Search for gravitational waves from binary black hole inspiral, merger, and ringdown

被引:90
|
作者
Abadie, J. [1 ]
Abbott, B. P. [1 ]
Abbott, R. [1 ]
Abernathy, M. [87 ]
Accadia, T. [36 ]
Acernese, F. [20 ,21 ]
Adams, C. [39 ]
Adhikari, R. [1 ]
Ajith, P. [1 ]
Allen, B. [3 ,100 ]
Allen, G. S. [73 ]
Ceron, E. Amador [100 ]
Amin, R. S.
Anderson, S. B. [1 ]
Anderson, W. G. [100 ]
Antonucci, F. [28 ]
Arain, M. A. [86 ]
Araya, M. C. [1 ]
Aronsson, M. [1 ]
Aso, Y. [1 ]
Aston, S. M. [85 ]
Astone, P. [28 ]
Atkinson, D. [38 ]
Aufmuth, P. [3 ,37 ]
Aulbert, C. [3 ,37 ]
Babak, S. [2 ]
Baker, P. [45 ]
Ballardin, G. [13 ]
Ballinger, T. [10 ]
Ballmer, S. [1 ]
Barker, D. [38 ]
Barnum, S. [40 ]
Barone, F. [20 ,22 ]
Barr, B. [87 ]
Barriga, P. [99 ]
Barsotti, L. [40 ]
Barsuglia, M. [5 ]
Barton, M. A. [38 ]
Bartos, I. [12 ]
Bassiri, R. [87 ]
Bastarrika, M. [87 ]
Bauchrowitz, J. [3 ,37 ]
Bauer, Th. S. [49 ]
Behnke, B. [2 ]
Beker, M. G. [49 ]
Belletoile, A. [36 ]
Benacquista, M. [80 ]
Bertolini, A. [3 ,37 ]
Betzwieser, J. [1 ]
Beveridge, N. [87 ]
机构
[1] CALTECH, LIGO, Pasadena, CA 91125 USA
[2] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Golm, Germany
[3] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany
[4] Andrews Univ, Berrien Springs, MI 49104 USA
[5] Univ Paris Diderot, Lab AstroParticule & Cosmol APC, Observ Paris, CNRS,IN2P3,CEA,DSM,IRFU, F-75013 Paris, France
[6] Australian Natl Univ, Canberra, ACT 0200, Australia
[7] Calif State Univ Fullerton, Fullerton, CA 92831 USA
[8] Caltech CaRT, Pasadena, CA 91125 USA
[9] Cardiff Univ, Cardiff CF24 3AA, S Glam, Wales
[10] Carleton Coll, Northfield, MN 55057 USA
[11] Charles Sturt Univ, Wagga Wagga, NSW 2678, Australia
[12] Columbia Univ, New York, NY 10027 USA
[13] EGO, I-56021 Cascina, PI, Italy
[14] Embry Riddle Aeronaut Univ, Prescott, AZ 86301 USA
[15] Eotvos Lorand Univ, H-1117 Budapest, Hungary
[16] Hobart & William Smith Coll, Geneva, NY 14456 USA
[17] Ist Nazl Fis Nucl, Sez Firenze, I-50019 Sesto Fiorentino, Italy
[18] Univ Urbino Carlo Bo, I-61029 Urbino, Italy
[19] Ist Nazl Fis Nucl, Sez Genova, I-16146 Genoa, Italy
[20] Ist Nazl Fis Nucl, Sez Napoli, Naples, Italy
[21] Univ Naples Federico II, I-80126 Naples, Italy
[22] Univ Salerno, I-84084 Salerno, Italy
[23] Ist Nazl Fis Nucl, Sez Perugia, I-06123 Perugia, Italy
[24] Univ Perugia, I-06123 Perugia, Italy
[25] Ist Nazl Fis Nucl, Sez Pisa, Pisa, Italy
[26] Univ Pisa, I-56127 Pisa, Italy
[27] Univ Siena, I-53100 Siena, Italy
[28] Ist Nazl Fis Nucl, Sez Roma, Rome, Italy
[29] Univ Roma La Sapienza, I-00185 Rome, Italy
[30] Univ Roma Tor Vergata, I-00133 Rome, Italy
[31] Univ Aquila, I-67100 Laquila, Italy
[32] Inst Appl Phys, Nizhnii Novgorod 603950, Russia
[33] Interuniv Ctr Astron & Astrophys, Pune 411007, Maharashtra, India
[34] Univ Paris 11, LAL, IN2P3, CNRS, F-91898 Orsay, France
[35] CNRS, ESPCI, F-75005 Paris, France
[36] Univ Savoie, LAPP, CNRS, IN2P3, F-74941 Annecy Le Vieux, France
[37] Leibniz Univ Hannover, D-30167 Hannover, Germany
[38] LIGO Hanford Observ, Richland, WA 99352 USA
[39] LIGO Livingston Observ, Livingston, LA 70754 USA
[40] MIT, LIGO, Cambridge, MA 02139 USA
[41] CNRS, IN2P3, LMA, F-69622 Villeurbanne, France
[42] Louisiana State Univ, Baton Rouge, LA 70803 USA
[43] Louisiana Tech Univ, Ruston, LA 71272 USA
[44] McNeese State Univ, Lake Charles, LA 70609 USA
[45] Montana State Univ, Bozeman, MT 59717 USA
[46] Moscow MV Lomonosov State Univ, Moscow 119992, Russia
[47] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[48] Natl Astron Observ Japan, Tokyo 1818588, Japan
[49] Nikhef, Amsterdam, Netherlands
[50] Vrije Univ Amsterdam, NL-1081 HV Amsterdam, Netherlands
来源
PHYSICAL REVIEW D | 2011年 / 83卷 / 12期
基金
美国国家航空航天局; 美国国家科学基金会; 英国科学技术设施理事会; 澳大利亚研究理事会;
关键词
MODELING KICKS; MASS; COALESCENCE; SPIN; FILTERS; CHOICE; RATES;
D O I
10.1103/PhysRevD.83.122005
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the first modeled search for gravitational waves using the complete binary black-hole gravitational waveform from inspiral through the merger and ringdown for binaries with negligible component spin. We searched approximately 2 years of LIGO data, taken between November 2005 and September 2007, for systems with component masses of 1-99M(circle dot) and total masses of 25-100M(circle dot). We did not detect any plausible gravitational-wave signals but we do place upper limits on the merger rate of binary black holes as a function of the component masses in this range. We constrain the rate of mergers for 19M(circle dot) <= m(1), m(2) <= 28M(circle dot) binary black-hole systems with negligible spin to be no more than 2.0 Mpc(-3) Myr(-1) at 90% confidence.
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页数:20
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