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

J. Abadie; B. P. Abbott; R. Abbott; M. Abernathy; T. Accadia; F. Acernese; C. Adams; R. Adhikari; P. Ajith; B. Allen; G. S. Allen; E. Amador Ceron; R. S. Amin; S. B. Anderson; W. G. Anderson; F. Antonucci; M. A. Arain; M. C. Araya; M. Aronsson; Y. Aso; S. M. Aston; P. Astone; D. Atkinson; P. Aufmuth; C. Aulbert; S. Babak; P. Baker; G. Ballardin; T. Ballinger; S. Ballmer; D. Barker; S. Barnum; F. Barone; B. Barr; P. Barriga; L. Barsotti; M. Barsuglia; M. A. Barton; I. Bartos; R. Bassiri; M. Bastarrika; J. Bauchrowitz; Th S. Bauer; B. Behnke; M. G. Beker; A. Belletoile; M. Benacquista; A. Bertolini; J. Betzwieser; N. Beveridge

doi:10.1103/PhysRevD.83.122005

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

J. Abadie^*, B. P. Abbott, R. Abbott, M. Abernathy, T. Accadia, F. Acernese, C. Adams, R. Adhikari, P. Ajith, B. Allen, G. S. Allen, E. Amador Ceron, R. S. Amin, S. B. Anderson, W. G. Anderson, F. Antonucci, M. A. Arain, M. C. Araya, M. Aronsson, Y. AsoS. M. Aston, P. Astone, D. Atkinson, P. Aufmuth, C. Aulbert, S. Babak, P. Baker, G. Ballardin, T. Ballinger, S. Ballmer, D. Barker, S. Barnum, F. Barone, B. Barr, P. Barriga, L. Barsotti, M. Barsuglia, M. A. Barton, I. Bartos, R. Bassiri, M. Bastarrika, J. Bauchrowitz, Th S. Bauer, B. Behnke, M. G. Beker, A. Belletoile, M. Benacquista, A. Bertolini, J. Betzwieser, N. Beveridge

^*Corresponding author for this work

Physics and Astronomy

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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 1-99M_ȯ and total masses of 25-100M_ȯ. 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 19M_ȯ≤m₁, m ₂≤28M_ȯ binary black-hole systems with negligible spin to be no more than 2.0Mpc^-3Myr^-1 at 90% confidence.

Original language	English (US)
Article number	122005
Journal	Physical Review D - Particles, Fields, Gravitation and Cosmology
Volume	83
Issue number	12
DOIs	https://doi.org/10.1103/PhysRevD.83.122005
State	Published - Jun 6 2011

ASJC Scopus subject areas

Nuclear and High Energy Physics
Physics and Astronomy (miscellaneous)

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10.1103/PhysRevD.83.122005

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Abadie, J., Abbott, B. P., Abbott, R., Abernathy, M., Accadia, T., Acernese, F., Adams, C., Adhikari, R., Ajith, P., Allen, B., Allen, G. S., Amador Ceron, E., Amin, R. S., Anderson, S. B., Anderson, W. G., Antonucci, F., Arain, M. A., Araya, M. C., Aronsson, M., ... Beveridge, N. (2011). Search for gravitational waves from binary black hole inspiral, merger, and ringdown. Physical Review D - Particles, Fields, Gravitation and Cosmology, 83(12), [122005]. https://doi.org/10.1103/PhysRevD.83.122005

@article{55ad8ebcec2e4388a4cfbaa358f22376,

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.",

author = "J. Abadie and Abbott, {B. P.} and R. Abbott and M. Abernathy and T. Accadia and F. Acernese and C. Adams and R. Adhikari and P. Ajith and B. Allen and Allen, {G. S.} and {Amador Ceron}, E. and Amin, {R. S.} and Anderson, {S. B.} and Anderson, {W. G.} and F. Antonucci and Arain, {M. A.} and Araya, {M. C.} and M. Aronsson and Y. Aso and Aston, {S. M.} and P. Astone and D. Atkinson and P. Aufmuth and C. Aulbert and S. Babak and P. Baker and G. Ballardin and T. Ballinger and S. Ballmer and D. Barker and S. Barnum and F. Barone and B. Barr and P. Barriga and L. Barsotti and M. Barsuglia and Barton, {M. A.} and I. Bartos and R. Bassiri and M. Bastarrika and J. Bauchrowitz and Bauer, {Th S.} and B. Behnke and Beker, {M. G.} and A. Belletoile and M. Benacquista and A. Bertolini and J. Betzwieser and N. Beveridge",

year = "2011",

month = jun,

day = "6",

doi = "10.1103/PhysRevD.83.122005",

language = "English (US)",

volume = "83",

journal = "Physical Review D - Particles, Fields, Gravitation and Cosmology",

issn = "1550-7998",

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Abadie, J, Abbott, BP, Abbott, R, Abernathy, M, Accadia, T, Acernese, F, Adams, C, Adhikari, R, Ajith, P, Allen, B, Allen, GS, Amador Ceron, E, Amin, RS, Anderson, SB, Anderson, WG, Antonucci, F, Arain, MA, Araya, MC, Aronsson, M, Aso, Y, Aston, SM, Astone, P, Atkinson, D, Aufmuth, P, Aulbert, C, Babak, S, Baker, P, Ballardin, G, Ballinger, T, Ballmer, S, Barker, D, Barnum, S, Barone, F, Barr, B, Barriga, P, Barsotti, L, Barsuglia, M, Barton, MA, Bartos, I, Bassiri, R, Bastarrika, M, Bauchrowitz, J, Bauer, TS, Behnke, B, Beker, MG, Belletoile, A, Benacquista, M, Bertolini, A, Betzwieser, J & Beveridge, N 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

TY - JOUR

T1 - Search for gravitational waves from binary black hole inspiral, merger, and ringdown

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 - Bastarrika, M.

AU - Bauchrowitz, J.

AU - Bauer, Th S.

AU - Behnke, B.

AU - Beker, M. G.

AU - Belletoile, A.

AU - Benacquista, M.

AU - Bertolini, A.

AU - Betzwieser, J.

AU - Beveridge, N.

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.

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UR - http://www.scopus.com/inward/citedby.url?scp=79960823290&partnerID=8YFLogxK

U2 - 10.1103/PhysRevD.83.122005

DO - 10.1103/PhysRevD.83.122005

M3 - Article

AN - SCOPUS:79960823290

SN - 1550-7998

VL - 83

JO - Physical Review D - Particles, Fields, Gravitation and Cosmology

JF - Physical Review D - Particles, Fields, Gravitation and Cosmology

IS - 12

M1 - 122005

ER -

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

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