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Generalized expanding and shearing magnetized viscous fluid cosmological model

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Abstract

We investigate the behavior of a magnetic field in a viscous fluid cosmological model where the expansionθ in the model is proportional toσ 11 , the component of shear tensorσ j i , 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.

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Authors and Affiliations

  1. Department of Mathematics, University of Rajasthan, 302004, Jaipur, India

    Raj Bali & Mahbub Ali

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  1. Raj Bali
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  2. Mahbub Ali
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Bali, R., Ali, M. Generalized expanding and shearing magnetized viscous fluid cosmological model. Int J Theor Phys 33, 2067–2074 (1994). https://doi.org/10.1007/BF00675172

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  • DOI: https://doi.org/10.1007/BF00675172

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