Quasi-Rip universe induced by the fluid with inhomogeneous equation of state
Brevik, I. · Obukhov, V. · Timoshkin, A.
Original · EN
We investigate a specific model for dark energy, which lead to the Quasi-Rip cosmology. In the Quasi-Rip model, the equation of the state parameter w is less than -1 in the first stage, but then in the second stage is larger than -1. The conditions for the appearance the Quasi-Rip in the terms of the parameters equation of state are received.
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