Abstract
We investigate the behavior of a magnetic field in a viscous fluid cosmological model where the free gravitational field is of Petrov type D and the coefficient of shear viscosity is proportional to the rate of expansion in the model. Also discussed are the behavior of the model when the magnetic field tends to zero and some other physical properties.
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Bali, R., Jain, D.R. An anisotropic magnetized viscous fluid cosmological model in general relativity. Int J Theor Phys 28, 903–910 (1989). https://doi.org/10.1007/BF00670003
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DOI: https://doi.org/10.1007/BF00670003