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Expanding and shearing inhomogeneous cosmological models for viscous fluid distributions with electromagnetic field

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Abstract

Some inhomogeneous viscous fluid cosmological models in the presence of an electromagnetic field for cylindrical symmetry are obtained. To get a determinate solution, it is assumed that the coefficient of shear viscosity is proportional to the rate of expansion. The paper also discusses the behaviour of the model when viscosity is absent and comments on some other physical properties.

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References

  • Bali, R. and Singh, G.: 1987,Astrophys. Space Sci. 138, 71.

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  • Hawking, S. W. and Ellis, G. F. R.: 1973,The Large-scale Structure of Space-time, Cambridge Univ. Press, Cambridge, p. 91.

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  • Landau, L. D. and Lifshitz, E. M.: 1963,Fluid Mechanics, Pergamon Press, New York, Vol. 6 p. 505.

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  • Lichnerowicz, A.: 1967,Relativistic Hydrodynamics and Magnetohydrodynamics, Benjamin, New York, p. 13.

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Authors and Affiliations

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

    Raj Bali & Ghanshyam Singh

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  1. Raj Bali
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  2. Ghanshyam Singh
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Bali, R., Singh, G. Expanding and shearing inhomogeneous cosmological models for viscous fluid distributions with electromagnetic field. Astrophys Space Sci 143, 377–386 (1988). https://doi.org/10.1007/BF00637149

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  • DOI: https://doi.org/10.1007/BF00637149

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