Thermodynamics of horizons from a dual quantum system

dc.creatorSarkar, Sudipta
dc.creatorPadmanabhan, T.
dc.date2006-07-11
dc.date.accessioned2026-07-07T12:53:43Z
dc.date.available2026-07-07T12:53:43Z
dc.descriptionIt was shown recently that, in the case of Schwarschild black hole, one can obtain the correct thermodynamic relations by studying a model quantum system and using a particular duality transformation. We study this approach further for the case a general spherically symmetric horizon. We show that the idea works for a general case only if we define the entropy S as a congruence ("observer") dependent quantity and the energy E as the integral over the source of the gravitational acceleration for the congruence. In fact, in this case, one recovers the relation S=E/2T between entropy, energy and temperature previously proposed by one of us in gr-qc/0308070. This approach also enables us to calculate the quantum corrections of the Bekenstein-Hawking entropy formula for all spherically symmetric horizons.
dc.description5 pages; no figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0607042
dc.identifierhttp://arxiv.org/abs/gr-qc/0607042
dc.identifierEntropy 9:100-107,2007
dc.identifierdoi:10.3390/e9030100
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/223719
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThermodynamics of horizons from a dual quantum system
dc.typetext

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