MAGNETIZED BIANCHI TYPE-VI0 COSMOLOGICAL MODEL FOR BAROTROPIC FLUID DISTRIBUTION WITH VARIABLE MAGNETIC PERMEABILITY AND DARK ENERGY

We have investigated Bianchi type-VI0 cosmological model for barotropic fluid distribution in the presence and absence of magnetic field with dark energy Lambda. To obtain the explicit solution of the model, we assume that the magnetic field is in xy plane, therefore the current is flowing along the z-axis. Thus F-12 is the only non-vanishing component of the electromagnetic field tensor F-ij. Also, we suppose expansion theta is proportional to the shear sigma. The behaviour of the models from physical and geometrical aspects in presence and absence of magnetic field is also discussed.