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Rotating ideal magnetohydrodynamic flow in General relativity

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Abstract

The field equations and the equation of motion for stationary, axisymmetric, rotating ideal magnetohydrodynamic flow are presented. Exact solutions are obtained for rigid rotation, for vanishing and nonvanishing Lorentz force.

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Author notes

  1. A. H. Khater

    Present address: Mathematics Department, Faculty of Science, King Abdulaziz University, Jeddah, Saudi Arabia

Authors and Affiliations

  1. Mathematics Department, Faculty of Science, Cairo University, Beni-Suef, Egypt

    A. H. Khater

  2. Mathematics Department, Faculty of Science, Minia University, Minia, Egypt

    M. J. Mourad

Authors
  1. A. H. Khater
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  2. M. J. Mourad
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Khater, A.H., Mourad, M.J. Rotating ideal magnetohydrodynamic flow in General relativity. Astrophys Space Sci 152, 215–222 (1989). https://doi.org/10.1007/BF00636307

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  • DOI: https://doi.org/10.1007/BF00636307

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