Sensitivity of the lower-edge of the pair instability black hole mass gap to the treatment of time dependent convection

19 Feb 2020 Renzo M. Farmer R. J. Justham S. de Mink S. E. Götberg Y. Marchant P.

Gravitational-wave detections are now probing the black hole (BH) mass distribution, including the predicted pair-instability mass gap. These data require robust quantitative predictions, which are challenging to obtain... (read more)

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  • SOLAR AND STELLAR ASTROPHYSICS
  • HIGH ENERGY ASTROPHYSICAL PHENOMENA