BH-NS merger simulations find a nearly universal dimensionless magnetic flux on the black hole across two decades of disk mass, which, extrapolated with prior long-term runs, implies all BH-NS mergers produce long-duration gamma-ray bursts.
A Unified Picture of Short and Long Gamma-Ray Bursts from Compact Binary Mergers,
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Implications of Magnetic Flux-Disk Mass Correlation in Black Hole-Neutron Star Mergers for GRB sub-populations
BH-NS merger simulations find a nearly universal dimensionless magnetic flux on the black hole across two decades of disk mass, which, extrapolated with prior long-term runs, implies all BH-NS mergers produce long-duration gamma-ray bursts.