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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
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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Nature broke the news in United Kingdom on Wednesday, April 1, 2026.
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