GW190521: A binary black hole merger with a total mass of 150  M⊙

LIGO Scientific Collaboration and Virgo Collaboration, B. P. Abbott, S. V. Angelova, C. Gier, S. Macfoy, S. Reid, G. S. Wallace

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Abstract

On May 21, 2019 at 03:02:29 UTC Advanced LIGO and Advanced Virgo observed a short duration gravitational-wave signal, GW190521, with a three-detector network signal-to-noise ratio of 14.7, and an estimated false-alarm rate of 1 in 4900 yr using a search sensitive to generic transients. If GW190521 is from a quasicircular binary inspiral, then the detected signal is consistent with the merger of two black holes with masses of 85-14+21 Mm and 66-18+17 Mm (90% credible intervals). We infer that the primary black hole mass lies within the gap produced by (pulsational) pair-instability supernova processes, with only a 0.32% probability of being below 65 Mm. We calculate the mass of the remnant to be 142-16+28 Mm, which can be considered an intermediate mass black hole (IMBH). The luminosity distance of the source is 5.3-2.6+2.4 Gpc, corresponding to a redshift of 0.82-0.34+0.28. The inferred rate of mergers similar to GW190521 is 0.13-0.11+0.30 Gpc-3 yr-1.

Original languageEnglish
Article number101102
Number of pages17
JournalPhysical Review Letters
Volume125
Issue number10
DOIs
Publication statusPublished - 4 Sep 2020

Keywords

  • gravitational waves
  • binary black hole mergers
  • GW190521

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