Magnetized anisotropic dark energy models with constant deceleration parameter

摘要

In this paper, we have studied the solutions of plane-symmetric Universe with variable $omega$ in the presence and the absence of magnetic field of energy density $ ho B$. A special law of variation for Hubblea€?s parameterproposed by Bermann in {it Nuovo Cimento} B 74, 182 (1983) has been utilized to solve the field equations. Some physical and kinematical properties of the models are also discussed.