Impact of the Rotation and Compactness of Progenitors on the Mass of Black Holes

@article{Mapelli2019ImpactOT,
  title={Impact of the Rotation and Compactness of Progenitors on the Mass of Black Holes},
  author={Michela Mapelli and Mario Spera and Enrico Montanari and Marco Limongi and Alessandro Chieffi and Nicola Giacobbo and Alessandro Bressan and Yann Bouffanais},
  journal={arXiv: High Energy Astrophysical Phenomena},
  year={2019}
}
We investigate the impact of stellar rotation on the formation of black holes (BHs), by means of our population-synthesis code SEVN. Rotation affects the mass function of BHs in several ways. In massive metal-poor stars, fast rotation reduces the minimum zero-age main sequence (ZAMS) mass for a star to undergo pair instability and pulsational pair instability. Moreover, stellar winds are enhanced by rotation, peeling-off the entire hydrogen envelope. As a consequence of these two effects, the… Expand

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