Axially symmetric steady-state flows in the vicinity of a Kerr black hole and the nature of the activity of galactic nuclei.

Details Axially symmetric steady-state flows in the vicinity of a Kerr black hole and the nature of the activity of galactic nuclei. Axially symmetric steady-state flows in the vicinity of a Kerr black hole and the nature of the activity of galactic nuclei.

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993svphu..36..529b&link_type=abstract

Soviet Physics Uspekhi, Vol. 36, No. 6, p. 529 - 539

Physics

26

Black Holes: Active Galactic Nuclei, Kerr Black Holes: Magnetohydrodynamics

Scientific paper

A generalization of the force-free equation describing steady-state axially symmetric flows in the vicinity of a Kerr black hole is carried out to the case of ideal magnetohydrodynamics. It is shown how this equation changes from an elliptic to a hyperbolic type in the vicinity of the horizon. The limits of applicability of the approach under discussion are examined for different astrophysical sources. It is shown that a high photon density strongly restricts the limits of applicability of the MHD approach.

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