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 M⊙ and 66-18+17 M⊙ (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 M⊙. We calculate the mass of the remnant to be 142-16+28M⊙, 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-3yr-1.
Original language | English |
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Article number | 101102 |
Number of pages | 17 |
Journal | Physical Review Letters |
Volume | 125 |
Issue number | 10 |
Early online date | 2 Sept 2020 |
DOIs | |
Publication status | Published - 4 Sept 2020 |
ASJC Scopus subject areas
- General Physics and Astronomy