GWTC-4 chirp-mass data show a peak-gap structure that is matched only by a bimodal black-hole mass model, supporting a link between black-hole masses and supernova physics.
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New gravitational-wave data support a bimodal black-hole mass distribution
GWTC-4 chirp-mass data show a peak-gap structure that is matched only by a bimodal black-hole mass model, supporting a link between black-hole masses and supernova physics.