Relativistic Accreting Flow onto Kerr Black Holes

Details Relativistic Accreting Flow onto Kerr Black Holes Relativistic Accreting Flow onto Kerr Black Holes

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pthph..81..549k&link_type=abstract

Progress of Theoretical Physics, Vol. 81, No. 3, pp. 549-554

Physics

Scientific paper

We have proven that the radial drift velocity of the adiabatic accretion
torus orbiting around a Kerr black hole must be subsonic at the inner
edge of any torus. This result is irrespective of distributions of
angular momentum of any torus.

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