Bianchi type-III Dark Energy Model in f(R,T) Gravity

被引：67

作者：

Reddy, D. R. K. ^{[1
]}

Kumar, R. Santhi ^{[2
]}

Kumar, T. V. Pradeep ^{[3
]}

机构：

[1] MVGR Coll Engn, Dept Sci & Humanities, Vizianagaram, India

[2] Aditya Inst Technol, Dept Basic Sci & Humanities, Tekkali, India

[3] Acharya Nagarjuna Univ, Coll Engn & Technol, Dept Math, Guntur, India

来源：

INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS | 2013年 / 52卷 / 01期

关键词：

Dark energy; Bianchi Type-III model; f; (R; T); gravity; SCALAR-TENSOR THEORY; EQUATION; LAMBDA; LAW;

D O I：

10.1007/s10773-012-1325-1

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

A dark energy model with EoS parameter is investigated in f(R,T) gravity in Bianchi type-III space-time in the presence of perfect fluid source. To obtain a determinate solution special law of variation for Hubble's parameter proposed by Berman (Nuovo Cimento B 74:183, 1983) is used. We have also assumed that the scalar expansion is proportional to shear and the EoS parameter is proportional to skewness parameter. It is observed that the EoS parameter, skewness parameters in the model turn out to be functions of cosmic time. Some physical and kinematical properties of the model are also discussed.

引用

页码：239 / 245

页数：7

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