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

摘要

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.