All-sky search for gravitational wave emission from scalar boson clouds around spinning black holes in LIGO O3 data

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

doi:10.1103/PhysRevD.105.102001

All-sky search for gravitational wave emission from scalar boson clouds around spinning black holes in LIGO O3 data

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

California Institute of Technology
Tokyo Institute of Technology
University of Salerno
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Monash University
University of Wisconsin-Milwaukee
Louisiana State University
Australian National University
Max-Planck-Institut fuer Gravitationsphysik
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Inter-University Centre for Astronomy and Astrophysics India
University of Cambridge
Friedrich-Schiller University
University of Birmingham
Northwestern University
Instituto Nacional de Pesquisas Espaciais
Cardiff University
Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
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National Astronomical Observatory
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IGFL, Université de Lyon, Université Lyon 1
University of Tokyo
Research Center for the Early Universe
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American University
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European Gravitational Observatory (EGO)
College of Computing
Chennai Mathematical Institute
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Columbia University
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King's College London
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National Institute for Mathematical Sciences
Christopher Newport University
Universiteit Utrecht
University of Oregon
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University of Liège
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University of Salerno
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University of Florida
Stanford University
University of Pisa
University of Perugia
University of Padova
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Bard College
Montana State University
Institute for Plasma Research
Ghent University
Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences
University of Sannio at Benevento
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Stony Brook University
Flatiron Institute
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Indian Institute of Science Education and Research (IISER)
Istituto di Astrofisica e Planetologia Spaziali
Andrews University
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Kyoto University
Yukawa Institute for Theoretical Physics
Van Swinderen Institute for Particle Physics and Gravity
Vrjie Universiteit Brussel
High Energy Accelerator Research Organization (KEK)
National Defense Academy of Japan
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Nagaoka University of Technology
Tata Institute of Fundamental Research, Mumbai
Technical University of Eindhoven
Sejong University
Concordia University Wisconsin
National Yang Ming Chiao Tung University
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Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

75 Citations (Scopus)

Résumé

This paper describes the first all-sky search for long-duration, quasimonochromatic gravitational-wave signals emitted by ultralight scalar boson clouds around spinning black holes using data from the third observing run of Advanced LIGO. We analyze the frequency range from 20 to 610 Hz, over a small frequency derivative range around zero, and use multiple frequency resolutions to be robust towards possible signal frequency wanderings. Outliers from this search are followed up using two different methods, one more suitable for nearly monochromatic signals, and the other more robust towards frequency fluctuations. We do not find any evidence for such signals and set upper limits on the signal strain amplitude, the most stringent being ≈10-25 at around 130 Hz. We interpret these upper limits as both an "exclusion region"in the boson mass/black hole mass plane and the maximum detectable distance for a given boson mass, based on an assumption of the age of the black hole/boson cloud system.

langue originale	Anglais
Numéro d'article	102001
journal	Physical Review D
Volume	105
Numéro de publication	10
Les DOIs	https://doi.org/10.1103/PhysRevD.105.102001
état	Publié - 15 mai 2022
Modification externe	Oui

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10.1103/PhysRevD.105.102001

Contient cette citation

@article{953b23bc14dc4c6f9e91030552607b5c,

title = "All-sky search for gravitational wave emission from scalar boson clouds around spinning black holes in LIGO O3 data",

abstract = "This paper describes the first all-sky search for long-duration, quasimonochromatic gravitational-wave signals emitted by ultralight scalar boson clouds around spinning black holes using data from the third observing run of Advanced LIGO. We analyze the frequency range from 20 to 610 Hz, over a small frequency derivative range around zero, and use multiple frequency resolutions to be robust towards possible signal frequency wanderings. Outliers from this search are followed up using two different methods, one more suitable for nearly monochromatic signals, and the other more robust towards frequency fluctuations. We do not find any evidence for such signals and set upper limits on the signal strain amplitude, the most stringent being ≈10-25 at around 130 Hz. We interpret these upper limits as both an {"}exclusion region{"}in the boson mass/black hole mass plane and the maximum detectable distance for a given boson mass, based on an assumption of the age of the black hole/boson cloud system.",

