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
Keywords: Bianchi type-III space-time, Bulk
Viscosity, Magnetic flux.