Bianchi Type III Magnetized Anisotropic Dark Energy Models with Constant Deceleration Parameter

Abstract

The Bianchi type III magnetized dark energy model with constant deceleration parameter is investigated. The energy-momentum tensor consists of anisotropic fluid with anisotropic EoS p = ωρ and a uniform magnetic field of energy density ρ_B.We obtain exact solutions to the field equations using the condition that expansion is proportional to the shear scalar . The physical behavior of the model is discussed with and without magnetic field. We conclude that universe model as well as anisotropic fluid does not approach isotropy through the evolution of the universe. The physical aspects of the dark energy models are discussed.