The new form of the equation of state for dark energy fluid and accelerating universe

Details The new form of the equation of state for dark energy fluid and accelerating universe The new form of the equation of state for dark energy fluid and accelerating universe

2006-06-04

arxiv.org/abs/hep-th/0606025v2

Phys.Lett.B639:144-150,2006

Physics

High Energy Physics

High Energy Physics - Theory

LaTeX file, 9 pages, extended version, to appear in PLB

Scientific paper

10.1016/j.physletb.2006.06.065

We suggest to generalize the dark energy equation of state (EoS) by introduction the relaxation equation for pressure which is equivalent to consideration of the inhomogeneous EoS cosmic fluid which often appears as the effective model from strings/brane-worlds. As another, more wide generalization we discuss the inhomogeneous EoS which contains derivatives of pressure. For several explicit examples motivated by the analogy with classical mechanics the accelerating FRW cosmology is constructed. It turns out to be the asymptotically de Sitter or oscillating universe with possible transition from deceleration to acceleration phase. The coupling of dark energy with matter in accelerating FRW universe is considered, it is shown to be consistent with constrained (or inhomogeneous) EoS.

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