An Inhomogeneous Cosmological Model in Electromagnetic Bulk Viscous Fluid with Variable (Λ)
An inhomogeneous cylindrically symmetric cosmological model for bulk viscous fluid distribution with electromagnetic field is obtained. To get a deterministic solution, it is assumed that the component σ11 of shear tensor σji is proportional to expansion ɵ and the coefficient of bulk viscosity is assumed to be a power function of mass density. The source of the magnetic field is due to an electric current produced along z-axis. Some physical and kinematical aspects of the models are also discussed in presence and absence of the magnetic field.