A new gravitational wave event reveals a binary black hole merger with total mass 190-265 solar masses, indicating black holes can form via gravitational-wave driven mergers beyond standard stellar channels.
2020 b , Classical and Quantum Gravity, 37, 055002, 10.1088/1361-6382/ab685e
4 Pith papers cite this work, alongside 347 external citations. Polarity classification is still indexing.
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GW231123: a Binary Black Hole Merger with Total Mass 190-265 $M_{\odot}$
A new gravitational wave event reveals a binary black hole merger with total mass 190-265 solar masses, indicating black holes can form via gravitational-wave driven mergers beyond standard stellar channels.
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Gravitational-Wave Parameter Estimation in non-Gaussian noise using Score-Based Likelihood Characterization
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Open Data from LIGO, Virgo, and KAGRA through the Second Part of the Fourth Observing Run
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