Inflationary attractor in Gauss-Bonnet brane cosmology

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dc.creatorMeng, Xin-He
dc.creatorWang, Peng
dc.date2003-12-09
dc.date2004-01-25
dc.date.accessioned2026-07-07T11:09:28Z
dc.date.available2026-07-07T11:09:28Z
dc.descriptionThe inflationary attractor properties of the canonical scalar field and Born-Infeld field are investigated in the Randall-Sundrum II scenario with a Gauss-Bonnet term in the bulk action. We find that the inflationary attractor property will always hold for both the canonical and Born-Infeld fields for any allowed non-negative Gauss-Bonnet coupling. We also briefly discuss the possibility of explaining the suppressed lower multiples and running scalar spectral index simultaneously in the scenario of Gauss-Bonnet brane inflation.
dc.description7 pages, no figures. An error in the discussion of BI field corrected, conclusion corrected
dc.identifierhttps://arxiv.org/abs/hep-ph/0312113
dc.identifierhttp://arxiv.org/abs/hep-ph/0312113
dc.identifierClass.Quant.Grav.21:2527-2536,2004
dc.identifierdoi:10.1088/0264-9381/21/11/001
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/190479
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleInflationary attractor in Gauss-Bonnet brane cosmology
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