Relativistic MHD flows in a steady gravitational field

Details Relativistic MHD flows in a steady gravitational field Relativistic MHD flows in a steady gravitational field

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983svjpp...9.1231l&link_type=abstract

(Fizika Plazmy, vol. 9, Nov.-Dec. 1983, p. 1231-1241) Soviet Journal of Plasma Physics (ISSN 0360-0343), vol. 9, Nov.-Dec. 1983,

Astronomy and Astrophysics

Astronomy

Black Holes (Astronomy), Gravitational Fields, Magnetohydrodynamic Flow, Relativistic Plasmas, Equations Of State, Magnetic Fields, Plasma Equilibrium, Rotating Matter, Steady State

Scientific paper

The equations of relativistic MHD in a strong, stationary gravitational field are derived. Some solutions of these equations are found which describe stationary plasma flows in the gravitational field of a rotating black hole. The plasma is assumed to be frozen in the magnetic field, and dissipative processes are ignored. The equation of state of the plasma is not specified. The results are extended to the case of a plasma with a zero chemical potential.

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