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Magnetohydrodynamic equilibrium conditions in the post-Newtonian approximation of general relativity

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Abstract

A set of equations, which are magnetohydrodynamic (MHD) equilibrium conditions in the post-Newtonian approximation of general relativity (PNA of GR), is obtained. The given system generalizes the previously obtained magnetohydrodynamic equilibrium conditions of classical mechanics and the hydrodynamic equilibrium conditions in the PNA of GR.

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Authors and Affiliations

  1. The Institute for Theoretical Physics, Academy of Sciences of the Ukrainian S.S.R., Kiev, USSR

    N. P. Bondarenko & O. V. Kravtsov

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  1. N. P. Bondarenko
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  2. O. V. Kravtsov
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Bondarenko, N.P., Kravtsov, O.V. Magnetohydrodynamic equilibrium conditions in the post-Newtonian approximation of general relativity. Astrophys Space Sci 32, 379–384 (1975). https://doi.org/10.1007/BF00643151

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  • DOI: https://doi.org/10.1007/BF00643151

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