Cardy-Verlinde Entropy Formula in the Presence of a General Cosmological State Equation

dc.creatorBrevik, I.
dc.date2002-04-04
dc.date.accessioned2026-07-07T12:29:07Z
dc.date.available2026-07-07T12:29:07Z
dc.descriptionAs recently found by Youm [hep-th/0201268], the entropy of the universe will no longer be expressible in the conventional Cardy-Verlinde form if one relaxes the radiation dominance state equation and instead assumes a more general equation of the form p=(γ-1)ρ, with γa constant. We show that Youm's generalized entropy formula remains valid when the cosmic fluid is no longer ideal, but is allowed to possess a constant bulk viscosity ζ. We supply our analysis with some numerical estimates, thus calculating the scale factor a(t) for a k=0 universe, and also calculate via a perturbative expansion in ζthe magnitude of the viscosity-induced correction to the scale factor if the universe is radiation dominated.
dc.description10 pages, LaTeX, no figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0204021
dc.identifierhttp://arxiv.org/abs/gr-qc/0204021
dc.identifierPhys.Rev.D65:127302,2002
dc.identifierdoi:10.1103/PhysRevD.65.127302
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/215770
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleCardy-Verlinde Entropy Formula in the Presence of a General Cosmological State Equation
dc.typetext

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