Bulk effects in the cosmological dynamics of brane-world scenarios

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dc.creatorCampos, Antonio
dc.creatorSopuerta, Carlos F.
dc.date2001-05-11
dc.date.accessioned2026-07-07T10:34:07Z
dc.date.available2026-07-07T10:34:07Z
dc.descriptionIn this paper we deal with the cosmological dynamics of Randall-Sundrum brane-world type scenarios in which the five-dimensional Weyl tensor has a non-vanishing projection onto the three-brane where matter fields are confined. Using dynamical systems techniques, we study how the state space of Friedmann-Lemaitre-Robertson-Walker (FLRW) and Bianchi type I cosmological models is affected by the bulk Weyl tensor, focusing in the differences that appear with respect to general relativity and also Randall-Sundrum cosmological scenarios without the Weyl tensor contribution.
dc.description13 pages, Revtex v3.0, 8 figures
dc.identifierhttps://arxiv.org/abs/hep-th/0105100
dc.identifierhttp://arxiv.org/abs/hep-th/0105100
dc.identifierPhys.Rev.D64:104011,2001
dc.identifierdoi:10.1103/PhysRevD.64.104011
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179364
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleBulk effects in the cosmological dynamics of brane-world scenarios
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