Evolution of accretion tori orbiting black holes. I - Theory

Details Evolution of accretion tori orbiting black holes. I - Theory Evolution of accretion tori orbiting black holes. I - Theory

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.203..323a&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 203, Apr. 1983, p. 323-338. Research supported by the Science and Engin

Astronomy and Astrophysics

Astronomy

14

Accretion Disks, Astronomical Models, Black Holes (Astronomy), Angular Momentum, Conservation Laws, Evolution (Development), Mass Distribution, Toruses

Scientific paper

A method for studying the evolution of accretion tori orbiting around black holes is outlined. It assumes that the time-scale of evolution is much longer than the dynamical time-scale. The method consists of the arrangement of sequences of models in dynamical equilibrium. It incorporates viscous redistribution of angular momentum, mass loss due to the relativistic 'Roche lobe overflow' and other dissipative phenomena.

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