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Evidence of the Pair-Instability Gap From Black-Hole Masses
Researchers found an unambiguous 44-to-116-solar-mass gap in merging black holes, supporting pair-instability supernovas as the cause, the paper said.
Summary by Nature
4 Articles
4 Articles
Evidence of the pair-instability gap from black-hole masses
Stellar theory predicts a forbidden range of black-hole masses between approximately 50 M⊙ and 130 M⊙ owing to pair-instability supernovae1–7, but evidence for such a gap in the mass distribution from gravitational-wave astronomy has proved elusive. Early hints of a cut-off in black-hole masses at about 45 M⊙ disappeared with the subsequent discovery of more massive binary black holes8,9. Here we report evidence of the pair-instability gap i
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Total News Sources4
Leaning Left1Leaning Right0Center2Last UpdatedBias Distribution67% Center
Bias Distribution
- 67% of the sources are Center
67% Center
L 33%
C 67%
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