QUASI-RIP UNIVERSE INDUCED BY THE FLUID WITH INHOMOGENEOUS EQUATION OF STATE.
We investigate a specic model for a dark energy which lead to the Quasi-Rip cosmology. In the Quasi-Rip model the equation of state parameter w is less than -1 in the rst 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.
Keywords: dark energy, cosmological constant, equation of state, bound structures
Issue: 13, 2012
Pages: 42 — 44
Downloads: 977