Magnetized Locally-rotationally Symmetric Bianchi Type-iii Cosmological Model With Wet Dark Fluid in General Relativity

Abstract

In this paper, we have investigated the effect of magnetic field and Wet dark fluid on locally-rotationally symmetric Bianchi type-III cosmological which is non-shearing. A new equation of state for the dark energy component of the universe has been used. It is modeled on the equation of state p = γ(ρ – ρ_∗) which can describe a liquid, for example water. The exact solutions to the corresponding field equations are obtained in quadrature form. The obtained solution have been studied in detailed for both power-law and exponential form. In addition to this we have discuss the geometrical and physical properties of said model.