R. Bali et M. Ali, GENERALIZED EXPANDING AND SHEARING MAGNETIZED VISCOUS-FLUID COSMOLOGICAL MODEL, International journal of theoretical physics, 33(10), 1994, pp. 2067-2074
We investigate the behavior of a magnetic field in a viscous fluid cos
mological model where the expansion theta in the model is proportional
to sigma(1)(1), the component of shear tenser sigma(i)(j), which lead
s to A = (BC)(n). We also assume that the shear viscosity is proportio
nal to the rate of expansion in the model. The behavior of the model i
n the absence of a magnetic field and viscosity discussed as are some
other physical and geometrical aspects.