Higher Dimensional Bianchi Type-V Cosmological Models with Perfect Fluid and Dark Energy

被引：4

作者：

Adhav, K. S. ^{[1
]}

Bansod, A. S. ^{[1
]}

Munde, S. L. ^{[1
]}

Desale, M. S. ^{[1
]}

机构：

[1] St Gadge Baba Amravati Univ, Dept Math, Amravati, India

来源：

INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS | 2011年 / 50卷 / 08期

基金：

英国科研创新办公室;

关键词：

Bianchi type-V space-time; Perfect fluid; Dark energy; Higher dimensions; PROBE WMAP OBSERVATIONS; GALAXY REDSHIFT SURVEY; ACCELERATING COSMOLOGIES; DATA RELEASE; DENSITY;

D O I：

10.1007/s10773-011-0751-9

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We have studied the Bianchi type-V cosmological models with binary mixture of perfect fluid and dark energy in five dimensions. The perfect fluid is obeying the equation of state p=gamma rho with gamma a[0,1]. The dark energy is considered to be either the quintessence or the Chaplygin gas. The exact solutions of the Einstein's field equations are obtained in quadrature form.

引用

页码：2573 / 2581

页数：9

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