GRMHD simulations of magnetically arrested advective flows around spinning stellar-mass black holes yield outflow powers of 10^39-10^40 erg/s, but the paper equates this mechanical power to observed ULX X-ray luminosity without modeling radiation.
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Magnetically arrested advective accretion flows and jets/outflows around stellar mass black holes: Explaining hard state ULXs with GRMHD simulations
GRMHD simulations of magnetically arrested advective flows around spinning stellar-mass black holes yield outflow powers of 10^39-10^40 erg/s, but the paper equates this mechanical power to observed ULX X-ray luminosity without modeling radiation.