Chaos in FRW cosmology with various types of a scalar field potential

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dc.creatorToporensky, A. V.
dc.date2000-11-30
dc.date.accessioned2026-07-07T03:25:27Z
dc.date.available2026-07-07T03:25:27Z
dc.descriptionThe results on chaos in FRW cosmology with a massive scalar field are extended to another scalar field potential. It is shown that for sufficiently steep potentials the chaos disappears. A simple and rather accurate analytical criterion for the chaos to disappear is given. On the contrary, for gently sloping potentials the transition to a strong chaotic regime can occur. Two examples, concerning asymptotically flat and Damour-Mukhanov potentials are given.
dc.description8 pages with 4 eps figures, submitted to the electronic proceedings of the 9-th Marcel Grossmann Meeting (Rome, 2-8 July, 2000)
dc.identifierhttps://arxiv.org/abs/gr-qc/0011113
dc.identifierhttp://arxiv.org/abs/gr-qc/0011113
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33720
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectChaotic Dynamics
dc.titleChaos in FRW cosmology with various types of a scalar field potential
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