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

Details METHODOLOGICAL NOTES: Axially symmetric steady-state flows in the vicinity of a Kerr black hole and the nature of the activity of galactic nuclei METHODOLOGICAL NOTES: 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=1993phyu...36..529b&link_type=abstract

Physics Uspekhi, Volume 36, Issue 6, pp. 529-539 (1993).

Physics

13

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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