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Good things always come in 3s: trimodality in the binary black-hole chirp-mass distribution supports bimodal black-hole formation
The latest GWTC-4 release from the LIGO-Virgo-KAGRA (LVK) collaboration nearly doubles the known population of double compact object mergers and reveals a new trimodal structure in the chirp-mass distribution of merging binary black holes (BBHs) below 30 Msun. Recent detailed stellar evolution model
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