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

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作者
M. Farasat Shamir
机构
[1] National University of Computer and Emerging Sciences,
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(; ) gravity and Bianchi type ;
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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 θ proportional to shear scalar σ which gives C=An, 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.
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页码:637 / 643
页数:6
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