Phase space geometry in scalar-tensor cosmology

dc.creatorFaraoni, Valerio
dc.date2005-02-03
dc.date.accessioned2026-07-07T10:48:17Z
dc.date.available2026-07-07T10:48:17Z
dc.descriptionWe study the phase space of spatially homogeneous and isotropic cosmology in general scalar-tensor theories. A reduction to a two-dimensional phase space is performed when possible-in these situations the phase space is usually a two-dimensional curved surface embedded in a three-dimensional space and composed of two sheets attached to each other, possibly with complicated topology. The results obtained are independent of the choice of the coupling function of the theory and, in certain situations, also of the potential.
dc.description18 pages, 9 figures, latex, to appear in Ann. Phys. (NY)
dc.identifierhttps://arxiv.org/abs/gr-qc/0502015
dc.identifierhttp://arxiv.org/abs/gr-qc/0502015
dc.identifierAnn.Phys.317:366-382,2005
dc.identifierdoi:10.1016/j.aop.2004.11.009
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/183827
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titlePhase space geometry in scalar-tensor cosmology
dc.typetext

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