Inflation in Models with Large Extra Dimensions Driven by a Bulk Scalar Field

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dc.creatorMohapatra, R. N.
dc.creatorPérez-Lorenzana, A.
dc.creatorPires, C. A. de S.
dc.date2000-03-09
dc.date2000-09-01
dc.date.accessioned2026-07-07T11:09:01Z
dc.date.available2026-07-07T11:09:01Z
dc.descriptionWe discuss inflation in models with large extra dimensions, driven by a bulk scalar field. The brane inflaton is then a single effective field, obtained from the bulk scalar field by scaling. The self interaction terms of the effective brane inflaton are then naturally suppressed. The picture is consistent with a fundamental string scale in the TeV range without the problem of a superlight inflaton. If hybrid inflation is considered, the right prediction for the density perturbations as observed by COBE can be obtained without any fine tunning. The bulk inflaton then decays preferentially into brane Higgses and reheating follows.
dc.description6 pages, LaTeX file, no figures. Minor changes. Final version to appear in Phys. Rev D
dc.identifierhttps://arxiv.org/abs/hep-ph/0003089
dc.identifierhttp://arxiv.org/abs/hep-ph/0003089
dc.identifierPhys.Rev.D62:105030,2000
dc.identifierdoi:10.1103/PhysRevD.62.105030
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/190328
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleInflation in Models with Large Extra Dimensions Driven by a Bulk Scalar Field
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