Bianchi Type VI0 Cosmological Models with Perfect Fluid and Dark Energy

被引：3

作者：

Katore, S. D. ^{[1
]}

Kapse, D. V. ^{[1
]}

Tayade, G. B. ^{[1
]}

机构：

[1] SGB Amravati Univ, Dept Math, Amravati 444602, India

来源：

INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS | 2011年 / 50卷 / 11期

关键词：

Cosmological models; Perfect fluid; Dark energy; Cosmological parameters; PROBE WMAP OBSERVATIONS; QUINTOM MODEL; COSMIC COINCIDENCE; CONSTRAINTS; QUINTESSENCE; PHANTOM; CONSEQUENCES; SUPERNOVAE; EQUATION; UNIVERSE;

D O I：

10.1007/s10773-011-0832-9

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We consider a self-consistent system of Bianchi Type VI0 cosmology and binary mixture of perfect fluid and dark energy. The perfect fluid is taken to be one obeying the usual equation of state p=gamma rho with gamma a[0,1]. The dark energy is considered to be either the quintessence or Chaplygin gas. Exact solutions to the corresponding Einstein's field equations are obtained as a quadrature. Models with power-law and exponential expansion have discussed in detail.

引用

页码：3299 / 3312

页数：14

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