Curvature in causal BD-type inflationary cosmology

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dc.creatorPena, Francisco
dc.creatorCataldo, Mauricio
dc.creatordel Campo, Sergio
dc.date2004-07-15
dc.date.accessioned2026-07-07T11:30:07Z
dc.date.available2026-07-07T11:30:07Z
dc.descriptionWe study a closed model of the universe filled with viscous fluid and quintessence matter components in a Brans-Dicke type cosmological model. The dynamical equations imply that the universe may look like an accelerated flat Friedmann-Robertson-Walker universe at low redshift. We consider here dissipative processes which follow a causal thermodynamics. The theory is applied to viscous fluid inflation, where accepted values for the total entropy in the observable universe is obtained.
dc.description11 pages, revtex 4. For a festschrift honoring Alberto Garcia. To be publishen in Gen. Rel. Grav
dc.identifierhttps://arxiv.org/abs/gr-qc/0407061
dc.identifierhttp://arxiv.org/abs/gr-qc/0407061
dc.identifierGen.Rel.Grav.37:803-811,2005
dc.identifierdoi:10.1007/s10714-005-0064-5
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196921
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleCurvature in causal BD-type inflationary cosmology
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