Plane Symmetric Vacuum Bianchi Type III Cosmology in f(R) Gravity

被引：14
|
作者：
Shamir, M. Farasat [1 ]
机构：
[1] Natl Univ Comp & Emerging Sci, Lahore 54770, Pakistan
来源：
INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS | 2011年 / 50卷 / 03期
关键词：
f (R) gravity and Bianchi type III; STRING COSMOLOGY; MODELS;
D O I：
10.1007/s10773-010-0587-8
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
The main purpose of this paper is to study the exact solution of Bianchi type III spacetime in the context of metric f(R) gravity. The field equations are solved by taking expansion scalar theta proportional to shear scalar sigma which gives C=A (n) , where A and C are the metric coefficients. The physical behavior of the solution has been discussed using some physical quantities. Also, the function of the Ricci scalar is evaluated.
引用
收藏
页码：637 / 643
页数：7
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