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Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/1676
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dc.contributor.authorAfshar, Hamiden_US
dc.contributor.authorBAGCHI, ARJUNen_US
dc.contributor.authorFareghbal, Rezaen_US
dc.contributor.authorGrumiller, Danielen_US
dc.contributor.authorRosseel, Janen_US
dc.date.accessioned2019-02-14T05:02:29Z-
dc.date.available2019-02-14T05:02:29Z-
dc.date.issued2013-09en_US
dc.identifier.citationPhysical Review Letters, 111(12), 121603.en_US
dc.identifier.issn0031-9007en_US
dc.identifier.issn1079-7114)en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/1676-
dc.identifier.urihttps://doi.org/10.1103/PhysRevLett.111.121603en_US
dc.description.abstractWe present the first example of a nontrivial higher spin theory in three-dimensional flat space. We propose flat-space boundary conditions and prove their consistency for this theory. We find that the asymptotic symmetry algebra is a (centrally extended) higher spin generalization of the Bondi-Metzner-Sachs algebra, which we describe in detail. We also address higher spin analogues of flat space cosmology solutions and possible generalizations.en_US
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.subjectSpin-3 Gravityen_US
dc.subjectThree-Dimensionalen_US
dc.subjectFlat Spaceen_US
dc.subjectSpace cosmologyen_US
dc.subject2013en_US
dc.titleSpin-3 Gravity in Three-Dimensional Flat Spaceen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitlePhysical Review Lettersen_US
dc.publication.originofpublisherForeignen_US
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