All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run

The LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration

doi:10.1103/PhysRevD.104.122004

All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run

The LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration

California Institute of Technology
Louisiana State University
University of Salerno
National Institute for Nuclear Physics
Monash University
National Science Foundation
University of Wisconsin-Milwaukee
Australian National University
Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
Leibniz University Hannover
Inter-University Centre for Astronomy and Astrophysics India
University of Cambridge
Friedrich Schiller University Jena
University of Birmingham
Northwestern University
Instituto Nacional de Pesquisas Espaciais
Cardiff University
Tata Institute of Fundamental Research
National Institutes of Natural Sciences - National Astronomical Observatory of Japan
University of Naples Federico II
Universite Claude Bernard Lyon 1
The University of Tokyo
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Université Paris-Saclay
European Gravitational Observatory
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Columbia University
The Graduate University for Advanced Studies
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National Institute for Subatomic Physics
King's College London
Korea Institute of Science and Technology Information
National Institute for Mathematical Sciences
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The University of Osaka
University of Oregon
Syracuse University
University of Liege
University of Minnesota Twin Cities
University of Milan - Bicocca
Osservatorio Astronomico di Brera
University of Glasgow
Massachusetts Institute of Technology
Wigner Research Centre for Physics
University of Florida
Stanford University
University of Pisa
University of Perugia
University of Padua
Montana State University
Institute for Plasma Research
Polish Academy of Sciences
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Adelaide University
California State University Los Angeles
University of Western Australia
Raja Ramanna Centre for Advanced Technology
University of Amsterdam
Missouri University of Science and Technology
Lomonosov Moscow State University
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National Center for Nuclear Research
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Radboud University Nijmegen
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Andrews University
Tokyo City University
National Institute of Advanced Industrial Science and Technology
University of Groningen
Vrije Universiteit Brussel
National Defense Academy of Japan
Nagaoka University of Technology
Sejong University
National Yang Ming Chiao Tung University
Rikkyo University

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

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Abstract

This paper presents the results of a search for generic short-duration gravitational-wave transients in data from the third observing run of Advanced LIGO and Advanced Virgo. Transients with durations of milliseconds to a few seconds in the 24-4096 Hz frequency band are targeted by the search, with no assumptions made regarding the incoming signal direction, polarization, or morphology. Gravitational waves from compact binary coalescences that have been identified by other targeted analyses are detected, but no statistically significant evidence for other gravitational wave bursts is found. Sensitivities to a variety of signals are presented. These include updated upper limits on the source rate density as a function of the characteristic frequency of the signal, which are roughly an order of magnitude better than previous upper limits. This search is sensitive to sources radiating as little as ∼10-10 Mc2 in gravitational waves at ∼70 Hz from a distance of 10 kpc, with 50% detection efficiency at a false alarm rate of one per century. The sensitivity of this search to two plausible astrophysical sources is estimated: neutron star f modes, which may be excited by pulsar glitches, as well as selected core-collapse supernova models.

Original language	English
Article number	122004
Journal	Physical Review D
Volume	104
Issue number	12
DOIs	https://doi.org/10.1103/PhysRevD.104.122004
State	Published - 15 Dec 2021
Externally published	Yes

Funding

Funders	Funder number
Council of Scientific and Industrial Research, India
Ministry of Education, India
Australian Research Council
ICTP South American Institute for Fundamental Research
National Research Foundation of Korea
Narodowe Centrum Nauki
Scottish Universities Physics Alliance
National Science Foundation
Conselleria d’Innovació, Universitats, Ciència i Societat Digital de la Generalitat Valenciana
National Astronomical Observatory of Japan
Scottish Funding Council
Actions de Recherche Concertées
Ministry of Science and Technology, Taiwan
French Lyon Institute of Origins
Leverhulme Trust
Science and Engineering Research Board
Generalitat de Catalunya
Instituto Nazionale di Fisica Nucleare
Department of Science and Technology, Ministry of Science and Technology, India
Centre National de la Recherche Scientifique
Canada Foundation for Innovation
Kavli Foundation
Nemzeti Kutatási Fejlesztési és Innovációs Hivatal
KISTI-GSDC
European Commission
Russian Foundation for Basic Research
U.S. Department of Energy
Brazilian Ministry of Science, Technology, and Innovations
Agencia Estatal de Investigación
Natural Sciences and Engineering Research Council of Canada
Research Grants Council, University Grants Committee
Russian Science Foundation
Advanced Technology Center
Fundacja na rzecz Nauki Polskiej
Hungarian Scientific Research Fund
Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung
Fonds De La Recherche Scientifique - FNRS
Royal Society
Universitat de les Illes Balears
European Regional Development Fund
Fonds Wetenschappelijk Onderzoek—Vlaanderen
University of Tokyo
Istituto Nazionale di Fisica Nucleare
Ministry of Education, Culture, Sports, Science and Technology
National Natural Science Foundation of China
Japan Society for the Promotion of Science	JP20H05854, 17H06133, JP17H06361, 20A203, 26000005, JP17H06364, JP17H06358, 18H01224, 20H05639
Science and Technology Facilities Council	ST/S002464/1
Fundação para a Ciência e a Tecnologia	Incentivo/SAU/LA0001/2013
???publication-publication-funding-organisation-not-added???	14476
Academia Sinica	AS-CDA-105-M06

