GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
Name
PhysRevLett.118.221101.pdf
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Author(s)
Aggarwal, Nancy
Barsotti, Lisa
Biscans, Sebastien
Brown, N. M.
Buikema, Aaron
Donovan, Frederick J
Eisenstein, Robert Alan
Essick, Reed Clasey
Evans, Matthew J
Fernandez Galiana, Alvaro-Miguel
Date Issued
June 2017
Journal
Physical Review Letters
Publisher
American Physical Society
Citation
Abbott, B. P. et al. “GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2.” Physical Review Letters 118.22 (2017): n. pag. © 2017 American Physical Society
Version
Final published version
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 31.2[superscript +8.4] [subscript −6.0]M⊙ and 19.4 [superscript +5.3] [subscript −5.9]M⊙ (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,
χ [subscript eff] = −0.12[superscript +0.21] [subscript −0.30]. This result implies that spin configurations with both component spins positively aligned with the orbital angular momentum are disfavored. The source luminosity distance is 880 [superscript +450] [subscript −390] Mpc corresponding to a redshift of z = 0.18[superscript +0.08][subscript −0.07]. 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 m[subscript g] ≤ 7.7 × 10 [superscript −23] eV/c[superscript 2]. In all cases, we find that GW170104 is consistent with general relativity.
MIT Department
Lincoln Laboratory
Massachusetts Institute of Technology. Department of Physics
Massachusetts Institute of Technology. Laboratory for Nuclear Science
MIT Kavli Institute for Astrophysics and Space Research
LIGO (Observatory : Massachusetts Institute of Technology)
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DOI of Published Version
https://doi.org/10.1103/PhysRevLett.118.221101
