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SCI Article

Search for gravitational waves from binary black hole inspiral, merger, and ringdown in LIGO-Virgo d
Author Kim, K. (Seoul 133791); Lee, H. K. (Seoul 133791); Kim, K. (Seoul 133791); Lee, H. K. (Seoul 133791);
Corresponding Author Info Aasi, J (reprint author), CALTECH, LIGO, Pasadena, CA 91125 USA.
E-mail 씠硫붿씪 븘씠肄
Document Type Article
Source PHYSICAL REVIEW D Volume:87 Issue:2 Pages:- Published:2013
Times Cited 49
External Information PDF 븘씠肄http://dx.doi.org/10.1103/PhysRevD.87.022002
Abstract We report a search for gravitational waves from the inspiral, merger and ringdown of binary black holes (BBH) with total mass between 25 and 100 solar masses, in data taken at the LIGO and Virgo observatories between July 7, 2009 and October 20, 2010. The maximum sensitive distance of the detectors over this period for a (20, 20)M-circle dot coalescence was 300 Mpc. No gravitational wave signals were found. We thus report upper limits on the astrophysical coalescence rates of BBH as a function of the component masses for nonspinning components, and also evaluate the dependence of the search sensitivity on component spins aligned with the orbital angular momentum. We find an upper limit at 90% confidence on the coalescence rate of BBH with nonspinning components of mass between 19 and 28M(circle dot) of 3:3 x 10(-7) mergers Mpc(-3) yr(-1).
Web of Science Categories Astronomy & Astrophysics; Physics, Particles & Fields
Funding Australian Research Council; International Science Linkages program of the Commonwealth of Australia; Council of Scientific and Industrial Research of India; Istituto Nazionale di Fisica Nucleare of Italy; Spanish Ministerio de Economia y Competitividad;
Language English
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