Bianchi Type III Anisotropic Dark Energy Models with Constant Deceleration Parameter

TL;DR

This paper investigates Bianchi type III anisotropic dark energy models with a constant deceleration parameter, analyzing their compatibility with observational data and discussing their physical properties.

Contribution

It introduces a specific anisotropic dark energy model with a constant deceleration parameter and examines its observational consistency and physical characteristics.

Findings

Equation of state parameter $$ is time-dependent.

Model's $$ range aligns with SN Ia, CMBR, and galaxy clustering data.

Physical aspects of the dark energy models are discussed.

Abstract

The Bianchi type III dark energy models with constant deceleration parameter are investigated. The equation of state parameter $\omega$ is found to be time dependent and its existing range for this model is consistent with the recent observations of SN Ia data, SN Ia data (with CMBR anisotropy) and galaxy clustering statistics. The physical aspect of the dark energy models are discussed.