Search for Gravitational Waves Associated with Gamma-Ray Bursts during the First Advanced LIGO Observing Run and Implications for the Origin of GRB 150906B

被引：46

作者：

Abbott, B. P. ^{[1
]}

Abbott, R. ^{[1
]}

Abbott, T. D. ^{[2
]}

Abernathy, M. R. ^{[3
]}

Acernese, F. ^{[4
,5
]}

Ackley, K. ^{[6
]}

Adams, C. ^{[7
]}

Adams, T. ^{[8
]}

Addesso, P. ^{[9
,10
]}

Adhikari, R. X. ^{[1
]}

Adya, V. B. ^{[11
]}

Affeldt, C. ^{[11
]}

Agathos, M. ^{[12
]}

Agatsuma, K. ^{[12
]}

Aggarwal, N. ^{[13
]}

Aguiar, O. D. ^{[14
]}

Aiello, L. ^{[15
,16
]}

Ain, A. ^{[17
]}

Ajith, P. ^{[18
]}

Allen, B. ^{[11
,19
,20
]}

Allocca, A. ^{[21
,22
]}

Altin, P. A. ^{[23
]}

Ananyeva, A. ^{[1
]}

Anderson, S. B. ^{[1
]}

Anderson, W. G. ^{[19
]}

Appert, S. ^{[1
]}

Arai, K. ^{[1
]}

Araya, M. C. ^{[1
]}

Areeda, J. S. ^{[24
]}

Arnaud, N. ^{[25
]}

Arun, K. G. ^{[26
]}

Ascenzi, S. ^{[16
,27
]}

Ashton, G. ^{[11
]}

Ast, M. ^{[28
]}

Aston, S. M. ^{[7
]}

Astone, P. ^{[29
]}

Aufmuth, P. ^{[20
]}

Aulbert, C. ^{[11
]}

Avila-Alvarez, A. ^{[24
]}

Babak, S. ^{[30
]}

Bacon, P. ^{[31
]}

Bader, M. K. M. ^{[12
]}

Baker, P. T. ^{[32
]}

Baldaccini, F. ^{[33
,34
]}

Ballardin, G. ^{[35
]}

Ballmer, S. W. ^{[36
]}

Barayoga, J. C. ^{[1
]}

Barclay, S. E. ^{[37
]}

Barish, B. C. ^{[1
]}

Barker, D. ^{[11
,38
]}

机构：

[1] CALTECH, LIGO, Pasadena, CA 91125 USA

[2] Louisiana State Univ, Baton Rouge, LA 70803 USA

[3] Amer Univ, Washington, DC 20016 USA

[4] Univ Salerno, I-84084 Salerno, Italy

[5] Complesso Univ Monte S Angelo, Ist Nazl Fis Nucl, Sez Napoli, I-80126 Naples, Italy

[6] Univ Florida, Gainesville, FL 32611 USA

[7] LIGO Livingston Observ, Livingston, LA 70754 USA

[8] Univ Savoie Mont Blanc, LAPP, CNRS, IN2P3, F-74941 Annecy Le Vieux, France

[9] Univ Sannio Benevento, I-82100 Benevento, Italy

[10] Ist Nazl Fis Nucl, Sez Napoli, Naples, Italy

[11] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany

[12] Nikhef, Sci Pk, NL-1098 XG Amsterdam, Netherlands

[13] MIT, LIGO, 77 Massachusetts Ave, Cambridge, MA 02139 USA

[14] Inst Nacl Pesquisas Espaciais, BR-12227010 Sao Paulo, Brazil

[15] Ist Nazl Fis Nucl, Gran Sasso Sci Inst, I-67100 Laquila, Italy

[16] Ist Nazl Fis Nucl, Sez Roma Tor Vergata, Rome, Italy

[17] Interuniv Ctr Astron & Astrophys, Pune 411007, Maharashtra, India

[18] Tata Inst Fundamental Res, Int Ctr Theoret Sci, Bangalore 560089, Karnataka, India

