Observation of Gravitational Waves from a Binary Black Hole Merger

被引:8688
作者
Abbott, B. P. [1 ]
Abbott, R. [1 ]
Abbott, T. D. [2 ]
Abernathy, M. R. [1 ]
Acernese, F. [3 ,4 ]
Ackley, K. [5 ]
Adams, C. [6 ]
Adams, T. [7 ]
Addesso, P. [3 ]
Adhikari, R. X. [1 ]
Adya, V. B. [8 ]
Affeldt, C. [8 ]
Agathos, M. [9 ]
Agatsuma, K. [9 ]
Aggarwal, N. [10 ]
Aguiar, O. D. [11 ]
Aiello, L. [12 ,13 ]
Ain, A. [14 ]
Ajith, P. [15 ]
Allen, B. [8 ,16 ,17 ]
Allocca, A. [18 ,19 ]
Altin, P. A. [20 ]
Anderson, S. B. [1 ]
Anderson, W. G. [16 ]
Arai, K. [1 ]
Arain, M. A. [5 ]
Araya, M. C. [1 ]
Arceneaux, C. C. [21 ]
Areeda, J. S. [22 ]
Arnaud, N. [23 ]
Arun, K. G. [24 ]
Ascenzi, S. [13 ,25 ]
Ashton, G. [26 ]
Ast, M. [27 ]
Aston, S. M. [6 ]
Astone, P. [28 ]
Aufmuth, P. [8 ]
Aulbert, C. [8 ]
Babak, S. [29 ]
Bacon, P. [30 ]
Bader, M. K. M. [9 ]
Baker, P. T. [31 ]
Baldaccini, F. [32 ,33 ]
Ballardin, G. [34 ]
Ballmer, S. W. [35 ]
Barayoga, J. C. [1 ]
Barclay, S. E. [36 ]
Barish, B. C. [1 ]
Barker, D. [37 ]
Barone, F. [3 ,4 ]
机构
[1] CALTECH, LIGO, Pasadena, CA 91125 USA
[2] Louisiana State Univ, Baton Rouge, LA 70803 USA
[3] Univ Salerno, Fisciano, I-84084 Salerno, Italy
[4] Complesso Univ Monte S Angelo, Sez Napoli, Ist Nazl Fis Nucl, I-80126 Naples, Italy
[5] Univ Florida, Gainesville, FL 32611 USA
[6] LIGO Livingston Observ, Livingston, LA 70754 USA
[7] Univ Savoie Mont Blanc, CNRS, IN2P3, LAPP, F-74941 Annecy Le Vieux, France
[8] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany
[9] Nikhef, Sci Pk, NL-1098 XG Amsterdam, Netherlands
[10] MIT, LIGO, 77 Massachusetts Ave, Cambridge, MA 02139 USA
[11] Inst Nacl Pesquisas Espaciais, BR-12227010 Sao Jose Dos Campos, Brazil
[12] Ist Nazl Fis Nucl, Gran Sasso Sci Inst, I-67100 Laquila, Italy
[13] Ist Nazl Fis Nucl, Sez Roma Tor Vergata, I-00133 Rome, Italy
[14] Inter Univ Ctr Astron & Astrophys, Pune 411007, Maharashtra, India
[15] Tata Inst Fundamental Res, Int Ctr Theoret Sci, Bangalore 560012, Karnataka, India
[16] Univ Wisconsin, Milwaukee, WI 53201 USA
[17] Leibniz Univ Hannover, D-30167 Hannover, Germany
[18] Univ Pisa, I-56127 Pisa, Italy
[19] Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy
[20] Australian Natl Univ, GPO Box 4, Canberra, ACT 0200, Australia
[21] Univ Mississippi, University, MS 38677 USA
[22] Calif State Univ Fullerton, Fullerton, CA 92831 USA
[23] Univ Paris Saclay, Univ Paris Sud, CNRS, IN2P3,LAL, Orsay, France
[24] Chennai Math Inst, Madras 603103, Tamil Nadu, India
[25] Univ Roma Tor Vergata, I-00133 Rome, Italy
[26] Univ Southampton, Southampton SO17 1BJ, Hants, England
[27] Univ Hamburg, Martinistr 52, D-22761 Hamburg, Germany
[28] Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy
[29] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Golm, Germany
