Phantom fields: bounce solutions in the early Universe and S-branes
arXiv:gr-qc/0608025 · doi:10.1142/S0218271808013911
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.
one reference and new interpretation of the solution are added, and the title is changed