GRMHD simulations show that rapidly spinning black holes with magnetically arrested disks can produce outflow powers matching hard-state ULXs, and suggest FSRQs and BL Lacs differ by SANE versus MAD magnetic states.
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Simulating ULXs and blazars as GRMHD accretion flows around a black hole
GRMHD simulations show that rapidly spinning black holes with magnetically arrested disks can produce outflow powers matching hard-state ULXs, and suggest FSRQs and BL Lacs differ by SANE versus MAD magnetic states.