3D flat holography: entropy and logarithmic corrections

dc.contributor.authorBAGCHI, ARJUNen_US
dc.contributor.authorBasu, Rudranilen_US
dc.contributor.departmentDept. of Physicsen_US
dc.date.accessioned2019-02-25T09:03:47Z
dc.date.available2019-02-25T09:03:47Z
dc.date.issued2014-03en_US
dc.description.abstractWe compute the leading corrections to the Bekenstein-Hawking entropy of the Flat Space Cosmological (FSC) solutions in 3D flat spacetimes, which are the flat analogues of the BTZ black holes in AdS3. The analysis is done by a computation of density of states in the dual 2D Galilean Conformal Field Theory and the answer obtained by this matches with the limiting value of the expected result for the BTZ inner horizon entropy as well as what is expected for a generic thermodynamic system. Along the way, we also develop other aspects of holography of 3D flat spacetimes.en_US
dc.identifier.citationJournal of High Energy Physics , 1403, 20.en_US
dc.identifier.issn1126-6708en_US
dc.identifier.issn1029-8479en_US
dc.identifier.sourcetitleJournal of High Energy Physicsen_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/2022
dc.identifier.urihttps://doi.org/10.1007/JHEP03(2014)020
dc.language.isoenen_US
dc.publication.originofpublisherForeignen_US
dc.publisherSpringer Natureen_US
dc.subjectGauge-gravity correspondenceen_US
dc.subjectConformalen_US
dc.subjectW Symmetryen_US
dc.subject3D flat holographyen_US
dc.subjectlogarithmic correctionsen_US
dc.subject2014en_US
dc.title3D flat holography: entropy and logarithmic correctionsen_US
dc.typeArticleen_US

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