Phantom fields: bounce solutions in the early Universe and S-branes

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dc.creatorDzhunushaliev, Vladimir
dc.creatorFolomeev, Vladimir
dc.creatorMyrzakulov, Kairat
dc.creatorMyrzakulov, Ratbay
dc.date2006-08-04
dc.date2007-04-17
dc.date.accessioned2026-07-07T12:39:59Z
dc.date.available2026-07-07T12:39:59Z
dc.descriptionThe cosmological model with two phantom scalar fields with the special choice of field's potential is considered. The obtained regular solution describes a bounce with a subsequent transition to the de Sitter stage of the expansion of the Universe. This solution also could be interpreted as a S-brane solution.
dc.descriptionone reference and new interpretation of the solution are added, and the title is changed
dc.identifierhttps://arxiv.org/abs/gr-qc/0608025
dc.identifierhttp://arxiv.org/abs/gr-qc/0608025
dc.identifierInt.J.Mod.Phys.D17:2351-2358,2008
dc.identifierdoi:10.1142/S0218271808013911
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/219311
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titlePhantom fields: bounce solutions in the early Universe and S-branes
dc.typetext

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