Brane-cosmology dynamics with induced gravity

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dc.creatorGumjudpai, Burin
dc.date2003-08-14
dc.date2003-10-26
dc.date.accessioned2026-07-07T11:08:41Z
dc.date.available2026-07-07T11:08:41Z
dc.descriptionThe Friedmann equations for a brane with induced gravity are analyzed and compared with the standard general relativity and Randall-Sundrum cases. Randall-Sundrum gravity modified the early universe dynamics, whereas induced gravity changes the late universe evolution. The early and late time limits are investigated. Induced gravity effects can contribute to late-universe acceleration. This conditions for this are found. Qualitative analysis is given for a range of scalar field potentials.
dc.description14 pages, 25 eps figures, higher-resolution figures can be obtained from the author. Minor corrections. To appear in Gen.Rel.Grav. 36 (2004)
dc.identifierhttps://arxiv.org/abs/gr-qc/0308046
dc.identifierhttp://arxiv.org/abs/gr-qc/0308046
dc.identifierGen.Rel.Grav.36:747-766,2004
dc.identifierdoi:10.1023/B:GERG.0000016922.72972.67
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/190220
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titleBrane-cosmology dynamics with induced gravity
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