Ruppeiner theory of black hole thermodynamics

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dc.creatorAman, Jan E
dc.creatorBedford, James
dc.creatorGrumiller, Daniel
dc.creatorPidokrajt, Narit
dc.creatorWard, John
dc.date2006-11-22
dc.date.accessioned2026-07-07T11:21:32Z
dc.date.available2026-07-07T11:21:32Z
dc.descriptionThe Ruppeiner metric as determined by the Hessian of the Gibbs surface provides a geometric description of thermodynamic systems in equilibrium. An interesting example is a black hole in equilibrium with its own Hawking radiation. In this article, we present results from the Ruppeiner study of various black hole families from different gravity theories e.g. 2D dilaton gravity, BTZ, general relativity and higher-dimensional Einstein-Maxwell gravity.
dc.description10 pages, 1 figure. Talk given by N Pidokrajt at ERE2006 in Palma de Mallorca, Spain
dc.identifierhttps://arxiv.org/abs/gr-qc/0611119
dc.identifierhttp://arxiv.org/abs/gr-qc/0611119
dc.identifierJ.Phys.Conf.Ser.66:012007,2007
dc.identifierdoi:10.1088/1742-6596/66/1/012007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194292
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleRuppeiner theory of black hole thermodynamics
dc.typetext

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