Bianchi Type III Anisotropic Dark Energy Models with Constant Deceleration Parameter
General Relativity and Quantum Cosmology
2011-01-05 v3
Abstract
The Bianchi type III dark energy models with constant deceleration parameter are investigated. The equation of state parameter 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.
Keywords
Cite
@article{arxiv.1007.1411,
title = {Bianchi Type III Anisotropic Dark Energy Models with Constant Deceleration Parameter},
author = {Anil Kumar Yadav and Lallan Yadav},
journal= {arXiv preprint arXiv:1007.1411},
year = {2011}
}
Comments
12 pages, 2 figures, Accepted version of IJTP