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

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

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ap%26ss..32..379b&link_type=abstract

Astrophysics and Space Science, vol. 32, Feb. 1975, p. 379-384.

Astronomy and Astrophysics

Astrophysics

4

Conservation Laws, Equations Of Motion, Equilibrium Equations, Magnetohydrodynamic Stability, Relativity, Angular Momentum, Approximation, Boundary Value Problems, Electromagnetic Fields, Functionals, Integral Equations

Scientific paper

A set of equations, which are magnetohydrodynarnic (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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