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Some expanding and shearing viscous fluid cosmological models in general relativity

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Abstract

Two cylindrically-symmetric cosmological models representing viscous fluid distributions when free-gravitational field of typeD where coefficient of shear viscosity is assumed to be proportional to the rate of expansion, are obtained. The behaviour of the models in the absence of viscosity and other physical properties are also discussed.

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References

  • Bali, Raj and Jain, Deepak Raj: 1988,Astrophys. Space Sci. (in press).

  • Ellis, G. F. R.: 1971, in R. K. Sachs (ed.),General Relativity and Cosmology, Academic Press, New York, p. 117.

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Authors and Affiliations

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

    Raj Bali & Deepak Raj Jain

Authors
  1. Raj Bali
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  2. Deepak Raj Jain
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Bali, R., Jain, D.R. Some expanding and shearing viscous fluid cosmological models in general relativity. Astrophys Space Sci 141, 207–216 (1988). https://doi.org/10.1007/BF00639489

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  • DOI: https://doi.org/10.1007/BF00639489

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