期刊
PHYSICAL REVIEW D
卷 83, 期 12, 页码 -出版社
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.83.122005
关键词
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资金
- United States National Science Foundation
- Science and Technology Facilities Council of the United Kingdom
- Max-Planck-Society
- State of Niedersachsen/Germany
- Australian Research Council
- Council of Scientific and Industrial Research of India
- Istituto Nazionale di Fisica Nucleare of Italy
- Spanish Ministerio de Educacion y Ciencia
- Conselleria d'Economia Hisenda i Innovacio of the Govern de les Illes Balears
- Foundation for Fundamental Research on Matter
- Netherlands Organisation for Scientific Research
- Polish Ministry of Science and Higher Education
- Foundation for Polish Science
- Royal Society
- Scottish Funding Council
- Scottish Universities Physics Alliance
- National Aeronautics and Space Administration
- Carnegie Trust
- Leverhulme Trust
- David and Lucile Packard Foundation
- Research Corporation
- Alfred P. Sloan Foundation
- Grants-in-Aid for Scientific Research [10J02592] Funding Source: KAKEN
- Division Of Physics
- Direct For Mathematical & Physical Scien [0757058, 0757957] Funding Source: National Science Foundation
- STFC [ST/I006242/1, ST/I001085/1, ST/I001026/1, PP/F001118/1, ST/I000887/1, ST/I006285/1, PP/F00110X/1, Gravitational Waves, ST/F01032X/1] Funding Source: UKRI
- Science and Technology Facilities Council [ST/I001026/1 Gravitational Waves, ST/I000887/1, ST/I006285/1, ST/I001085/1, ST/F01032X/1, PP/F00110X/1, ST/I000887/1 Gravitational Waves, PP/F001118/1, ST/I006242/1, ST/I001026/1, Gravitational Waves, ST/I006242/1 Gravitational Waves] Funding Source: researchfish
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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