Bianchi Type-V Cosmological Model with Two Fluids in the Presence of Magnetic Flux in General Relativity

Abstract

In this paper, we have investigated Bianchi type-V two fluid cosmological model, i.e., with matter and radiating source in presence of electromagnetic field in general relativity. In this model one of the fluids represents the matter contents of the universe and another fluid is the CMB radiation. The magnetic field is due to an electric current produced along x-axis, F₂₃ is the only non-vanishing component of electromagnetic field tensor F_ij. Here we discuss the physical properties of model and behavior of kinematical parameters like expansion, shear and the anisotropy parameters are discussed in details in each section.