Bianchi V inflation in the Brans-Dicke theory?

dc.creatorCota, Jorge L. Cervantes
dc.date1999-12-10
dc.date.accessioned2026-07-07T12:01:27Z
dc.date.available2026-07-07T12:01:27Z
dc.descriptionIt is shown some exact solutions in the Brans-Dicke (BD) theory for a Bianchi V metric having the property of inflationary expansion, graceful exit, and asymptotic evolution to a Friedmann-Robertson-Walker (FRW) open model. It is remarkable that an inflationary behaviour can occur, even without a cosmological potential or constant. However, the horizon and flatness problems cannot be solve within the standard BD theory because the inflationary period is severely restricted by the value of the BD parameter $ω$.
dc.description28 pages, 6 figuras
dc.identifierhttps://arxiv.org/abs/gr-qc/9912047
dc.identifierhttp://arxiv.org/abs/gr-qc/9912047
dc.identifierClass.Quant.Grav.16:3903-3922,1999
dc.identifierdoi:10.1088/0264-9381/16/12/309
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/207102
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBianchi V inflation in the Brans-Dicke theory?
dc.typetext

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