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

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

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ijtp...50..637s&link_type=abstract

International Journal of Theoretical Physics, Volume 50, Issue 3, pp.637-643

Physics

2

Scientific paper

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= 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.

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