Two-Fluid Cosmological Models in Bianchi Type-V Space-Time

被引：12

作者：

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

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

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

Raut, R. B. ^{[1
]}

机构：

[1] Sant Gadge Baba Amravati Univ, Dept Math, Amravati 444602, India

来源：

INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS | 2011年 / 50卷 / 06期

关键词：

Bianchi type-V space-time; Two fluids; VARIABLE-G; LAMBDA; SUPERNOVAE; CONSTANT; UNIVERSE; OMEGA;

D O I：

10.1007/s10773-011-0699-9

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We have presented anisotropic, homogeneous two-fluid cosmological models using Bianchi type-V space-time. Here one fluid represents the matter content of the universe and another fluid is chosen to model the CMB radiation. The radiation and matter content of the universe are in interactive phase. Also we have discussed the behavior of fluid parameters and kinematical parameters.

引用

页码：1846 / 1851

页数：6

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