Bianchi Type III Anisotropic Dark Energy Models with Constant Deceleration Parameter

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.

12 pages, 2 figures, Accepted version of IJTP

References in corpus (7)

• Dynamics of dark energy
• Reconstructing Dark Energy
• Dark Energy and Gravity
• Constraining Dark Energy Anisotropic Stress
• Cosmic Acceleration, Dark Energy and Fundamental Physics
• The dark energy equation of state
• $\Lambda$-CDM Universe: A Phenomenological Approach With Many Possibilities

Cited by in corpus (1)

• Bianchi Type-I Anisotropic Dark Energy Models with Constant Deceleration Parameter