Black hole entropy: quantum vs thermal fluctuations

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dc.creatorChatterjee, Ashok
dc.creatorMajumdar, Parthasarathi
dc.date2003-03-07
dc.date.accessioned2026-07-07T03:27:42Z
dc.date.available2026-07-07T03:27:42Z
dc.descriptionThe relation between logarithmic corrections to the area law for black hole entropy, due to thermal fluctuations around an equilibrium canonical ensemble, and those originating from quantum spacetime fluctuations within a microcanonical framework, is explored for three and four dimensional asymptotically anti-de Sitter black holes. For the BTZ black hole, the two logarithmic corrections are seen to precisely cancel each other, while for four dimensional adS-Schwarzschild black holes a partial cancellation is obtained. We discuss the possibility of extending the analysis to asymptotically flat black holes.
dc.description11 Pages Revtex, no figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0303030
dc.identifierhttp://arxiv.org/abs/gr-qc/0303030
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34533
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBlack hole entropy: quantum vs thermal fluctuations
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