[30] Univ Paris Diderot, CNRS, IN2P3,APC, CEA Irfu,Observ Paris,Sorbonne Paris Cite,AstroPa, F-75205 Paris 13, France
[31] Montana State Univ, Bozeman, MT 59717 USA
[32] Univ Perugia, I-06100 Perugia, Italy
[33] Ist Nazl Fis Nucl, Sez Perugia, I-06123 Perugia, Italy
[34] EGO, I-56021 Pisa, Italy
[35] Syracuse Univ, Syracuse, NY USA
[36] Univ Glasgow, SUPA, Glasgow G12 8QQ, Lanark, Scotland
[37] LIGo Hanford Observ, Richland, WA 99352 USA
[38] RMKI, Wigner RCP, Konkoly Thege Miklos 29-33, H-1121 Budapest, Hungary
[39] Columbia Univ, New York, NY 10027 USA
[40] Stanford Univ, Stanford, CA 94305 USA
[41] Univ Padua, Dipartimento Fis & Astron, I-35131 Padua, Italy
[42] Ist Nazl Fis Nucl, Sez Padova, I-35131 Padua, Italy
[43] CAMK PAN, PL-00716 Warsaw, Poland
[44] Warsaw Univ, Astron Observ, PL-00478 Warsaw, Poland
[45] Univ Birmingham, Birmingham B15 2TT, W Midlands, England
[46] Univ Genoa, I-16146 Genoa, Italy
[47] Ist Nazl Fis Nucl, Sez Genova, Via Dodecaneso 33, I-16146 Genoa, Italy
[48] RRCAT, Indore 452013, Madhya Pradesh, India
[49] Lomonosov Moscow State Univ, Fac Phys, Moscow 119991, Russia
[50] Univ West Scotland, SUPA, Paisley PA1 2BE, Renfrew, Scotland
基金
澳大利亚研究理事会; 美国国家科学基金会; 匈牙利科学研究基金会; 俄罗斯基础研究基金会; 新加坡国家研究基金会; 加拿大自然科学与工程研究理事会;
关键词
MASS; RADIATION; STELLAR; PULSAR; COALESCENCE; SYSTEM; FIELD; LIGO;
D O I
10.1103/PhysRevLett.116.061102
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
On September 14, 2015 at 09: 50: 45 UTC the two detectors of the Laser Interferometer Gravitational-Wave Observatory simultaneously observed a transient gravitational-wave signal. The signal sweeps upwards in frequency from 35 to 250 Hz with a peak gravitational-wave strain of 1.0 x 10(-21). It matches the waveform predicted by general relativity for the inspiral and merger of a pair of black holes and the ringdown of the resulting single black hole. The signal was observed with a matched-filter signal-to-noise ratio of 24 and a false alarm rate estimated to be less than 1 event per 203 000 years, equivalent to a significance greater than 5.1 sigma. The source lies at a luminosity distance of 410(-180)(+160) Mpc corresponding to a redshift z = 0.09(-0.01)(+0.03). In the source frame, the initial black hole masses are 36(-4)(+5)M(circle dot) and 29(-4)(+4)M(circle dot), and the final black hole mass is 62(-4)(+4) M-circle dot, with 3.0(-0.5)(+0.5) M(circle dot)c(2) radiated in gravitational waves. All uncertainties define 90% credible intervals. These observations demonstrate the existence of binary stellar-mass black hole systems. This is the first direct detection of gravitational waves and the first observation of a binary black hole merger.
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页数:16
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