Search for gravitational waves from low mass compact binary coalescence in 186 days of LIGO's fifth science run

被引：99

作者：

Abbott, B. P. ^{[15
]}

Abbott, R. ^{[15
]}

Adhikari, R. ^{[15
]}

Ajith, P. ^{[1
]}

Allen, B. ^{[1
,55
]}

Allen, G. ^{[32
]}

Amin, R. S. ^{[19
]}

Anderson, S. B. ^{[15
]}

Anderson, W. G. ^{[55
]}

Arain, M. A. ^{[43
]}

Araya, M. ^{[15
]}

Armandula, H. ^{[15
]}

Armor, P. ^{[55
]}

Aso, Y. ^{[15
]}

Aston, S. ^{[3
,59
]}

Aufmuth, P. ^{[14
]}

Aulbert, C. ^{[1
]}

Babak, S. ^{[61
]}

Baker, P. ^{[22
]}

Ballmer, S. ^{[15
]}

Barker, C. ^{[16
]}

Barker, D. ^{[16
]}

Barr, B. ^{[44
]}

Barriga, P. ^{[54
]}

Barsotti, L. ^{[18
]}

Barton, M. A. ^{[15
]}

Bartos, I. ^{[8
]}

Bassiri, R. ^{[44
]}

Bastarrika, M. ^{[44
]}

Behnke, B. ^{[61
]}

Benacquista, M. ^{[39
]}

Betzwieser, J. ^{[15
]}

Beyersdorf, P. T. ^{[28
]}

Bilenko, I. A. ^{[23
]}

Billingsley, G. ^{[15
]}

Biswas, R. ^{[55
]}

Black, E. ^{[15
]}

Blackburn, J. K. ^{[15
]}

Blackburn, L. ^{[18
]}

Blair, D. ^{[54
]}

Bland, B. ^{[16
]}

Bodiya, T. P. ^{[18
]}

Bogue, L. ^{[17
]}

Bork, R. ^{[15
]}

Boschi, V. ^{[15
]}

Bose, S. ^{[56
]}

Brady, P. R. ^{[55
]}

Braginsky, V. B. ^{[23
]}

Brau, J. E. ^{[49
]}

Bridges, D. O. ^{[17
]}

机构：

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

[2] Andrews Univ, Berrien Springs, MI 49104 USA

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

[4] CALTECH, CaRT, Pasadena, CA 91125 USA

[5] Cardiff Univ, Cardiff CF24 3AA, S Glam, Wales

[6] Carleton Coll, Northfield, MN 55057 USA

[7] Charles Sturt Univ, Wagga Wagga, NSW 2678, Australia

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

[9] Embry Riddle Aeronaut Univ, Prescott, AZ 86301 USA

[10] Eotvos Lorand Univ, ELTE, H-1053 Budapest, Hungary

[11] Hobart & William Smith Coll, Geneva, NY 14456 USA

[12] Inst Appl Phys, Nizhnii Novgorod 603950, Russia

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

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

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

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

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

[18] MIT, LIGO, Cambridge, MA 02139 USA

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

[20] Louisiana Tech Univ, Ruston, LA 71272 USA

[21] Loyola Univ, New Orleans, LA 70118 USA

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

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

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

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

[26] Northwestern Univ, Evanston, IL 60208 USA

[27] Rochester Inst Technol, Rochester, NY 14623 USA

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

[29] Sonoma State Univ, Rohnert Pk, CA 94928 USA

[30] SE Louisiana Univ, Hammond, LA 70402 USA

[31] Southern Univ, Baton Rouge, LA 70813 USA

[32] Stanford Univ, Stanford, CA 94305 USA

[33] Syracuse Univ, Syracuse, NY 13244 USA

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

[35] Univ Melbourne, Parkville, Vic 3010, Australia

[36] Univ Mississippi, University, MS 38677 USA

[37] Univ Sheffield, Sheffield S10 2TN, S Yorkshire, England

[38] Univ Texas Austin, Austin, TX 78712 USA

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

[40] Trinity Univ, San Antonio, TX 78212 USA

[41] Univ Illes Balears, E-07122 Palma de Mallorca, Spain

[42] Univ Adelaide, Adelaide, SA 5005, Australia

[43] Univ Florida, Gainesville, FL 32611 USA

[44] Univ Glasgow, Glasgow G12 8QQ, Lanark, Scotland

[45] Univ Maryland, College Pk, MD 20742 USA

[46] Univ Massachusetts, Amherst, MA 01003 USA

[47] Univ Michigan, Ann Arbor, MI 48109 USA

[48] Univ Minnesota, Minneapolis, MN 55455 USA

[49] Univ Oregon, Eugene, OR 97403 USA

[50] Univ Rochester, Rochester, NY 14627 USA

来源：

PHYSICAL REVIEW D | 2009年 / 80卷 / 04期

基金：

英国科学技术设施理事会; 美国国家科学基金会;

关键词：

CONSTRAINING POPULATION; SYNTHESIS MODELS; FORMS;

D O I：

10.1103/PhysRevD.80.047101

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report on a search for gravitational waves from coalescing compact binaries, of total mass between 2 and 35M(circle dot), using LIGO observations between November 14, 2006 and May 18, 2007. No gravitational-wave signals were detected. We report upper limits on the rate of compact binary coalescence as a function of total mass. The LIGO cumulative 90%-confidence rate upper limits of the binary coalescence of neutron stars, black holes and black hole-neutron star systems are 1.4x10(-2), 7.3x10(-4) and 3.6x10(-3) yr(-1) L-10(-1), respectively, where L-10 is 10(10) times the blue solar luminosity.

引用

页数：8

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