Nonsingular multidimensional cosmologies with Lobachevsky spatial sections

dc.creatorBronnikov, K. A.
dc.date2004-10-23
dc.date.accessioned2026-07-07T03:29:06Z
dc.date.available2026-07-07T03:29:06Z
dc.descriptionExamples of nonsingular cosmological models are presented on the basis of exact solutions to multidimensional gravity equations. These examples involve pure imaginary scalar fields, or, in other terms, ``phantom'' fields with an unusual sign of the kinetic term in the Lagrangian. We show that, with such fields, hyperbolic nonsingular models with a cosmological bounce (unlike spherical and spatially flat models) emerge without special relations among the integration constants, i.e., without fine tuning. In such models, the extra-dimension scale factors as well as scalar fields evolve smoothly between different finite asymptotic values. Examples of theories which create phantom scalar fields are obtained from string-inspired multidimensional field models and from theories of gravity in integrable Weyl space-times.
dc.description10 pages, submitted to Proc. Int. School GAS04, Kiten, Bulgaria, June 10-16, 2004
dc.identifierhttps://arxiv.org/abs/gr-qc/0410119
dc.identifierhttp://arxiv.org/abs/gr-qc/0410119
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35085
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleNonsingular multidimensional cosmologies with Lobachevsky spatial sections
dc.typetext

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