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

TL;DR

This paper investigates Bianchi type III cosmological models with anisotropic dark energy within Brans-Dicke gravity, deriving solutions under specific assumptions and analyzing their physical properties.

Contribution

It introduces new solutions for Bianchi type III models in Brans-Dicke theory with anisotropic dark energy, using constant deceleration and scalar-field scale factor relations.

Findings

Derived explicit solutions for anisotropic dark energy in Bianchi type III models.

Analyzed physical behavior of solutions using relevant physical quantities.

Explored implications of constant deceleration parameter in this context.

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 $\phi$ and scale factor $a$ to find the solutions. The physical behavior of the solutions has been discussed using some physical quantities.