de Sitter Thermodynamics: A glimpse into non equilibrium

dc.creatorAros, Rodrigo
dc.date2008-01-30
dc.date2008-02-11
dc.date.accessioned2026-07-07T11:55:42Z
dc.date.available2026-07-07T11:55:42Z
dc.descriptionIn this article is shown that the thermodynamical evolution of a Schwarzschild de Sitter space is the evaporation of its black hole. The result is extended in higher dimensions to Lovelock theories of gravity with a single positive cosmological constant.
dc.identifierhttps://arxiv.org/abs/0801.4591
dc.identifierhttp://arxiv.org/abs/0801.4591
dc.identifierPhys.Rev.D77:104013,2008
dc.identifierdoi:10.1103/PhysRevD.77.104013
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/205332
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titlede Sitter Thermodynamics: A glimpse into non equilibrium
dc.typetext

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