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Search for Eccentric Binary Black Hole Mergers with Advanced LIGO and Advanced Virgo during their First and Second Observing Runs

https://doi.org/10.3847/1538-4357/ab3c2d

  • AuthorB. P. Abbott,김환선,손재주,오상훈,오정근
  • JournalThe Astrophysical Journal (0004-637X), 883(2), 149-1 ~ 149-10
  • Enrollment typeSCI
  • publication date 20190930
When formed through dynamical interactions, stellar-mass binary black holes (BBHs) may retain eccentric orbits (e > 0.1 at 10 Hz) detectable by ground-based gravitational-wave detectors.