author = "\{(The LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration)\} and R. Abbott and H. Abe and F. Acernese and K. Ackley and N. Adhikari and Adhikari, \{R. X.\} and Adkins, \{V. K.\} 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 Alfaidi, \{R. A.\} 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 M. Andr{\'e}s-Carcasona and T. Andri{\'c} and Angelova, \{S. V.\} and S. Ansoldi and Antelis, \{J. M.\} and S. Antier and T. Apostolatos and Appavuravther, \{E. Z.\} and S. Appert and Apple, \{S. K.\} and K. Arai and A. Araya and Araya, \{M. C.\} and Areeda, \{J. S.\} and M. Ar{\`e}ne and N. Aritomi and N. Arnaud and M. Arogeti and S. Chaty",

year = "2022",

month = may,

day = "15",

doi = "10.1103/PhysRevD.105.102001",

language = "English",

volume = "105",

journal = "Physical Review D",

issn = "2470-0010",

publisher = "American Physical Society",

number = "10",

}

TY - JOUR

T1 - All-sky search for gravitational wave emission from scalar boson clouds around spinning black holes in LIGO O3 data

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

AU - Abbott, R.

AU - Abe, H.

AU - Acernese, F.

AU - Ackley, K.

AU - Adhikari, N.

AU - Adhikari, R. X.

AU - Adkins, V. K.

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 - Alfaidi, R. A.

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 - Andrés-Carcasona, M.

AU - Andrić, T.

AU - Angelova, S. V.

AU - Ansoldi, S.

AU - Antelis, J. M.

AU - Antier, S.

AU - Apostolatos, T.

AU - Appavuravther, E. Z.

AU - Appert, S.

AU - Apple, S. K.

AU - Arai, K.

AU - Araya, A.

AU - Araya, M. C.

AU - Areeda, J. S.

AU - Arène, M.

AU - Aritomi, N.

AU - Arnaud, N.

AU - Arogeti, M.

AU - Chaty, S.

PY - 2022/5/15

Y1 - 2022/5/15

N2 - This paper describes the first all-sky search for long-duration, quasimonochromatic gravitational-wave signals emitted by ultralight scalar boson clouds around spinning black holes using data from the third observing run of Advanced LIGO. We analyze the frequency range from 20 to 610 Hz, over a small frequency derivative range around zero, and use multiple frequency resolutions to be robust towards possible signal frequency wanderings. Outliers from this search are followed up using two different methods, one more suitable for nearly monochromatic signals, and the other more robust towards frequency fluctuations. We do not find any evidence for such signals and set upper limits on the signal strain amplitude, the most stringent being ≈10-25 at around 130 Hz. We interpret these upper limits as both an "exclusion region"in the boson mass/black hole mass plane and the maximum detectable distance for a given boson mass, based on an assumption of the age of the black hole/boson cloud system.

AB - This paper describes the first all-sky search for long-duration, quasimonochromatic gravitational-wave signals emitted by ultralight scalar boson clouds around spinning black holes using data from the third observing run of Advanced LIGO. We analyze the frequency range from 20 to 610 Hz, over a small frequency derivative range around zero, and use multiple frequency resolutions to be robust towards possible signal frequency wanderings. Outliers from this search are followed up using two different methods, one more suitable for nearly monochromatic signals, and the other more robust towards frequency fluctuations. We do not find any evidence for such signals and set upper limits on the signal strain amplitude, the most stringent being ≈10-25 at around 130 Hz. We interpret these upper limits as both an "exclusion region"in the boson mass/black hole mass plane and the maximum detectable distance for a given boson mass, based on an assumption of the age of the black hole/boson cloud system.

U2 - 10.1103/PhysRevD.105.102001

DO - 10.1103/PhysRevD.105.102001

M3 - Article

AN - SCOPUS:85132162142

SN - 2470-0010

VL - 105

JO - Physical Review D

JF - Physical Review D

IS - 10

M1 - 102001

ER -

All-sky search for gravitational wave emission from scalar boson clouds around spinning black holes in LIGO O3 data

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