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

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

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Cited by in corpus (8)

• Thick brane solutions
• Bouncing cosmological solutions from f(R,T) gravity
• A non-singular bouncing cosmology in $f(R,T)$ gravity
• Hairy Kiselev Black Hole Solutions
• Anti-de-Sitter Island-Universes from 5D Standing Waves
• Star-plus-wormhole systems with two interacting scalar fields
• 4D static solutions with interacting phantom fields
• Compact and extended objects from self-interacting phantom fields