Warm-Chaplygin inflationary universe model

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dc.creatordel Campo, Sergio
dc.creatorHerrera, Ramon
dc.date2008-06-03
dc.date.accessioned2026-07-07T12:14:39Z
dc.date.available2026-07-07T12:14:39Z
dc.descriptionWarm inflationary universe models in the context of a Chaplygin gas equation are studied. General conditions required for these models to be realizable are derived and discussed. By using a chaotic potential we develop models for a dissipation coefficient of the form $Γ\propto ϕ^n$, with $n=0$ or $n\neq 0$.
dc.description17 pages, 4 figures, Accepted for publication in Physics Letters B
dc.identifierhttps://arxiv.org/abs/0806.0575
dc.identifierhttp://arxiv.org/abs/0806.0575
dc.identifierPhys.Lett.B665:100-105,2008
dc.identifierdoi:10.1016/j.physletb.2008.05.063
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/211264
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titleWarm-Chaplygin inflationary universe model
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