Chaplygin inflation on the brane

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dc.creatorHerrera, Ramon
dc.date2008-05-07
dc.date.accessioned2026-07-07T11:33:46Z
dc.date.available2026-07-07T11:33:46Z
dc.descriptionBrane inflationary universe model in the context of a Chaplygin gas equation of state is studied. General conditions for this model to be realizable are discussed. In the high-energy limit and by using a chaotic potential we describe in great details the characteristic of this model. The parameters of the model are restricted by using recent astronomical observations.
dc.description13 pages, 2 figures, Accepted for publication in Physics Letters B
dc.identifierhttps://arxiv.org/abs/0805.1005
dc.identifierhttp://arxiv.org/abs/0805.1005
dc.identifierPhys.Lett.B664:149-153,2008
dc.identifierdoi:10.1016/j.physletb.2008.05.004
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198010
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titleChaplygin inflation on the brane
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