Paper Title
Non Shearing Locally-Rotationally Symmetric Bianchi Type-Iii String Cosmological Model In Presence Of Magnetic Flux With Bulk Viscosity In General Relativity

In this paper, we have investigated the nature of non shearing, locally-rotationally symmetric Bianchi type-III string cosmological model in presence of bulk viscosity and magnetic flux. Here we make the assumption that the coefficient of viscosity is proportional to the expansion scalar i.e. and we discuss the physical and geometrical properties of model in presence and absence of magnetic field. Keywords: Bianchi type-III space-time, Bulk Viscosity, Magnetic flux.