Journal
INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS
Volume 52, Issue 1, Pages 239-245Publisher
SPRINGER/PLENUM PUBLISHERS
DOI: 10.1007/s10773-012-1325-1
Keywords
Dark energy; Bianchi Type-III model; f (R, T) gravity
Categories
Ask authors/readers for more resources
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 Hubble's 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.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available