Inviscid hydromagnetic horizon boundary conditions

Details Inviscid hydromagnetic horizon boundary conditions Inviscid hydromagnetic horizon boundary conditions

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phrvd..44.2970p&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 44, Issue 10, 15 November 1991, pp.2970-2982

Astronomy and Astrophysics

Astrophysics

5

Magnetohydrodynamics And Plasmas, Fundamental Problems And General Formalism, Relativity And Gravitation

Scientific paper

This article examines the state of a magnetized fluid or plasma arbitrarily close to the event horizon of a Kerr black hole. It is found that the bulk four-velocity attains a unique asymptotic form as viewed by all external observers and there are no stable equilibria arbitrarily close to the horizon. Of particular astrophysical interest, it is shown that if one attempts to suspend a plasma just outside the horizon with magnetic ropes then the large-scale magnetic-field lines will be reconnected and the plasma will accrete toward the hole.

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