Singularities and isotropy in a Brans-Dicke Bianchi-type VII universe

dc.creatorNúñez-Yépez, H. N.
dc.date1998-10-02
dc.date.accessioned2026-07-07T03:32:41Z
dc.date.available2026-07-07T03:32:41Z
dc.descriptionWe study the dynamical effects in the scale factors due to the scalar $ϕ$-field at the early stages of a supposedly anisotropic Universe expansion in connection with the problem of the initial singularity in the scalar-tensor cosmology of Jordan-Brans-Dicke. This is done by considering the behaviour of the general analytical solutions for the homogeneous model of Bianchi type VII in the vacuum case. We conclude that the Bianchi-VII$_0$ model shows an isotropic expansion and that its only physical solution is equivalent to a Friedman-Robertson-Walker spacetime whose evolution begins in a singularity and ends in another; moreover, we obtain that the general Bianchi-VII$_h$ (with $h\neq 0$) models show strong curvature singularities that produces a complete collapse of the homogeinity surfaces to a 2-plane, to a string-like one-dimensional manifold, or to a single point.
dc.description12 pages, 3 figures submitted to Gen. Rel. Grav
dc.identifierhttps://arxiv.org/abs/gr-qc/9810008
dc.identifierhttp://arxiv.org/abs/gr-qc/9810008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36327
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSingularities and isotropy in a Brans-Dicke Bianchi-type VII universe
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