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Bianchi Type-III Dark Energy Model in a Saez-Ballester Scalar-Tensor Theory |
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| Authors: | |
| Institution: | 1.Department of Basic Science and Humanities,GMR Institute of Technology,Rajam,India;2.Department of Science and Humanities,M.V.G.R. College of Engineering,Vizainagaram,India |
| Abstract: | In this paper, we investigate Bianchi type-III universe which has dynamical energy density. We introduce three different skewness parameters along spatial directions to quantify the deviation of pressure from isotropy. We also assume that the skewness parameters are time dependent. The Saez-Ballester (J. Phys. Lett. A 113:467, 1986) field equations have been solved by applying a variation law for generalized Hubble’s parameter given by Bermann (Nuovo Cimento B 74:182, 1983). Some physical and kinematical properties of dark energy model are discussed. |
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