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Dynamical equations of a magnetofluid universe

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Abstract

Dynamical equations of magnetofluid are derived for Robertson-Walker line element. We recover the results of perfect fluid in a special case when the magnetic field is made to vanish. Certain conditions are derived to show that the magnetofluid universe is open or closed.

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References

  • Gott, J. R. and Turner, E. L.: 1976,Astrophys. J. 209, 1.

    Google Scholar 

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

    Google Scholar 

  • Pandey, U. S. and Dubey, G. S.: 1983,Astrophys. Space Sci. 97, 427.

    Google Scholar 

  • Pandey, U. S. and Dubey, G. S.: 1984,Astrophys. Space Sci. 102, 71.

    Google Scholar 

  • Pandey, U. S. and Dubey, G. S.: 1986,Astrophys. Space Sci. 126, 99.

    Google Scholar 

  • Pandey, U. S. and Dubey, G. S.: 1988,Astrophys. Space Sci. 150, 205.

    Google Scholar 

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Dubey, G.S., Pandey, U.S. & Prasad, S.S. Dynamical equations of a magnetofluid universe. Astrophys Space Sci 188, 331–335 (1992). https://doi.org/10.1007/BF00644919

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  • DOI: https://doi.org/10.1007/BF00644919

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