Search for gravitational waves from intermediate mass binary black holes

被引：47

作者：

Abadie, J. ^{[1
]}

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

Abbott, R. ^{[1
]}

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

Abernathy, M. ^{[3
]}

Accadia, T. ^{[4
]}

Acernese, F. ^{[5
,7
,8
]}

Adams, C. ^{[9
]}

Adhikari, R. ^{[1
]}

Affeldt, C. ^{[10
,11
]}

Agathos, M. ^{[12
]}

Agatsuma, K. ^{[14
]}

Ajith, P. ^{[1
]}

Allen, B. ^{[10
,11
,15
]}

Ceron, E. Amador ^{[15
]}

Amariutei, D. ^{[16
]}

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

Anderson, W. G. ^{[15
]}

Arai, K. ^{[1
]}

Arain, M. A. ^{[16
]}

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

Aston, S. M. ^{[17
]}

Astone, P. ^{[18
]}

Atkinson, D. ^{[20
]}

Aufmuth, P. ^{[10
,11
]}

Aulbert, C. ^{[10
,11
]}

Aylott, B. E. ^{[17
]}

Babak, S. ^{[21
]}

Baker, P. ^{[22
]}

Ballardin, G. ^{[23
]}

Ballmer, S. ^{[24
]}

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

Barker, D. ^{[20
]}

Barone, F. ^{[7
,8
,70
]}

Barr, B. ^{[3
]}

Barsotti, L. ^{[25
]}

Barsuglia, M. ^{[26
]}

Barton, M. A. ^{[20
]}

Bartos, I. ^{[27
]}

Bassiri, R. ^{[3
]}

Bastarrika, M. ^{[3
]}

Basti, A. ^{[28
]}

Batch, J. ^{[20
]}

Bauchrowitz, J. ^{[10
,11
]}

Bauer, Th. S. ^{[12
]}

Bebronne, M. ^{[4
]}

Beck, D. ^{[31
]}

Behnke, B. ^{[21
]}

Bejger, M. ^{[34
]}

Beker, M. G. ^{[12
]}

机构：

[1] LIGO Calif Inst Technol, Pasadena, CA 91125 USA

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

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

[4] Univ Savoie, Lab Annecy le Vieux Phys Particules LAPP, CNRS IN2P3, F-74941 Annecy Le Vieux, France

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

[6] Univ Naples Federico II, Naples, Italy

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

[8] Complesso Univ Monte S Angelo, I-80126 Naples, Italy

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

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

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

[12] Nikhef, Amsterdam, Netherlands

[13] Vrije Univ Amsterdam, NL-1081 HV Amsterdam, Netherlands

[14] Natl Astron Observ Japan, Tokyo 1818588, Japan

[15] Univ Wisconsin, Milwaukee, WI 53201 USA

[16] Univ Florida, Gainesville, FL 32611 USA

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

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

[19] Univ Roma La Sapienza, I-00185 Rome, Italy

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

[21] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Golm, Germany

[22] Montana State Univ, Bozeman, MT 59717 USA

[23] EGO, I-56021 Cascina Pisa, Italy

[24] Syracuse Univ, Syracuse, NY 13244 USA

[25] LIGO Massachusetts Inst Technol, Cambridge, MA 02139 USA

[26] Univ Paris Diderot, Lab AstroParticule & Cosmol APC, CNRS IN2P3, CEA DSM IRFU,Observ Pais, F-75013 Paris, France

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

[28] Ist Nazl Fis Nucl, Sez Pisa, Pisa, Italy

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

[30] Univ Siena, I-53100 Siena, Italy

[31] Stanford Univ, Stanford, CA 94305 USA

[32] IM PAN, PL-00956 Warsaw, Poland

[33] Warsaw Univ, Astron Observ, PL-00478 Warsaw, Poland

[34] CAMK PAN, PL-00716 Warsaw, Poland

[35] Bialystok Univ, PL-15424 Bialystok, Poland

[36] IPJ, PL-05400 Otwock, Poland

[37] Inst Astron, PL-65265 Zielona Gora, Poland

[38] Univ Texas Brownsville & Texas Southmost Coll, Brownsville, TX 78520 USA

[39] San Jose State Univ, San Jose, CA 95192 USA

[40] Moscow MV Lomonosov State Univ, Moscow 119992, Russia

[41] Univ Paris 11, LAL, CNRS IN2P3, F-91898 Orsay, France

[42] CNRS, ESPCI, F-75005 Paris, France

[43] NASA Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[44] Univ Western Australia, Crawley, WA 6009, Australia

[45] Penn State Univ, University Pk, PA 16802 USA

[46] Univ Nice Sophia Antipolis, CNRS, Observ Cote Azur, F-06304 Nice, France

[47] Univ Rennes 1, Inst Phys Rennes, CNRS, F-35042 Rennes, France

[48] IN2P3 CNRS, LMA, F-69622 Lyon, France

[49] Washington State Univ, Pullman, WA 99164 USA

[50] Ist Nazl Fis Nucl, Sez Perugia, Perugia, Italy

来源：

PHYSICAL REVIEW D | 2012年 / 85卷 / 10期

基金：

英国科学技术设施理事会; 美国国家科学基金会; 澳大利亚研究理事会;

关键词：

INSPIRALLING COMPACT BINARIES; GROWTH; CLUSTERS; FORMS; 5TH;

D O I：

10.1103/PhysRevD.85.102004

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the results of a weakly modeled burst search for gravitational waves from mergers of nonspinning intermediate mass black holes in the total mass range 100-450 M-circle dot and with the component mass ratios between 1: and 4:1. The search was conducted on data collected by the LIGO and Virgo detectors between November of 2005 and October of 2007. No plausible signals were observed by the search which constrains the astrophysical rates of the intermediate mass black holes mergers as a function of the component masses. In the most efficiently detected bin centered on 88 + 88 M-circle dot, for nonspinning sources, the rate density upper limit is 0.13 per Mpc(3) per Myr at the 90% confidence level.

引用

页数：13

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