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

Vladimir Dzhunushaliev·Vladimir Folomeev·Kairat Myrzakulov·Ratbay Myrzakulov
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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.

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Vladimir Dzhunushaliev, Vladimir Folomeev, Kairat Myrzakulov, Ratbay Myrzakulov. 2007-04-17. Phantom fields: bounce solutions in the early Universe and S-branes. https://doi.org/10.1142/s0218271808013911

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