Self-gravitating thin disks around rapidly rotating black holes

Details Self-gravitating thin disks around rapidly rotating black holes Self-gravitating thin disks around rapidly rotating black holes

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...389..141l&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 389, April 10, 1992, p. 141-156.

Astronomy and Astrophysics

Astronomy

23

Accretion Disks, Active Galactic Nuclei, Black Holes (Astronomy), Einstein Equations, Angular Momentum, Angular Velocity, Astronomical Models, Boundary Conditions, Gravitational Fields, Multigrid Methods, Partial Differential Equations, Stellar Rotation

Scientific paper

Sequences of equilibrium numerical models were constructed for self-gravitating thin disks encircling rapidly rotating black holes. The multigrid method was used for solving numerically the stationary axisymmetric Einstein equations. The black hole is described either by specifying its angular velocity and the coordinate radius of the horizon or, alternatively, by specifying the area of the horizon and the angular momentum.

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