Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/3131
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dc.contributor.authorMALVIMAT, VINAYen_US
dc.contributor.authorMondal, Sayiden_US
dc.contributor.authorSengupta, Gautamen_US
dc.date.accessioned2019-06-26T04:00:25Z
dc.date.available2019-06-26T04:00:25Z
dc.date.issued2019-05en_US
dc.identifier.citationJournal of High Energy Physics, 2019(5).en_US
dc.identifier.issn1029-8479en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/3131-
dc.identifier.urihttps://doi.org/10.1007/JHEP05(2019)183en_US
dc.description.abstractWe investigate the time evolution of entanglement negativity following a global quench for mixed state configurations of two disjoint and adjacent intervals in a (1 + 1)-dimensional conformal field theory (CFT1+1) dual to the eternal black hole sliced in half by an end of the world brane, through the AdS3/CFT2 correspondence. To this end we obtain the time evolution of the holographic entanglement negativity for such mixed states from a dual bulk eternal black hole geometry and elucidate the relevant geodesic structures. The holographic entanglement negativity for such mixed states, following a global quench is described by half of the results for the eternal black hole. Significantly our results exactly match with the corresponding CFT1+1 computations.en_US
dc.language.isoenen_US
dc.publisherSpringer Natureen_US
dc.subjectAdS-CFT Correspondenceen_US
dc.subjectGauge-gravity correspondenceen_US
dc.subjectTOC-JUN-2019en_US
dc.subject2019en_US
dc.titleTime evolution of entanglement negativity from black hole interiorsen_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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