The Impact of Pair-instability Mass Loss on the Binary Black Hole Mass Distribution

@article{Stevenson2019TheIO,
  title={The Impact of Pair-instability Mass Loss on the Binary Black Hole Mass Distribution},
  author={S. Stevenson and Matthew Sampson and J. Powell and A. Vigna-G{\'o}mez and C. Neijssel and D. Sz'ecsi and I. Mandel},
  journal={The Astrophysical Journal},
  year={2019},
  volume={882},
  pages={121}
}
  • S. Stevenson, Matthew Sampson, +4 authors I. Mandel
  • Published 2019
  • Physics
  • The Astrophysical Journal
  • A population of binary black hole mergers has now been observed in gravitational waves by Advanced LIGO and Virgo. The masses of these black holes appear to show evidence for a pile-up between $30$--$45$ $M_\odot$ and a cut-off above $\sim 45$ $M_\odot$. One possible explanation for such a pile-up and subsequent cut-off are pulsational pair-instability supernovae (PPISNe) and pair-instability supernovae (PISNe) in massive stars. We investigate the plausibility of this explanation in the context… CONTINUE READING
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