Bianchi Type-III Dark Energy Model in f(R,T) gravity with a variable Deceleration parameter
General Physics
2016-01-13 v1
Abstract
In this paper, we have investigated Bianchi Type-III Dark Energy Model in f(R,T) theory of gravity proposed by Harko et al. (Phys. Rev. D84 : 024020, 2011). To find a determinate solution of the field equations we have used (i) the fact that scalar expansion of the space-time is proportional to the shear scalar and (ii) a variable deceleration parameter given by Mishra et al. (Int. J. Theor. Phys. 52: 2546, 2013). Physical and kinematical properties of the model are also discussed. It is observed that our model is in agreement with the recent cosmological observations.
Cite
@article{arxiv.1601.02648,
title = {Bianchi Type-III Dark Energy Model in f(R,T) gravity with a variable Deceleration parameter},
author = {D. R. K. Reddy and G. Ramesh and S. Umadevi},
journal= {arXiv preprint arXiv:1601.02648},
year = {2016}
}