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GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
Phys. Rev. Lett. 118, 221101 – Published 1 June, 2017Erratum Phys. Rev. Lett. 121, 129901 (2018)
DOI: https://doi.org/10.1103/PhysRevLett.118.221101
Abstract
We describe the observation of GW170104, a gravitational-wave signal produced by the coalescence of a pair of stellar-mass black holes. The signal was measured on January 4, 2017 at 10∶11:58.6 UTC by the twin advanced detectors of the Laser Interferometer Gravitational-Wave Observatory during their second observing run, with a network signal-to-noise ratio of 13 and a false alarm rate less than 1 in 70 000 years. The inferred component black hole masses are and (at the 90% credible level). The black hole spins are best constrained through measurement of the effective inspiral spin parameter, a mass-weighted combination of the spin components perpendicular to the orbital plane, . This result implies that spin configurations with both component spins positively aligned with the orbital angular momentum are disfavored. The source luminosity distance is corresponding to a redshift of . We constrain the magnitude of modifications to the gravitational-wave dispersion relation and perform null tests of general relativity. Assuming that gravitons are dispersed in vacuum like massive particles, we bound the graviton mass to . In all cases, we find that GW170104 is consistent with general relativity.
Physics Subject Headings (PhySH)
Erratum
Erratum: GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2 [Phys. Rev. Lett. 118, 221101 (2017)]
Synopsis
LIGO Picks Up on the Third Ring
The LIGO collaboration reports its third detection of gravitational waves coming from the merger of two black holes.
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