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Phantom fields: bounce solutions in the early universe and s-branes

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dc.contributor.author Dzhunushaliev Vladimir
dc.contributor.author Folomeev Vladimir
dc.contributor.author Myrzakulov Kairat
dc.date.accessioned 2012-06-30T11:34:14Z
dc.date.available 2012-06-30T11:34:14Z
dc.date.issued 2012-06-30
dc.identifier.uri http://dspace.enu.kz/handle/data/989
dc.description.abstract The 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. en_US
dc.language.iso en en_US
dc.subject DE corresponds S-branes 4D scalar en_US
dc.title Phantom fields: bounce solutions in the early universe and s-branes en_US


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