Bianchi type I model with two interacting scalar fields

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dc.creatorFolomeev, Vladimir
dc.date2007-03-01
dc.date.accessioned2026-07-07T11:21:48Z
dc.date.available2026-07-07T11:21:48Z
dc.descriptionThe flat anisotropic model of the early Universe is considered. Two interacting scalar fields with special form of potential energy are a source of matter fields. Analytic solutions for inflationary and scalaron stages are found. It is shown that the solutions tend asymptotically to isotropic Friedmann model.
dc.description6 pages, 1 figure
dc.identifierhttps://arxiv.org/abs/gr-qc/0703004
dc.identifierhttp://arxiv.org/abs/gr-qc/0703004
dc.identifierInt.J.Mod.Phys.D16:1845-1852,2007
dc.identifierdoi:10.1142/S0218271807011139
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194371
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBianchi type I model with two interacting scalar fields
dc.typetext

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