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Search for Gravitational Waves from Binary Black Hole Inspiral, Merger and Ringdown in LIGO-Virgo Data from 2009-2010

We report a search for gravitational waves from the inspiral, merger and ringdown of binary black holes (BBH) with total mass between 25 and 100 solar masses, in data taken at the LIGO and Virgo observatories between July 7, 2009 and October 20, 2010. The maximum sensitive distance of the detectors... Full description

Journal Title: arXiv.org Feb 25, 2013
Main Author: Aasi, J
Other Authors: Abadie, J , Abbott, B , Abbott, R , Abbott, T , Abernathy, M , Accadia, T , Acernese, F , Adams, C , Adams, T , Addesso, P , Adhikari, R , Affeldt, C , Agathos, M , Agatsuma, K , Ajith, P , Allen, B , Allocca, A , Amariutei, D , Anderson
Format: Electronic Article Electronic Article
Language: English
Subjects:
ID: DOI: 10.1103/PhysRevD.87.022002
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title: Search for Gravitational Waves from Binary Black Hole Inspiral, Merger and Ringdown in LIGO-Virgo Data from 2009-2010
format: Article
creator:
  • Aasi, J
  • Abadie, J
  • Abbott, B
  • Abbott, R
  • Abbott, T
  • Abernathy, M
  • Accadia, T
  • Acernese, F
  • Adams, C
  • Adams, T
  • Addesso, P
  • Adhikari, R
  • Affeldt, C
  • Agathos, M
  • Agatsuma, K
  • Ajith, P
  • Allen, B
  • Allocca, A
  • Amariutei, D
  • Anderson
subjects:
  • Acquisitions & Mergers
  • Gravitational Waves
  • Gravitational Waves
  • Binary Stars
  • Observatories
  • Angular Momentum
  • Sensitivity Analysis
  • Gravitation
  • Dependence
  • Searching
  • Coalescing
  • Black Holes
  • Cosmology and Nongalactic Astrophysics
  • High Energy Astrophysical Phenomena
ispartof: arXiv.org, Feb 25, 2013
description: We report a search for gravitational waves from the inspiral, merger and ringdown of binary black holes (BBH) with total mass between 25 and 100 solar masses, in data taken at the LIGO and Virgo observatories between July 7, 2009 and October 20, 2010. The maximum sensitive distance of the detectors over this period for a (20,20) Msun coalescence was 300 Mpc. No gravitational wave signals were found. We thus report upper limits on the astrophysical coalescence rates of BBH as a function of the component masses for non-spinning components, and also evaluate the dependence of the search sensitivity on component spins aligned with the orbital angular momentum. We find an upper limit at 90% confidence on the coalescence rate of BBH with non-spinning components of mass between 19 and 28 Msun of 3.3 \times 10^-7 mergers /Mpc^3 /yr.
language: eng
source:
identifier: DOI: 10.1103/PhysRevD.87.022002
fulltext: fulltext_linktorsrc
url: Link


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titleSearch for Gravitational Waves from Binary Black Hole Inspiral, Merger and Ringdown in LIGO-Virgo Data from 2009-2010
creatorAasi, J ; Abadie, J ; Abbott, B ; Abbott, R ; Abbott, T ; Abernathy, M ; Accadia, T ; Acernese, F ; Adams, C ; Adams, T ; Addesso, P ; Adhikari, R ; Affeldt, C ; Agathos, M ; Agatsuma, K ; Ajith, P ; Allen, B ; Allocca, A ; Amariutei, D ; Anderson
ispartofarXiv.org, Feb 25, 2013
identifierDOI: 10.1103/PhysRevD.87.022002
subjectAcquisitions & Mergers ; Gravitational Waves ; Gravitational Waves ; Binary Stars ; Observatories ; Angular Momentum ; Sensitivity Analysis ; Gravitation ; Dependence ; Searching ; Coalescing ; Black Holes ; Cosmology and Nongalactic Astrophysics ; High Energy Astrophysical Phenomena
descriptionWe report a search for gravitational waves from the inspiral, merger and ringdown of binary black holes (BBH) with total mass between 25 and 100 solar masses, in data taken at the LIGO and Virgo observatories between July 7, 2009 and October 20, 2010. The maximum sensitive distance of the detectors over this period for a (20,20) Msun coalescence was 300 Mpc. No gravitational wave signals were found. We thus report upper limits on the astrophysical coalescence rates of BBH as a function of the component masses for non-spinning components, and also evaluate the dependence of the search sensitivity on component spins aligned with the orbital angular momentum. We find an upper limit at 90% confidence on the coalescence rate of BBH with non-spinning components of mass between 19 and 28 Msun of 3.3 \times 10^-7 mergers /Mpc^3 /yr.
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titleSearch for Gravitational Waves from Binary Black Hole Inspiral, Merger and Ringdown in LIGO-Virgo Data from 2009-2010
descriptionWe report a search for gravitational waves from the inspiral, merger and ringdown of binary black holes (BBH) with total mass between 25 and 100 solar masses, in data taken at the LIGO and Virgo observatories between July 7, 2009 and October 20, 2010. The maximum sensitive distance of the detectors over this period for a (20,20) Msun coalescence was 300 Mpc. No gravitational wave signals were found. We thus report upper limits on the astrophysical coalescence rates of BBH as a function of the component masses for non-spinning components, and also evaluate the dependence of the search sensitivity on component spins aligned with the orbital angular momentum. We find an upper limit at 90% confidence on the coalescence rate of BBH with non-spinning components of mass between 19 and 28 Msun of 3.3 \times 10^-7 mergers /Mpc^3 /yr.
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titleSearch for Gravitational Waves from Binary Black Hole Inspiral, Merger and Ringdown in LIGO-Virgo Data from 2009-2010
authorAasi, J ; Abadie, J ; Abbott, B ; Abbott, R ; Abbott, T ; Abernathy, M ; Accadia, T ; Acernese, F ; Adams, C ; Adams, T ; Addesso, P ; Adhikari, R ; Affeldt, C ; Agathos, M ; Agatsuma, K ; Ajith, P ; Allen, B ; Allocca, A ; Amariutei, D ; Anderson
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atitleSearch for Gravitational Waves from Binary Black Hole Inspiral, Merger and Ringdown in LIGO-Virgo Data from 2009-2010
jtitlearXiv.org
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abstractWe report a search for gravitational waves from the inspiral, merger and ringdown of binary black holes (BBH) with total mass between 25 and 100 solar masses, in data taken at the LIGO and Virgo observatories between July 7, 2009 and October 20, 2010. The maximum sensitive distance of the detectors over this period for a (20,20) Msun coalescence was 300 Mpc. No gravitational wave signals were found. We thus report upper limits on the astrophysical coalescence rates of BBH as a function of the component masses for non-spinning components, and also evaluate the dependence of the search sensitivity on component spins aligned with the orbital angular momentum. We find an upper limit at 90% confidence on the coalescence rate of BBH with non-spinning components of mass between 19 and 28 Msun of 3.3 \times 10^-7 mergers /Mpc^3 /yr.
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pubCornell University Library, arXiv.org
doi10.1103/PhysRevD.87.022002
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date2013-02-25