Bianchi type-III dark energy model in f(R,T) gravity

Reddy, D.R.K.; Santhi Kumar, R.; Pradeep Kumar, T.V.

doi:10.1007/s10773-012-1325-1

Bianchi type-III dark energy model in f(R,T) gravity

2013

7 pages

Published in:

Int.J.Theor.Phys. 52 (2013) 239-245

DOI:

10.1007/s10773-012-1325-1

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Abstract: (Springer)

A dark energy model with EoS parameter is investigated in f(R,T) gravity in Bianchi type-III space-time in the presence of perfect fluid source. To obtain a determinate solution special law of variation for Hubbles parameter proposed by Berman (Nuovo Cimento B 74:183, 1983) is used. We have also assumed that the scalar expansion is proportional to shear and the EoS parameter is proportional to skewness parameter. It is observed that the EoS parameter, skewness parameters in the model turn out to be functions of cosmic time. Some physical and kinematical properties of the model are also discussed.

Dark energy
Bianchi Type-III model
f(R,T) gravity

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