@Article{AbadieAAAAAAAAAAAAACAAAAAAAAAAAABBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCDDDDDDDDDDDDRDDDPDDDDDDDDEDDDDDDDDDDDEEEEEEEEEEEFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHIIIIIJJJJJJJJJJKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMNNNNNNNNNNNNOOOOOOOOOOOOOOPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPQQRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSTTTTTTTTTTTTTTTTTTTTTTTUVVBVPVVVVVVVVVVVVVVVVVVVVWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWYYYYYYYYYZZZZZZZZZZCC:2012:SeGrWa,
author = "Abadie, J. and Abbott, B. P. and Abbott, R. and Abbott, T. D. and
Abernathy, M. and Accadia, T. and Acernese, F. and Adams, C. and
Adhikari, R. and Affeldt, C. and Agathos, M. and Agatsuma, K. and
Ajith, P. and Allen, B. and Ceron, E. Amador and Amariutei, D. and
Anderson, S. B. and Anderson, W. G. and Arai, K. and Arain, M. A.
and Araya, M. C. and Aston, S. M. and Astone, P. and Atkinson, D.
and Aufmuth, P. and Aulbert, C. and Aylott, B. E. and Babak, S.
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C. B. and Barker, D. and Barone, F. and Barr, B. and Barsotti, L.
and Barsuglia, M. and Barton, M. A. and Bartos, I. and Bassiri, R.
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and Bauer, Th. S. and Bebronne, M. and Beck, D. and Behnke, B. and
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Belopolski, I. and Benacquista, M. and Berliner, J. M. and
Bertolini, A. and Betzwieser, J. and Beveridge, N. and Beyersdorf,
P. T. and Bilenko, I. A. and Billingsley, G. and Birch, J. and
Biswas, R. and Bitossi, M. and Bizouard, M. A. and Black, E. and
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Bondarescu, R. and Bondu, F. and Bonelli, L. and Bonnand, R. and
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Bouhou, B. and Braccini, B. S. and Bradaschia, C. and Brady, P. R.
and Braginsky, V. B. and Branchesi, M. and Brau, J. E. and Breyer,
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Zweizig, J. and Collaboration, LIGO Sci and Collaboration, Virgo",
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{Instituto Nacional de Pesquisas Espaciais (INPE)}",
title = "Search for gravitational waves from intermediate mass binary black
holes",
journal = "Physical Review D",
year = "2012",
volume = "85",
number = "10",
pages = "102004",
note = "{Setores de Atividade: Pesquisa e desenvolvimento
cient{\'{\i}}fico.}",
keywords = "Black Holes, Gravitational Waves, LIGO, Compact Binaries.",
abstract = "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 100450 M and with the
component mass ratios between 1:1 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 ef\ficiently detected
bin centered on 88 þ 88 M , for nonspinning sources, the rate
density upper limit is 0.13 per Mpc 3 per Myr at the 90%
con\fidence level.",
doi = "10.1103/PhysRevD.85.102004",
url = "http://dx.doi.org/10.1103/PhysRevD.85.102004",
issn = "1550-2368 and 1550-7998",
label = "lattes: 2701172317925881 162 AbadieCost:2012:SeGrWa",
language = "en",
targetfile = "Abadie-Search for-PhysRevD.85.102004[1].pdf",
urlaccessdate = "28 abr. 2024"
}