GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2

Abstract

© 2017 American Physical Society.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 31.2-6.0+8.4M' and 19.4-5.9+5.3M (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, χeff=-0.12-0.30+0.21. This result implies that spin configurations with both component spins positively aligned with the orbital angular momentum are disfavored. The source luminosity distance is 880-390+450 Mpc corresponding to a redshift of z=0.18-0.07+0.08. 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 mg≤7.7×10-23 eV/c2. In all cases, we find that GW170104 is consistent with general relativity.

Metadata

Authors/Creators:

Abbott, B.P.
Abbott, R.
Abbott, T.D.
Acernese, F.
Ackley, K.
Adams, C.
Adams, T.
Addesso, P.
Adhikari, R.X.
Adya, V.B.
Affeldt, C.
Afrough, M.
Agarwal, B.
Agathos, M.
Agatsuma, K.
Aggarwal, N.
Aguiar, O.D.
Aiello, L.
Ain, A.
Ajith, P.
Allen, B.
Allen, G.
Allocca, A.
Altin, P.A.
Amato, A.
Ananyeva, A.
Anderson, S.B.
Anderson, W.G.
Antier, S.
Appert, S.
Arai, K.
Araya, M.C.
Areeda, J.S.
Arnaud, N.
Arun, K.G.
Ascenzi, S.
Ashton, G.
Ast, M.
Aston, S.M.
Astone, P.
Aufmuth, P.
Aulbert, C.
Aultoneal, K.
Avila-Alvarez, A.
Babak, S.
Bacon, P.
Bader, M.K.M.
Bae, S.
Baker, P.T.
Baldaccini, F.
Ballardin, G.
Ballmer, S.W.
Banagiri, S.
Barayoga, J.C.
Barclay, S.E.
Barish, B.C.
Barker, D.
Barone, F.
Barr, B.
Barsotti, L.
Barsuglia, M.
Barta, D.
Bartlett, J.
Bartos, I.
Bassiri, R.
Basti, A.
Batch, J.C.
Baune, C.
Bawaj, M.
Bazzan, M.
Bécsy, B.
Beer, C.
Bejger, M.
Belahcene, I.
Bell, A.S.
Berger, B.K.
Bergmann, G.
Berry, C.P.L.
Bersanetti, D.
Bertolini, A.
Betzwieser, J.
Bhagwat, S.
Bhandare, R.
Bilenko, I.A.
Billingsley, G.
LIGO Scientific and Virgo Collaboration, .

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.

Keywords:

TEGA.EDO@SHEFFIELD.AC.UK

Dates:

Published (online): 1 June 2017
Published: 1 June 2017

Institution:

The University of Sheffield

Academic Units:

The University of Sheffield > Faculty of Science (Sheffield) > Department of Physics and Astronomy (Sheffield)

Funding Information:

Funder	Grant number
SCIENCE AND TECHNOLOGY FACILITIES COUNCIL	ST/K001337/1
ENGINEERING AND PHYSICAL SCIENCE RESEARCH COUNCIL (EPSRC)	NONE
SCIENCE AND TECHNOLOGY FACILITIES COUNCIL	ST/I006242/1
ENGINEERING AND PHYSICAL SCIENCE RESEARCH COUNCIL (EPSRC)	NONE
ENGINEERING AND PHYSICAL SCIENCE RESEARCH COUNCIL (EPSRC)	NONE
SCIENCE AND TECHNOLOGY FACILITIES COUNCIL	ST/K000365/1
SCIENCE AND TECHNOLOGY FACILITIES COUNCIL	ST/N000080/1
SCIENCE AND TECHNOLOGY FACILITIES COUNCIL	ST/N005716/1
SCIENCE AND TECHNOLOGY FACILITIES COUNCIL	UNSPECIFIED