Black hole entropy in modified gravity models

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dc.creatorBriscese, F.
dc.creatorElizalde, E.
dc.date2007-08-02
dc.date2008-01-13
dc.date.accessioned2026-07-07T11:18:22Z
dc.date.available2026-07-07T11:18:22Z
dc.descriptionAn analysis of some modified gravity models, based on the study of pure Schwarzschild and of Schwarzschild-de Sitter black holes, and involving the use of the Noether charge method, is carried out. Corrections to the classical Einsteinian black hole entropy appear. It is shown explicitly how the condition of positive entropy can be used in order to constrain the viability of modified gravity theories.
dc.description5 pages, 3 figures, revtex file, version to appear in PRD
dc.identifierhttps://arxiv.org/abs/0708.0432
dc.identifierhttp://arxiv.org/abs/0708.0432
dc.identifierPhys.Rev.D77:044009,2008
dc.identifierdoi:10.1103/PhysRevD.77.044009
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193321
dc.subjectHigh Energy Physics - Theory
dc.titleBlack hole entropy in modified gravity models
dc.typetext

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