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10.1103/PhysRevD.104.122004

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@article{6c1495e8fece4eea8aea867a1729becd,

title = "All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run",

abstract = "This paper presents the results of a search for generic short-duration gravitational-wave transients in data from the third observing run of Advanced LIGO and Advanced Virgo. Transients with durations of milliseconds to a few seconds in the 24-4096 Hz frequency band are targeted by the search, with no assumptions made regarding the incoming signal direction, polarization, or morphology. Gravitational waves from compact binary coalescences that have been identified by other targeted analyses are detected, but no statistically significant evidence for other gravitational wave bursts is found. Sensitivities to a variety of signals are presented. These include updated upper limits on the source rate density as a function of the characteristic frequency of the signal, which are roughly an order of magnitude better than previous upper limits. This search is sensitive to sources radiating as little as ∼10-10 Mc2 in gravitational waves at ∼70 Hz from a distance of 10 kpc, with 50\% detection efficiency at a false alarm rate of one per century. The sensitivity of this search to two plausible astrophysical sources is estimated: neutron star f modes, which may be excited by pulsar glitches, as well as selected core-collapse supernova models.",

author = "\{The LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration\} and R. Abbott and Abbott, \{T. D.\} and F. Acernese and K. Ackley and C. Adams and N. Adhikari and Adhikari, \{R. X.\} and Adya, \{V. B.\} and C. Affeldt and D. Agarwal and M. Agathos and K. Agatsuma and N. Aggarwal and Aguiar, \{O. D.\} and L. Aiello and A. Ain and P. Ajith and T. Akutsu and S. Albanesi and A. Allocca and Altin, \{P. A.\} and A. Amato and C. Anand and S. Anand and A. Ananyeva and Anderson, \{S. B.\} and Anderson, \{W. G.\} and M. Ando and T. Andrade and N. Andres and T. Andri{\'c} and Angelova, \{S. V.\} and S. Ansoldi and Antelis, \{J. M.\} and S. Antier and S. Appert and Koji Arai and Koya Arai and Y. Arai and S. Araki and A. Araya and Araya, \{M. C.\} and Areeda, \{J. S.\} and M. Ar{\`e}ne and N. Aritomi and N. Arnaud and Aronson, \{S. M.\} and Arun, \{K. G.\} and H. Asada and J. Scheuer",

note = "Publisher Copyright: {\textcopyright} 2021 us.",

year = "2021",

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day = "15",

doi = "10.1103/PhysRevD.104.122004",

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T1 - All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run

AU - The LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration

AU - Abbott, R.

AU - Abbott, T. D.

AU - Acernese, F.

AU - Ackley, K.

AU - Adams, C.

AU - Adhikari, N.

AU - Adhikari, R. X.

AU - Adya, V. B.

AU - Affeldt, C.

AU - Agarwal, D.

AU - Agathos, M.

AU - Agatsuma, K.

AU - Aggarwal, N.

AU - Aguiar, O. D.

AU - Aiello, L.

AU - Ain, A.

AU - Ajith, P.

AU - Akutsu, T.

AU - Albanesi, S.

AU - Allocca, A.

AU - Altin, P. A.

AU - Amato, A.

AU - Anand, C.

AU - Anand, S.

AU - Ananyeva, A.

AU - Anderson, S. B.

AU - Anderson, W. G.

AU - Ando, M.

AU - Andrade, T.

AU - Andres, N.

AU - Andrić, T.

AU - Angelova, S. V.

AU - Ansoldi, S.

AU - Antelis, J. M.

AU - Antier, S.

AU - Appert, S.

AU - Arai, Koji

AU - Arai, Koya

AU - Arai, Y.

AU - Araki, S.

AU - Araya, A.

AU - Araya, M. C.

AU - Areeda, J. S.

AU - Arène, M.

AU - Aritomi, N.

AU - Arnaud, N.

AU - Aronson, S. M.

AU - Arun, K. G.

AU - Asada, H.

AU - Scheuer, J.

PY - 2021/12/15

Y1 - 2021/12/15

N2 - This paper presents the results of a search for generic short-duration gravitational-wave transients in data from the third observing run of Advanced LIGO and Advanced Virgo. Transients with durations of milliseconds to a few seconds in the 24-4096 Hz frequency band are targeted by the search, with no assumptions made regarding the incoming signal direction, polarization, or morphology. Gravitational waves from compact binary coalescences that have been identified by other targeted analyses are detected, but no statistically significant evidence for other gravitational wave bursts is found. Sensitivities to a variety of signals are presented. These include updated upper limits on the source rate density as a function of the characteristic frequency of the signal, which are roughly an order of magnitude better than previous upper limits. This search is sensitive to sources radiating as little as ∼10-10 Mc2 in gravitational waves at ∼70 Hz from a distance of 10 kpc, with 50% detection efficiency at a false alarm rate of one per century. The sensitivity of this search to two plausible astrophysical sources is estimated: neutron star f modes, which may be excited by pulsar glitches, as well as selected core-collapse supernova models.

AB - This paper presents the results of a search for generic short-duration gravitational-wave transients in data from the third observing run of Advanced LIGO and Advanced Virgo. Transients with durations of milliseconds to a few seconds in the 24-4096 Hz frequency band are targeted by the search, with no assumptions made regarding the incoming signal direction, polarization, or morphology. Gravitational waves from compact binary coalescences that have been identified by other targeted analyses are detected, but no statistically significant evidence for other gravitational wave bursts is found. Sensitivities to a variety of signals are presented. These include updated upper limits on the source rate density as a function of the characteristic frequency of the signal, which are roughly an order of magnitude better than previous upper limits. This search is sensitive to sources radiating as little as ∼10-10 Mc2 in gravitational waves at ∼70 Hz from a distance of 10 kpc, with 50% detection efficiency at a false alarm rate of one per century. The sensitivity of this search to two plausible astrophysical sources is estimated: neutron star f modes, which may be excited by pulsar glitches, as well as selected core-collapse supernova models.

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DO - 10.1103/PhysRevD.104.122004

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AN - SCOPUS:85122352068

SN - 2470-0010

VL - 104

JO - Physical Review D

JF - Physical Review D

IS - 12

M1 - 122004

ER -

All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run

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