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Bianchi Type-III Dark Energy Model in f(R,T) gravity with a variable Deceleration parameter

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.

preprint2016arXivOpen access
D. R. K. ReddyG. RameshS. Umadevi
physics.gen-ph
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Open access3 authors1 topic
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D. R. K. ReddyG. RameshS. Umadevi

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