Dark Energy Cosmological Model in a Modified Theory of Gravity

被引：28

作者：

Chirde, V. R. ^{[1
]}

Shekh, S. H. ^{[2
]}

机构：

[1] GSG Mahavidyalaya, Dept Math, Umarkhed 445206, India

[2] Dr BN Coll Engn & Tech, Dept Math, Yavatmal 445001, India

来源：

ASTROPHYSICS | 2015年 / 58卷 / 01期

关键词：

Non-static plane symmetric metric: f(R; T) gravity: Dark Energy; BIANCHI TYPE-I; CHAPLYGIN-GAS; ACCELERATING UNIVERSE; F(R; T); THEORY; PHANTOM; REDSHIFT; CONSTRAINTS; SUPERNOVAE; QUANTUM; OMEGA;

D O I：

10.1007/s10511-015-9369-6

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The dark energy model with equation of state (EoS) parameter is derived for a non-static plane symmetric space-time filled with a perfect fluid source in the framework of f (R, T) gravity (Harko et al., arXiv: 1104.2669v2 [gr-qc], 2011). To obtain a determinate solution, a special form of deceleration parameter (DP) is used. We have assumed that the relation between metric potentials and the EoS parameter is proportional to the skewness parameter. It is observed that the EoS parameter, and the skewness parameter 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：106 / 119

页数：14

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