• BIANCHI TYPE III DARK ENERGY COSMOLOGICAL MODEL IN SCALAR TENSOR THEORY OF GRAVITATION
Abstract
Bianchi Type-III Dark Energy model with variable equation of state (EoS) parameter is resented in the scalar tensor theory of Gravitation proposed by Saez and Ballester (Phys. Lett. A 113:467, 1986). To get a determinate solution of the field equation we take the help of special law of variation for Hubble parameter presented by Barman which yields a cosmological model with negative constant deceleration parameter. Some physical and kinematical properties of model are also discussed.
Keywords
Scalar-Tensor theory. Dark energy, cosmological model.
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