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^+21_−14 M⊙ and 66^+17_−18 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^+28_−16 M⊙, which can be considered an intermediate mass black hole (IMBH). The luminosity distance of the source is 5.3^+2.4_−2.6 Gpc, corresponding to a redshift of 0.82^+0.28_−0.34. The inferred rate of mergers similar to GW190521 is 0.13^+0.30_−0.11 Gpc^−3 yr^−1.

GW190521: A Binary Black Hole Merger with a Total Mass of 150  M⊙

Bischi, M.;Brighenti, F.;Greco, G.;Guidi, G.;Martelli, F.;Montani, M.;Piergiovanni, F.;Vetrano, F.;Vicere', A.;
2020

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^+21_−14 M⊙ and 66^+17_−18 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^+28_−16 M⊙, which can be considered an intermediate mass black hole (IMBH). The luminosity distance of the source is 5.3^+2.4_−2.6 Gpc, corresponding to a redshift of 0.82^+0.28_−0.34. The inferred rate of mergers similar to GW190521 is 0.13^+0.30_−0.11 Gpc^−3 yr^−1.
File in questo prodotto:
File Dimensione Formato  
GW190521_Discovery_PhysRevLett.125.101102.pdf

accesso aperto

Descrizione: Articolo principale
Tipologia: Versione editoriale
Licenza: Creative commons
Dimensione 1.44 MB
Formato Adobe PDF
1.44 MB Adobe PDF Visualizza/Apri

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11576/2678671
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus 947
  • ???jsp.display-item.citation.isi??? 655
social impact