Generalized expanding and shearing magnetized viscous fluid cosmological model

We investigate the behavior of a magnetic field in a viscous fluid cosmological model where the expansion in the model is proportional to ₁ ¹ , the component of shear tensor _i ^j , which leads to A=(Bc)ⁿ. We also assume that the shear viscosity is proportional to the rate of expansion in the model. The behavior of the model in the absence of a magnetic field and viscosity is discussed as are some other physical and geometrical aspects.