Abstract
The Bianchi type III dark energy model with constant deceleration parameter is investigated. The equation of state parameter ω 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 aspects of the dark energy models is discussed.
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Yadav, A.K., Yadav, L. Bianchi Type III Anisotropic Dark Energy Models with Constant Deceleration Parameter. Int J Theor Phys 50, 218–227 (2011). https://doi.org/10.1007/s10773-010-0510-3
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DOI: https://doi.org/10.1007/s10773-010-0510-3