Regular Article - Theoretical Physics
Locally rotationally symmetric Bianchi type I cosmology in f(R, T) gravity
Department of Sciences and Humanities, National University of Computer and Emerging Sciences, Lahore Campus, Lahore, Pakistan
* e-mail: firstname.lastname@example.org
Accepted: 9 July 2015
Published online: 4 August 2015
This manuscript is devoted to the investigation of the Bianchi type I universe in the context of f(R, T) gravity. For this purpose, we explore the exact solutions of locally rotationally symmetric Bianchi type I spacetime. The modified field equations are solved by assuming an expansion scalar proportional to the shear scalar , which gives , where A, B are the metric coefficients and n is an arbitrary constant. In particular, three solutions have been found and physical quantities are calculated in each case.
© The Author(s), 2015