Details
Original language | English |
---|---|
Article number | 122005 |
Journal | Physical Review D - Particles, Fields, Gravitation and Cosmology |
Volume | 83 |
Issue number | 12 |
Publication status | Published - 6 Jun 2011 |
Abstract
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 1-99Mȯ and total masses of 25-100Mȯ. 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 19Mȯ≤m1, m 2≤28Mȯ binary black-hole systems with negligible spin to be no more than 2.0Mpc-3Myr-1 at 90% confidence.
ASJC Scopus subject areas
- Physics and Astronomy(all)
- Nuclear and High Energy Physics
- Physics and Astronomy(all)
- Physics and Astronomy (miscellaneous)
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In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 83, No. 12, 122005, 06.06.2011.
Research output: Contribution to journal › Article › Research › peer review
}
TY - JOUR
T1 - Search for gravitational waves from binary black hole inspiral, merger, and ringdown
AU - The LIGO Scientific Collaboration
AU - Abadie, J.
AU - Abbott, B. P.
AU - Abbott, R.
AU - Abernathy, M.
AU - Accadia, T.
AU - Acernese, F.
AU - Adams, C.
AU - Adhikari, R.
AU - Ajith, P.
AU - Allen, B.
AU - Allen, G. S.
AU - Amador Ceron, E.
AU - Amin, R. S.
AU - Anderson, S. B.
AU - Anderson, W. G.
AU - Antonucci, F.
AU - Arain, M. A.
AU - Araya, M. C.
AU - Aronsson, M.
AU - Aso, Y.
AU - Aston, S. M.
AU - Astone, P.
AU - Atkinson, D.
AU - Aufmuth, P.
AU - Aulbert, C.
AU - Babak, S.
AU - Baker, P.
AU - Ballardin, G.
AU - Ballinger, T.
AU - Ballmer, S.
AU - Barker, D.
AU - Barnum, S.
AU - Barone, F.
AU - Barr, B.
AU - Barriga, P.
AU - Barsotti, L.
AU - Barsuglia, M.
AU - Barton, M. A.
AU - Bartos, I.
AU - Bassiri, R.
AU - Burmeister, O.
AU - Danzmann, K.
AU - Hewitson, M.
AU - Kawazoe, F.
AU - Kim, H.
AU - Lück, H.
AU - Vahlbruch, H.
AU - Wanner, A.
AU - Willke, B.
AU - Yamamoto, K.
AU - Bauchrowitz, Jörg
AU - Bertolini, A.
AU - Bock, Oliver
AU - Born, Michael
AU - Breyer, J.
AU - Brinkmann, Marc
AU - Britzger, Michael
AU - Dahl, Christian
AU - Degallaix, J.
AU - Di Palma, I.
AU - Eberle, Tobias
AU - Fehrmann, Henning
AU - Frede, Maik
AU - Friedrich, D.
AU - Giampanis, S.
AU - Goßler, S.
AU - Graef, C.
AU - Grote, Hartmut
AU - Hage, B.
AU - Khalaidovski, A.
AU - Kringel, Volker
AU - Kuehn, G.
AU - Kwee, P.
AU - Lastzka, Nico
AU - Leong, J.
AU - Machenschalk, B.
AU - Mehmet, Moritz
AU - Meier, T.
AU - Messenger, Chris
AU - Mossavi, K.
AU - Pareja, M.
AU - Pickenpack, M.
AU - Pletsch, H. J.
AU - Prijatelj, M.
AU - Prix, Reinhard
AU - Puncken, O.
AU - Röver, C.
AU - Rüdiger, Albrecht
AU - Salemi, F.
AU - Schilling, R.
AU - Schnabel, R.
AU - Schulz, Bastian
AU - Steinlechner, Sebastian
AU - Tarabrin, Sergey P.
AU - Taylor, John R.
AU - Thüring, André
AU - Veltkamp, C.
AU - Weinert, Michael
AU - Weßels, Peter
AU - Westphal, Tobias
AU - Winkelmann, L.
AU - Winkler, W.
PY - 2011/6/6
Y1 - 2011/6/6
N2 - 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 1-99Mȯ and total masses of 25-100Mȯ. 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 19Mȯ≤m1, m 2≤28Mȯ binary black-hole systems with negligible spin to be no more than 2.0Mpc-3Myr-1 at 90% confidence.
AB - 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 1-99Mȯ and total masses of 25-100Mȯ. 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 19Mȯ≤m1, m 2≤28Mȯ binary black-hole systems with negligible spin to be no more than 2.0Mpc-3Myr-1 at 90% confidence.
UR - http://www.scopus.com/inward/record.url?scp=79960823290&partnerID=8YFLogxK
U2 - 10.1103/PhysRevD.83.122005
DO - 10.1103/PhysRevD.83.122005
M3 - Article
AN - SCOPUS:79960823290
VL - 83
JO - Physical Review D - Particles, Fields, Gravitation and Cosmology
JF - Physical Review D - Particles, Fields, Gravitation and Cosmology
SN - 1550-7998
IS - 12
M1 - 122005
ER -