Rip Cosmology via Inhomogeneous Fluid
arXiv:1309.4553 · doi:10.3390/galaxies1020107
Abstract
The conditions for the appearance of the Little Rip, Pseudo Rip and Quasi Rip universes in the terms of the parameters in the equation of state of some dark fluid are investigated. Several examples of the Rip cosmologies are investigated.
107-113
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