Slowly rotating 80–85 M☉ Pop III stars can keep most of their mass and form black holes with spins up to a_BH ≲ 0.7 just below the pair-instability gap.
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Fast-spinning massive black holes from slowly rotating low-metallicity stars: Implications for GW231123
Slowly rotating 80–85 M☉ Pop III stars can keep most of their mass and form black holes with spins up to a_BH ≲ 0.7 just below the pair-instability gap.
- Mass and Spin Growth of Very Massive Stars in Star Clusters Potentially Associated with Little Red Dots