Anisotropic Dark Energy Bianchi Type III Cosmological Models in Brans Dicke Theory of Gravity

Abstract

The main purpose of this paper is to explore the solutions of Bianchi type $III$ cosmological model in Brans Dicke theory of gravity in the background of anisotropic dark energy. We use the assumption of constant deceleration parameter and power law relation between scalar field $\varphi$ and scale factor $a$ to find the solutions. The physical behavior of the solutions has been discussed using some physical quantities.

14 pages, accepted for publication in Canadian Journal of Physics. arXiv admin note: substantial text overlap with arXiv:0910.5787

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Cited by in corpus (3)

• Killing and Noether Symmetries of Plane Symmetric Spacetime
• Effects of anisotropy on interacting ghost dark energy in Brans-Dicke theories
• Bulk viscous cosmological model in Brans Dicke theory with new form of time varying deceleration parameter