@Article{AasiAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAABBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBBCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCDCDDDDDDDDDDDDDDDDDDDRDDDDDDDDDDDDDDDDDDDDDEEEEEEEEEEEEEFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFFGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGGHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHHIIIIIIJJJJJJJJJJJKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKKLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLLMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMMNNNNNNNNNNNNNNNNOOOOOOOOOOOOOOPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPPQQQQQRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRRSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSSTTTTTTTTTTTTTTTTTTTTTUUUUVVVVVVVVVVVVVVVVVVVVVVVVVVVVVVVWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWWYYYYYYYYZZZZZZZZZZ:2014:SeGrRa,
author = "Aasi, J. and Abbott, B. P. and Abbott, R. and Abbott, T. and
Abernathy, M. R. and Accadia, T. and Acernese, F. and Ackley, K.
and Adams, C. and Adams, T. and Addesso, P. and Adhikari, R. X.
and Affeldt, C. and Agathos, M. and Aggarwal, N. and Aguiar,
Odylio Denys de and Ain, A. and Ajith, P. and Alemic, A. and
Allen, B. and Allocca, A. and Amariutei, D. and Andersen, M. and
Anderson, R. and Anderson, S. B. and Anderson, W. G. and Arai, K.
and Araya, M. C. and Arceneaux, C. and Areeda, J. and Aston, S. M.
and Astone, P. and Aufmuth, P. and Aulbert, C. and Austin, L. and
Aylott, B. E. and Babak, S. and Baker, P. T. and Ballardin, G. and
Ballmer, S. W. and Barayoga, J. C. and Barbet, M. and Barish, B.
C. 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. and
Basti, A. and Batch, J. C. and Bauchrowitz, J. and Bauer, T. S.
and Bavigadda, V. and Behnke, B. and Bejger, M. and Beker, M. G.
and Belczynski, C. and Bell, A. S. and Bell, C. and Bergmann, G.
and Bersanetti, D. and Bertolini, A. and Betzwieser, J. and
Beyersdorf, P. T. and Bilenko, I. A. and Billingsley, G. and
Birch, J. and Biscans, S. and Bitossi, M. and Bizouard, M. A. and
Black, E. and Blackburn, J. K. and Blackburn, L. and Blair, D. and
Bloemen, S. and Blom, M. and Bock, O. and Bodiya, T. P. and Boer,
M. and Bogaert, G. and Bogan, C. and Bond, C. and Bondu, F. and
Bonelli, L. and Bonnand, R. and Bork, R. and Born, M. and Boschi,
V. and Bose, S. and Bosi, L. and Bradaschia, C. and Brady, P. R.
and Braginsky, V. B. and Branchesi, M. and Brau, J. E. and Briant,
T. and Bridges, D. O. and Brillet, A. and Brinkmann, M. and
Brisson, V. and Brooks, A. F. and Brown, D. A. and Brown, D. D.
and Br{\"u}ckner, F. and Buchman, S. and Bulik, T. and Bulten, H.
J. and Buonanno, A. and Burman, R. and Buskulic, D. and Buy, C.
and Cadonati, L. and Cagnoli, G. and Calder{\'o}n Bustillo, J.
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and Canuel, B. and Cao, J. and Capano, C. D. and Carbognani, F.
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Chakraborty, R. and Chalermsongsak, T. and Chamberlin, S. J. and
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and Chen, Y. and Chincarini, A. and Chiummo, A. and Cho, H. S. and
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Augusto and Coughlin, M. W. and Coughlin, S. and Coulon, J. -P.
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affiliation = "{} and {} and {} and {} and {} and {} and {} and {} and {} and {}
and {} and {} and {} and {} and {} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {} and {} and {} and {} and {} and
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and {} and {} and {} and {} and {} and {} and {Instituto Nacional
de Pesquisas Espaciais (INPE)}",
title = "Search for gravitational radiation from intermediate mass black
hole binaries in data from the second LIGO-Virgo joint science
run",
journal = "Physical Review D",
year = "2014",
volume = "89",
number = "12",
pages = "122003 (15pp.)",
abstract = "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
<200Mpc, 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 450M 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 88M
black holes and is equal to 0.12Mpc-3Myr-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 ~20%.",
doi = "10.1103/PhysRevD.89.122003",
url = "http://dx.doi.org/10.1103/PhysRevD.89.122003",
issn = "1550-2368 and 1550-7998",
label = "scopus 2014-07
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language = "en",
targetfile = "PhysRevD.89.122003.pdf",
urlaccessdate = "27 abr. 2024"
}