Bianchi Type III Anisotropic Dark Energy Models with Constant Deceleration Parameter

Details Bianchi Type III Anisotropic Dark Energy Models with Constant Deceleration Parameter Bianchi Type III Anisotropic Dark Energy Models with Constant Deceleration Parameter

2010-07-08

arxiv.org/abs/1007.1411v3

Int.J.Theor.Phys.50:218-227,2011

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

12 pages, 2 figures, Accepted version of IJTP

Scientific paper

10.1007/s10773-010-0510-3

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.

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