Search for gravitational waves from binary black hole inspiral, merger, and ringdown

Research output: Contribution to journalArticleResearchpeer review

Authors

  • The LIGO Scientific Collaboration
  • O. Burmeister
  • K. Danzmann
  • H. Lück
  • H. Vahlbruch
  • Jörg Bauchrowitz
  • A. Bertolini
  • Oliver Bock
  • Michael Born
  • J. Breyer
  • Marc Brinkmann
  • Michael Britzger
  • Christian Dahl
  • J. Degallaix
  • I. Di Palma
  • Tobias Eberle
  • Henning Fehrmann
  • Maik Frede
  • D. Friedrich
  • S. Giampanis
  • S. Goßler
  • C. Graef
  • Hartmut Grote
  • B. Hage
  • A. Khalaidovski
  • Volker Kringel
  • G. Kuehn
  • P. Kwee
  • Nico Lastzka
  • J. Leong
  • B. Machenschalk
  • Moritz Mehmet
  • T. Meier
  • Chris Messenger
  • K. Mossavi
  • M. Pareja
  • M. Pickenpack
  • H. J. Pletsch
  • M. Prijatelj
  • Reinhard Prix
  • O. Puncken
  • C. Röver
  • Albrecht Rüdiger
  • F. Salemi
  • R. Schilling
  • R. Schnabel
  • Bastian Schulz
  • Sebastian Steinlechner
  • Sergey P. Tarabrin
  • John R. Taylor
  • André Thüring
  • C. Veltkamp
  • Michael Weinert
  • Peter Weßels
  • Tobias Westphal
  • L. Winkelmann
  • W. Winkler

External Research Organisations

  • California Institute of Caltech (Caltech)
  • Universite de Savoie
  • Monte S. Angelo University Federico II
  • Universita di Salerno
  • Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • University of Wisconsin Milwaukee
  • Stanford University
  • Louisiana State University
  • University of Florida
  • National Science Foundation (NSF)
  • Montana State University
  • Carleton College
  • Massachusetts Institute of Technology
  • University of Western Australia
  • Observatoire de Paris (OBSPARIS)
  • Columbia University
  • University of Glasgow
  • Istituto Nazionale di Fisica Nucleare (INFN)
  • University of Birmingham
  • European Gravitational Observatory (EGO)
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Details

Original languageEnglish
Article number122005
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume83
Issue number12
Publication statusPublished - 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

Cite this

Search for gravitational waves from binary black hole inspiral, merger, and ringdown. / The LIGO Scientific Collaboration; Burmeister, O.; Danzmann, K. et al.
In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 83, No. 12, 122005, 06.06.2011.

Research output: Contribution to journalArticleResearchpeer review

The LIGO Scientific Collaboration, Burmeister, O, Danzmann, K, Lück, H, Vahlbruch, H, Bauchrowitz, J, Bertolini, A, Bock, O, Born, M, Breyer, J, Brinkmann, M, Britzger, M, Dahl, C, Degallaix, J, Di Palma, I, Eberle, T, Fehrmann, H, Frede, M, Friedrich, D, Giampanis, S, Goßler, S, Graef, C, Grote, H, Hage, B, Khalaidovski, A, Kringel, V, Kuehn, G, Kwee, P, Lastzka, N, Leong, J, Machenschalk, B, Mehmet, M, Meier, T, Messenger, C, Mossavi, K, Pareja, M, Pickenpack, M, Pletsch, HJ, Prijatelj, M, Prix, R, Puncken, O, Röver, C, Rüdiger, A, Salemi, F, Schilling, R, Schnabel, R, Schulz, B, Steinlechner, S, Tarabrin, SP, Taylor, JR, Thüring, A, Veltkamp, C, Weinert, M, Weßels, P, Westphal, T, Winkelmann, L & Winkler, W 2011, 'Search for gravitational waves from binary black hole inspiral, merger, and ringdown', Physical Review D - Particles, Fields, Gravitation and Cosmology, vol. 83, no. 12, 122005. https://doi.org/10.1103/PhysRevD.83.122005
The LIGO Scientific Collaboration, Burmeister, O., Danzmann, K., Lück, H., Vahlbruch, H., Bauchrowitz, J., Bertolini, A., Bock, O., Born, M., Breyer, J., Brinkmann, M., Britzger, M., Dahl, C., Degallaix, J., Di Palma, I., Eberle, T., Fehrmann, H., Frede, M., Friedrich, D., ... Winkler, W. (2011). Search for gravitational waves from binary black hole inspiral, merger, and ringdown. Physical Review D - Particles, Fields, Gravitation and Cosmology, 83(12), Article 122005. https://doi.org/10.1103/PhysRevD.83.122005
The LIGO Scientific Collaboration, Burmeister O, Danzmann K, Lück H, Vahlbruch H, Bauchrowitz J et al. Search for gravitational waves from binary black hole inspiral, merger, and ringdown. Physical Review D - Particles, Fields, Gravitation and Cosmology. 2011 Jun 6;83(12):122005. doi: 10.1103/PhysRevD.83.122005
The LIGO Scientific Collaboration ; Burmeister, O. ; Danzmann, K. et al. / Search for gravitational waves from binary black hole inspiral, merger, and ringdown. In: Physical Review D - Particles, Fields, Gravitation and Cosmology. 2011 ; Vol. 83, No. 12.
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title = "Search for gravitational waves from binary black hole inspiral, merger, and ringdown",
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.",
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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 -