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Viscous accretion and ejection from tori around black holes in general relativity
We systematically perform long-term (millions of Schwarzschild time) axisymmetric viscous hydrodynamics simulations for tori around black holes in general relativity supposing the super-Eddington accretion flow. The initial condition for the tori is modeled simply by the Fishbone-Moncrief torus with
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