Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/2261
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dc.contributor.authorAfshar, Hamiden_US
dc.contributor.authorBAGCHI, ARJUNen_US
dc.contributor.authorDetournay, S.en_US
dc.contributor.authorGrumiller, Danielen_US
dc.contributor.authorProhazka, S.en_US
dc.contributor.authorRiegler, Maxen_US
dc.date.accessioned2019-03-15T11:25:58Z
dc.date.available2019-03-15T11:25:58Z
dc.date.issued2014-11en_US
dc.identifier.citationLecture Notes in Physics, 892.en_US
dc.identifier.issn0075-8450en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/2261-
dc.identifier.urihttps://doi.org/10.1007/978-3-319-10070-8__12en_US
dc.description.abstractChern–Simons theories in three dimensions are topological field theories that may have a holographic interpretation for suitable chosen gauge groups and boundary conditions on the fields. Conformal Chern–Simons gravity is a topological model of three-dimensional gravity that exhibits Weyl invariance and allows various holographic descriptions, including Anti-de Sitter, Lobachevsky and flat space holography. The same model also allows to address some aspects that arise in higher spin gravity in a considerably simplified setup, since both types of models have gauge symmetries other than diffeomorphisms. In these lectures we summarize briefly recent results.en_US
dc.language.isoenen_US
dc.publisherSpringer Natureen_US
dc.subjectPartition Functionen_US
dc.subjectCentral Chargeen_US
dc.subjectHigh Spinen_US
dc.subjectMassive Gravityen_US
dc.subjectAsymptotic Symmetryen_US
dc.subject2014en_US
dc.subjectBook chapteren_US
dc.subject2015en_US
dc.titleHolographic Chern-Simons Theoriesen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitleLecture Notes in Physicsen_US
dc.publication.originofpublisherForeignen_US
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