Phantom fields: bounce solutions in the early Universe and S-branes
Reviewed by Pithpith:DKDYPDCCopen to challenge →
classification
gr-qc
keywords
solutionbouncefieldsphantomuniversechoiceconsideredcosmological
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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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