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Bianchi type-III Dark Energy Model in f(R,T) Gravity |
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| Authors: | D R K Reddy R Santhi Kumar T V Pradeep Kumar |
| Institution: | 1. Department of Science and Humanities, MVGR College of Engineering, Vizianagaram, India 2. Department of Basic Science and Humanities, Aditya Institute of Technology, Tekkali, India 3. Dept. of Mathematics, Acharya Nagarjuna University College of Engineering and Technology, Guntur, India |
| Abstract: | 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. |
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