Black hole spacetimes with self-gravitating, massive accretion tori

Physics

Scientific paper

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Scientific paper

We review the theory of stationary, axisymmetric spacetimes with black
holes surrounded by a massive torus and present a numerical scheme for
finding self-consistent solutions in a compactified grid that reaches to
spatial infinity. Such numerical solutions have been utilized in
studying nonaxisymmetric dynamical instabilities occurring in the torus.

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