[19] Univ Wisconsin, Milwaukee, WI 53201 USA

[20] Leibniz Univ Hannover, D-30167 Hannover, Germany

[21] Univ Pisa, I-56127 Pisa, Italy

[22] Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy

[23] Australian Natl Univ, Canberra, ACT 0200, Australia

[24] Calif State Univ Fullerton, Fullerton, CA 92831 USA

[25] Univ Paris Sud, LAL, CNRS, IN2P3,Univ Paris Saclay, F-91898 Orsay, France

[26] Chennai Math Inst, Madras 603103, Tamil Nadu, India

[27] Univ Roma Tor Vergata, I-00133 Rome, Italy

[28] Univ Hamburg, D-22761 Hamburg, Germany

[29] Ist Nazl Fis Nucl, Sez Roma, Rome, Italy

[30] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Potsdam, Germany

[31] Univ Paris Diderot, APC, AstroParticule & Cosmol, CNRS,IN2P3,CEA,Irfu,Observ Paris,Sorbonne Paris C, F-75205 Paris 13, France

[32] West Virginia Univ, Morgantown, WV 26506 USA

[33] Univ Perugia, I-06123 Perugia, Italy

[34] Ist Nazl Fis Nucl, Sez Perugia, I-06123 Perugia, Italy

[35] EGO, I-56021 Pisa, Italy

[36] Syracuse Univ, Syracuse, NY 13244 USA

[37] Univ Glasgow, SUPA, Glasgow G12 8QQ, Lanark, Scotland

[38] LIGO Hanford Observ, Richland, WA 99352 USA

[39] Wigner RCP, RMKI, Konkoly Thege Miklos Ut 29-33, H-1121 Budapest, Hungary

[40] Columbia Univ, New York, NY 10027 USA

[41] Stanford Univ, Stanford, CA 94305 USA

[42] Univ Padua, Dipartimento Fis & Astron, I-35131 Padua, Italy

[43] Ist Nazl Fis Nucl, Sez Padova, I-35131 Padua, Italy

[44] MTA Eotvos Univ, Lendulet Astrophys Res Grp, H-1117 Budapest, Hungary

[45] Polish Acad Sci, Nicolaus Copernicus Astron Ctr, PL-00716 Warsaw, Poland

[46] Georgia Inst Technol, Ctr Relativist Astrophys, Atlanta, GA 30332 USA

[47] Georgia Inst Technol, Sch Phys, Atlanta, GA 30332 USA

[48] Univ Birmingham, Birmingham B15 2TT, W Midlands, England

[49] Univ Genoa, I-16146 Genoa, Italy

[50] Ist Nazl Fis Nucl, Sez Genova, I-16146 Genoa, Italy

来源：

ASTROPHYSICAL JOURNAL | 2017年 / 841卷 / 02期

基金：

新加坡国家研究基金会; 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; 巴西圣保罗研究基金会;

关键词：

binaries: close; gamma-ray burst: general; gravitational waves; COOLED ACCRETION DISKS; DOUBLE NEUTRON-STARS; EQUATION-OF-STATE; BAND FOLLOW-UP; BLACK-HOLE; MASS-DISTRIBUTION; PRECURSOR ACTIVITY; EXTENDED EMISSION; RELATIVISTIC JETS; UNUSUAL SUPERNOVA;

D O I：

10.3847/1538-4357/aa6c47

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the results of the search for gravitational waves (GWs) associated with gamma-ray bursts detected during the first observing run of the Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO). We find no evidence of a GW signal for any of the 41 gamma-ray bursts for which LIGO data are available with sufficient duration. For all gamma-ray bursts, we place lower bounds on the distance to the source using the optimistic assumption that GWs with an energy of 10(-2)M(circle dot)c(2). were emitted within the 16-500 Hz band, and we find a median 90% confidence limit of 71 Mpc at 150 Hz. For the subset of 19 short/hard gamma-ray bursts, we place lower bounds on distance with a median 90% confidence limit of 90 Mpc for binary neutron star (BNS) coalescences, and 150 and 139 Mpc for neutron star-black hole coalescences with spins aligned to the orbital angular momentum and in a generic configuration, respectively. These are the highest distance limits ever achieved by GW searches. We also discuss in detail the results of the search for GWs associated with GRB 150906B, an event that was localized by the InterPlanetary Network near the local galaxy NGC 3313, which is at a luminosity distance of 54 Mpc (z = 0.0124). Assuming the gamma-ray emission is beamed with a jet half-opening angle <= 30 degrees, we exclude a BNS and a neutron star-black hole in NGC 3313 as the progenitor of this event with confidence > 99%. Further, we exclude such progenitors up to a distance of 102 Mpc and 170 Mpc, respectively.

引用

页数：18

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