A causal model for a closed universe

Simple item page
dc.creatorCataldo, M.
dc.creatordel Campo, S.
dc.creatorMinning, P.
dc.creatorPena, F.
dc.date2003-12-17
dc.date.accessioned2026-07-07T11:32:14Z
dc.date.available2026-07-07T11:32:14Z
dc.descriptionWe study a closed model of a universe filled with viscous fluid and quintessence matter components. The dynamical equations imply that the universe might look like an accelerated flat Friedmann-Robertson-Walker (FRW) universe at low redshift. We consider here dissipative processes which obey a causal thermodynamics. Here, we account for the entropy production via causal dissipative inflation.
dc.description9 pages. Accepted for publication in IJMPD
dc.identifierhttps://arxiv.org/abs/hep-th/0312219
dc.identifierhttp://arxiv.org/abs/hep-th/0312219
dc.identifierInt.J.Mod.Phys.D13:871,2004
dc.identifierdoi:10.1142/S0218271804004943
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/197529
dc.subjectHigh Energy Physics - Theory
dc.titleA causal model for a closed universe
dc.typetext

Files

Collections

arXiv