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1 | 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 | 980 |