We have studied anisotropic and homogeneous Bianchi type-VIh cosmological models of the universe with variable equation of state (EoS) parameter (w) in General Relativity. A special form of deceleration parameter (q) which gives an early deceleration and late time accelerating cosmological model has been utilized to solve the Einstein’s field equations. The geometrical and physical aspects of the models are also studied.
Cite this article:
K.S. Adhav, D.R.K. Reddy, G.B. Tayade. Accelerating Bianchi type- VIh Cosmological Model with variable EoS parameter. Int. J. Tech. 4(1): Jan.-June. 2014; Page 27-31