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

LIGO Scientific Collaboration; Virgo Collaboration

doi:10.1103/PhysRevD.83.122005

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

LIGO Scientific Collaboration, Virgo Collaboration

Research output: Contribution to journal › Article › Academic › peer-review

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(circle dot) and total masses of 25-100M(circle dot). 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(circle dot) <= m(1), m(2) <= 28M(circle dot) binary black-hole systems with negligible spin to be no more than 2.0 Mpc(-3) Myr(-1) at 90% confidence.

Original language	English
Article number	122005
Number of pages	20
Journal	Physical Review D
Volume	83
Issue number	12
DOIs	https://doi.org/10.1103/PhysRevD.83.122005
Publication status	Published - 6 Jun 2011
Externally published	Yes

Keywords

MODELING KICKS
MASS
COALESCENCE
SPIN
FILTERS
CHOICE
RATES

Access to Document

10.1103/PhysRevD.83.122005Licence: Free access - publisher

2 Erratum / corrigendum / retractions

Érratum: Search for gravitational waves from binary black hole inspiral, merger, and ringdown (vol 83, 122005, 2011)
Abadie, J., Abbott, B. P., Abbott, R., Abernathy, M., Accadia, T., Acernese, F., Adams, C., Adhikari, R., Ajith, P., Allen, B., Allen, G. S., Ceron, E. A., Amin, R. S., Anderson, S. B., Anderson, W. G., Antonucci, F., Arain, M. A., Araya, M. C., Aronsson, M. & Aso, Y. & 34 others, Aston, S. M., 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, M. A., Bartos, I., Bassiri, R., Bastarrika, M., Bauchrowitz, J., Bauer, T. S., Behnke, B., Beker, M. G., Belletoile, A., Benacquista, M., Bertolini, A., Betzwieser, J., Beveridge, N., Danilishin, S. L., Hild, S., Steinlechner, S. & van den Brand, J. F. J., 20 Sept 2012, In: Physical Review D. 86, 6, 3 p., 069903.
Research output: Contribution to journal › Erratum / corrigendum / retractions › Academic
Publisher's Note: Search for gravitational waves from binary black hole inspiral, merger, and ringdown (vol 83, 122005, 2011)
Abadie, J., Abbott, B. P., Abbott, R., Abernathy, M., Accadia, T., Acernese, F., Adams, C., Adhikari, R., Ajith, P., Allen, B., Allen, G. S., Ceron, E. A., Amin, R. S., Anderson, S. B., Anderson, W. G., Antonucci, F., Arain, M. A., Araya, M. C., Aronsson, M. & Aso, Y. & 34 others, Aston, S. M., 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, M. A., Bartos, I., Bassiri, R., Bastarrika, M., Bauchrowitz, J., Bauer, T. S., Behnke, B., Beker, M. G., Belletoile, A., Benacquista, M., Bertolini, A., Betzwieser, J., Beveridge, N., Danilishin, S. L., Hild, S., Steinlechner, S. & van den Brand, J. F. J., 18 Apr 2012, In: Physical Review D. 85, 8, 2 p., 089904.
Research output: Contribution to journal › Erratum / corrigendum / retractions › Academic

Cite this

@article{b37c63219d9c4573b20905e64e30f44e,

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 1-99M(circle dot) and total masses of 25-100M(circle dot). 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(circle dot) <= m(1), m(2) <= 28M(circle dot) binary black-hole systems with negligible spin to be no more than 2.0 Mpc(-3) Myr(-1) at 90% confidence.",

keywords = "MODELING KICKS, MASS, COALESCENCE, SPIN, FILTERS, CHOICE, RATES",

author = "J. Abadie and B.P. Abbott 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 G.S. Allen and E.A. Ceron and R.S. Amin and S.B. Anderson and W.G. Anderson and F. Antonucci and M.A. Arain and M.C. Araya and M. Aronsson and Y. Aso and S.M. Aston 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 M.A. Barton and I. Bartos and R. Bassiri and M. Bastarrika and J. Bauchrowitz and T.S. Bauer and B. Behnke and M.G. Beker and A. Belletoile and S.L. Danilishin and S. Hild and S. Steinlechner and {van den Brand}, J.F.J. and {LIGO Scientific Collaboration} and {Virgo Collaboration}",

year = "2011",

month = jun,

day = "6",

doi = "10.1103/PhysRevD.83.122005",

language = "English",

volume = "83",

journal = "Physical Review D",

issn = "1550-7998",

publisher = "American Physical Society",

number = "12",

}

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 - Ceron, E.A.

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, T.S.

AU - Behnke, B.

AU - Beker, M.G.

AU - Belletoile, A.

AU - Danilishin, S.L.

AU - Hild, S.

AU - Steinlechner, S.

AU - van den Brand, J.F.J.

AU - LIGO Scientific Collaboration

AU - Virgo Collaboration

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 1-99M(circle dot) and total masses of 25-100M(circle dot). 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(circle dot) <= m(1), m(2) <= 28M(circle dot) binary black-hole systems with negligible spin to be no more than 2.0 Mpc(-3) Myr(-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 1-99M(circle dot) and total masses of 25-100M(circle dot). 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(circle dot) <= m(1), m(2) <= 28M(circle dot) binary black-hole systems with negligible spin to be no more than 2.0 Mpc(-3) Myr(-1) at 90% confidence.

KW - MODELING KICKS

KW - MASS

KW - COALESCENCE

KW - SPIN

KW - FILTERS

KW - CHOICE

KW - RATES

U2 - 10.1103/PhysRevD.83.122005

DO - 10.1103/PhysRevD.83.122005

M3 - Article

SN - 1550-7998

VL - 83

JO - Physical Review D

JF - Physical Review D

IS - 12

M1 - 122005

ER -

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

Abstract

Keywords

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Research output

Érratum: Search for gravitational waves from binary black hole inspiral, merger, and ringdown (vol 83, 122005, 2011)

Publisher's Note: Search for gravitational waves from binary black hole inspiral, merger, and ringdown (vol 83, 122005, 2011)

Cite this