en_US
dc.identifier.urihttps://doi.org/10.1007/JHEP08(2021)098en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/6215-
dc.description.abstractWe use the Poincaré series method to compute gravity partition functions associated to SU(N)1 WZW models with arbitrarily large numbers of modular invariants. The result is an average over these invariants, with the weights being given by inverting a matrix whose size is of order the number of invariants. For the chosen models, this matrix takes a special form that allows us to invert it for arbitrary size and thereby explicitly calculate the weights of this average. For the identity seed we find that the weights are positive for all N, consistent with each model being dual to an ensemble average over CFT’s.en_US
dc.language.isoenen_US
dc.publisherSpringer Natureen_US
dc.subjectAdS-CFT Correspondenceen_US
dc.subjectConformal Field Theoryen_US
dc.subjectModels of Quantum Gravityen_US
dc.subjectChern-Simons Theoriesen_US
dc.subject2021-AUG-WEEK5en_US
dc.subjectTOC-AUG-2021en_US
dc.subject2021en_US
dc.titleAdS3 gravity and RCFT ensembles with multiple invariantsen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitleJournal of High Energy Physicsen_US
dc.publication.originofpublisherForeignen_US
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