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- Title:
- Search for gravitational radiation from intermediate mass black hole binaries in data from the second LIGO-Virgo joint science run
- Aasi, J.
- Abbott, B. P.
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- Abernathy, M. R.
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- Chamberlin, S. J.
- Chao, S.
- Charlton, P.
- Chassande-Mottin, E.
- Chen, X.
- Chen, Y.
- Chincarini, A.
- Chiummo, A.
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- Chow, J.
- Christensen, N.
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- Gustafson, R.
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- Heidmann, A.
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- Heitmann, H.
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- Huerta, E.
- Hughey, B.
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- Huynh-Dinh, T.
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- Perimeter Inst Theoret Phys
- Amer Univ
- Univ Adelaide
- Raman Res Inst
- Korea Inst Sci & Technol Informat
- Bialystok Univ
- Univ Southampton
- IISER TVM
- Inst Appl Phys
- Seoul Natl Univ
- Hanyang Univ
- IM PAN
- NCBJ
- Inst Plasma Res
- Univ Melbourne
- Monash Univ
- Univ Strathclyde
- ESPCI
- Argentinian Gravitat Wave Grp
- Univ Camerino
- Univ Texas Austin
- Southern Univ
- A&M Coll
- Coll William & Mary
- IISER Kolkata
- Natl Inst Math Sci
- Hobart & William Smith Coll
- RRCAT
- Univ West Scotland
- Inst Astron
- Indian Inst Technol
- Universidade Estadual Paulista (UNESP)
- Andrews Univ
- Trinity Univ
- Univ Washington
- SE Louisiana Univ
- Abilene Christian Univ
- 1550-7998
- United States National Science Foundation for the construction and operation of the LIGO Laboratory
- Science and Technology Facilities Council of the United Kingdom
- Max-Planck-Society
- State of Niedersachsen/Germany
- 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
- 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
- FOCUS Programme of Foundation for Polish Science
- Royal Society
- Scottish Funding Council
- Scottish Universities Physics Alliance
- National Aeronautics and Space Administration
- OTKA of Hungary
- Lyon Institute of Origins (LIO)
- National Research Foundation of Korea
- Industry Canada
- Province of Ontario through the Ministry of Economic Development and Innovation
- National Science and Engineering Research Council Canada
- Carnegie Trust
- Leverhulme Trust
- David and Lucile Packard Foundation
- Research Corporation
- Alfred P. Sloan Foundation
- This paper reports on an unmodeled, all-sky search for gravitational waves from merging intermediate mass black hole binaries (IMBHB). The search was performed on data from the second joint science run of the LIGO and Virgo detectors (July 2009-October 2010) and was sensitive to IMBHBs with a range up to similar to 200 Mpc, averaged over the possible sky positions and inclinations of the binaries with respect to the line of sight. No significant candidate was found. Upper limits on the coalescence-rate density of nonspinning IMBHBs with total masses between 100 and 450 M-circle dot and mass ratios between 0.25 and 1 were placed by combining this analysis with an analogous search performed on data from the first LIGO-Virgo joint science run (November 2005-October 2007). The most stringent limit was set for systems consisting of two 88 M-circle dot black holes and is equal to 0.12 Mpc(-3) Myr(-1) at the 90% confidence level. This paper also presents the first estimate, for the case of an unmodeled analysis, of the impact on the search range of IMBHB spin configurations: the visible volume for IMBHBs with nonspinning components is roughly doubled for a population of IMBHBs with spins aligned with the binary's orbital angular momentum and uniformly distributed in the dimensionless spin parameter up to 0.8, whereas an analogous population with antialigned spins decreases the visible volume by similar to 20%.
- 12-Jun-2012
- Physical Review D. College Pk: Amer Physical Soc, v. 89, n. 12, 15 p., 2012.
- 15
- Amer Physical Soc
- http://dx.doi.org/10.1103/PhysRevD.89.122003
- Acesso restrito
- outro
- http://repositorio.unesp.br/handle/11449/117042
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