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Bianchi Type-III Universe with Anisotropic Dark Energy and Special form of Deceleration Parameter

Abstract

The present study deals with Bianchi type-III cosmological models with anisotropic dark energy and special form of deceleration parameter. To have a general description of an anisotropic dark energy component, a phenomenological parameterization of dark energy in terms of its equation of state (EoS) and two skewness parameters ( ,  ) have been introduced. The geometrical and physical behaviour of the models are also discussed.

K. S. Adhav, R.P.Wankhade, A.S.Bansod

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