A FRW Dark Fluid with a Non-Linear Inhomogeneous Equation of State

Abstract

A dark Friedman-Robertson-Walker fluid governed by a non-linear inhomogeneous equation of state is considered which can be viewed as a conveniently simple paradigm for a whole class of models which exhibit phase transitions from a non-phantom towards a phantom era (superacceleration transition). From another side, such dark fluid models may describe also quintessence-like cosmic acceleration. Thermodynamical considerations for the processes involved, which are of great importance in the characterization of the global evolution of the corresponding universe, are given too. Connecting the proposed equation of state with an anisotropic Kasner universe with viscosity, we are led to the plausible conjecture of a dark fluid origin of the anisotropies in the early universe.

11 pages pdf, 2 figures; to appear in Eur. Phys. J. C

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• Little Rip cosmological models with time-dependent equation of state
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• Inhomogeneous Dark Fluid and Dark Matter, Leading to a Bounce Cosmology
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