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Radiative Models of Sagittarius A* and M87 from Relativistic MHD Simulations
(2011-07)
The discovery that the magnetorotational instability (MRI) is likely the
mechanism of angular momentum transport and accretion has led to rapid
progress in the theory of black hole accretion. General relativistic
MHD (GRMHD) simulations currently provide the most
realistic physical description of black hole accretion ...