Warm inflation on the brane

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dc.creatorCid, M. Antonella
dc.creatordel Campo, Sergio
dc.creatorHerrera, Ramon
dc.date2007-10-16
dc.date.accessioned2026-07-07T11:38:09Z
dc.date.available2026-07-07T11:38:09Z
dc.descriptionIn this paper, warm inflationary models on a brane scenario are studied. Here we consider slow-roll inflation and high-dissipation regime in a high-energy scenario. General conditions required for these models to be realizable are derived. We describe scalar and tensor perturbations for these scenarios. Specifically we study power-law potentials considering a dissipation parameter to be a constant on the one hand and $ϕ$ dependent on the other hand. We use recent astronomical observations to restrict the parameters appearing in our model.
dc.description20 pages and 2 figures
dc.identifierhttps://arxiv.org/abs/0710.3148
dc.identifierhttp://arxiv.org/abs/0710.3148
dc.identifierJCAP0710:005,2007
dc.identifierdoi:10.1088/1475-7516/2007/10/005
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/199462
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleWarm inflation on the brane
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