2016/01/04 by J. K. Singh, Sarita Rani
Physics and Astronomy · #gr-qc
paper · pdf · doi:10.1134/s0040577917120121
17 pages, 11 figures. arXiv admin note: text overlap with arXiv:1206.0391 by other authors
arxiv created 2016/01/04 · arxiv updated 2018/02/14
This paper deals with a spatially homogeneous and totally anisotropic Bianchi type-V cosmological model within the framework of self interacting Brans Dicke theory of gravity in the background of anisotropic dark energy (DE) with variable equation of state (EoS) parameter and constant deceleration parameter. Constant deceleration parameter leads to two models of universe, i.e. power law model and exponential model. EoS parameter ω and its existing range for the models is in good agreement with the most recent observational data. We notice that ω given by (37) i.e ω(t) = log(k1t) is more suitable in explaining the evolution of the universe. The physical behaviors of the solutions have also been discussed using some physical quantities. Finally, we observe that despite having several prominent features, both of the DE models discussed fail in details.