Dynamics of Bianchi Type-III Universe with Magnetized Anisotropic Dark Energy

Abstract

Bianchi type -III cosmological model in the presence of magnetized anisotropic dark energy 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.