The holographic entropy increases in quadratic curvature gravity

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dc.contributor.author Bhattacharjee, Srijit
dc.contributor.author Sarkar, Sudipta
dc.contributor.author Wall, Aron C.
dc.date.accessioned 2015-05-03T14:02:17Z
dc.date.available 2015-05-03T14:02:17Z
dc.date.issued 2015-04
dc.identifier.citation Bhattacharjee, Srijit; Sarkar, Sudipta and Wall, Aron C., “The holographic entropy increases in quadratic curvature gravity”, arXiv, Cornell University Library, DOI: arXiv:1504.04706, Apr. 2015. en_US
dc.identifier.uri https://repository.iitgn.ac.in/handle/123456789/1724
dc.description.abstract Standard methods for calculating the black hole entropy beyond general relativity are ambiguous when the horizon is non stationary. We fix these ambiguities in all quadratic curvature gravity theories, by demanding that the entropy be increasing at every time, for linear perturbations to a stationary black hole. Our result matches with the entropy formula found previously in holographic entanglement entropy calculations. We explicitly calculate the entropy increase for Vaidya-like solutions in Ricci-tensor gravity to show that (unlike the Wald entropy) the holographic entropy obeys a Second Law. en_US
dc.description.statementofresponsibility by Srijit Bhattacharjee, Sudipta Sarkar and Aron C. Wall
dc.language.iso en en_US
dc.publisher Cornell University Library en_US
dc.subject Holographic entropy en_US
dc.subject Quadratic curvature gravity theory en_US
dc.title The holographic entropy increases in quadratic curvature gravity en_US
dc.type Preprint en_US


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