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arXiv · 1007.1411

Bianchi Type III Anisotropic Dark Energy Models with Constant Deceleration Parameter

Anil Kumar Yadav·Lallan Yadav
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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.

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Anil Kumar Yadav, Lallan Yadav. 2010-07-08. Bianchi Type III Anisotropic Dark Energy Models with Constant Deceleration Parameter. https://doi.org/10.1007/s10773-010-0510-3

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