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This article presents evidence for the pair-instability mass gap in black holes, indicating a lower edge at approximately 44.3 M⊙, based on gravitational-wave observations. The findings suggest that hierarchical mergers in dense stellar clusters contribute to the black hole mass spectrum, with two distinct populations identified: low-spin black holes below the gap and high-spin black holes occupying the gap. Additionally, the study provides a measurement of the 12C(α, γ)16O reaction rate, linking gravitatio

Author

legndaryguy536

Language

EN