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

被引：199

作者：

Nojiri, Shin'ichi ^{[1
]}

Odintsov, Sergei D.

机构：

[1] Nagoya Univ, Dept Phys, Nagoya, Aichi 4648602, Japan

[2] Fac Ciencias, ICREA, E-08193 Bellaterra, Barcelona, Spain

[3] Fac Ciencias, CSIC, IEEC, Inst Ciencies Espai, E-08193 Bellaterra, Barcelona, Spain

[4] Tomsk State Pedag Univ, Lab Fundamental Studies, Tomsk, Russia

来源：

PHYSICS LETTERS B | 2006年 / 639卷 / 3-4期

关键词：

D O I：

10.1016/j.physletb.2006.06.065

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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. (c) 2006 Elsevier B.V. All rights reserved.

引用

页码：144 / 150

页数：7

共 56 条

[11] Observational constraints on dark energy with generalized equations of state [J].