A Search Using GEO600 for Gravitational Waves Coincident with Fast Radio Bursts from SGR 1935+2154

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

doi:10.3847/1538-4357/ad8de0

A Search Using GEO600 for Gravitational Waves Coincident with Fast Radio Bursts from SGR 1935+2154

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

Max-Planck-Institut fuer Gravitationsphysik
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University of Washington
Astroparticule and Cosmol APC
California State University Fullerton
Villanova University
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University of Genoa
European Gravitational Observatory (EGO)
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4 Citations (Scopus)

Résumé

The magnetar SGR 1935+2154 is the only known Galactic source of fast radio bursts (FRBs). FRBs from SGR 1935 +2154 were first detected by the Canadian Hydrogen Intensity Mapping Experiment (CHIME)/FRB and the Survey for Transient Astronomical Radio Emission 2 in 2020 April, after the conclusion of the LIGO, Virgo, and KAGRA Collaborations’ O3 observing run. Here, we analyze four periods of gravitational wave (GW) data from the GEO600 detector coincident with four periods of FRB activity detected by CHIME/FRB, as well as X-ray glitches and X-ray bursts detected by NICER and NuSTAR close to the time of one of the FRBs. We do not detect any significant GW emission from any of the events. Instead, using a short-duration GW search (for bursts <1 s) we derive 50% (90%) upper limits of 10⁴⁸ (10⁴⁹) erg for GWs at 300 Hz and 10⁴⁹ (10⁵⁰) erg at 2 kHz, and constrain the GW-to-radio energy ratio to <10¹⁴−10¹⁶. We also derive upper limits from a long-duration search for bursts with durations between 1 and 10 s. These represent the strictest upper limits on concurrent GW emission from FRBs.

langue originale	Anglais
Numéro d'article	20
journal	Astrophysical Journal
Volume	977
Numéro de publication	2
Les DOIs	https://doi.org/10.3847/1538-4357/ad8de0
état	Publié - 1 déc. 2024
Modification externe	Oui

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10.3847/1538-4357/ad8de0

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@article{1dad515c4ce447749710ef50eda9a515,

title = "A Search Using GEO600 for Gravitational Waves Coincident with Fast Radio Bursts from SGR 1935+2154",

abstract = "The magnetar SGR 1935+2154 is the only known Galactic source of fast radio bursts (FRBs). FRBs from SGR 1935 +2154 were first detected by the Canadian Hydrogen Intensity Mapping Experiment (CHIME)/FRB and the Survey for Transient Astronomical Radio Emission 2 in 2020 April, after the conclusion of the LIGO, Virgo, and KAGRA Collaborations{\textquoteright} O3 observing run. Here, we analyze four periods of gravitational wave (GW) data from the GEO600 detector coincident with four periods of FRB activity detected by CHIME/FRB, as well as X-ray glitches and X-ray bursts detected by NICER and NuSTAR close to the time of one of the FRBs. We do not detect any significant GW emission from any of the events. Instead, using a short-duration GW search (for bursts <1 s) we derive 50\% (90\%) upper limits of 1048 (1049) erg for GWs at 300 Hz and 1049 (1050) erg at 2 kHz, and constrain the GW-to-radio energy ratio to <1014−1016. We also derive upper limits from a long-duration search for bursts with durations between 1 and 10 s. These represent the strictest upper limits on concurrent GW emission from FRBs.",

author = "\{The LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration\} and Abac, \{A. G.\} and R. Abbott and I. Abouelfettouh and F. Acernese and K. Ackley and S. Adhicary and N. Adhikari and Adhikari, \{R. X.\} and Adkins, \{V. K.\} and D. Agarwal and M. Agathos and \{Aghaei Abchouyeh\}, M. and Aguiar, \{O. D.\} and I. Aguilar and L. Aiello and A. Ain and P. Ajith and T. Akutsu and S. Albanesi and Alfaidi, \{R. A.\} and A. Al-Jodah and C. All{\'e}n{\'e} and A. Allocca and S. Al-Shammari and Altin, \{P. A.\} and S. Alvarez-Lopez and A. Amato and L. Amez-Droz and A. Amorosi and C. Amra and A. Ananyeva and Anderson, \{S. B.\} and Anderson, \{W. G.\} and M. Andia and M. Ando and T. Andrade and N. Andres and M. Andr{\'e}s-Carcasona and T. Andri{\'c} and J. Anglin and S. Ansoldi and Antelis, \{J. M.\} and S. Antier and M. Aoumi and Appavuravther, \{E. Z.\} and S. Appert and Apple, \{S. K.\} and K. Arai and A. Araya and S. Chaty",

note = "Publisher Copyright: {\textcopyright} 2024. The Author(s). Published by the American Astronomical Society.",

year = "2024",

month = dec,

day = "1",

doi = "10.3847/1538-4357/ad8de0",

language = "English",

volume = "977",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "2",

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TY - JOUR

T1 - A Search Using GEO600 for Gravitational Waves Coincident with Fast Radio Bursts from SGR 1935+2154

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

AU - Abac, A. G.

AU - Abbott, R.

AU - Abouelfettouh, I.

AU - Acernese, F.

AU - Ackley, K.

AU - Adhicary, S.

AU - Adhikari, N.

AU - Adhikari, R. X.

AU - Adkins, V. K.

AU - Agarwal, D.

AU - Agathos, M.

AU - Aghaei Abchouyeh, M.

AU - Aguiar, O. D.

AU - Aguilar, I.

AU - Aiello, L.

AU - Ain, A.

AU - Ajith, P.

AU - Akutsu, T.

AU - Albanesi, S.

AU - Alfaidi, R. A.

AU - Al-Jodah, A.

AU - Alléné, C.

AU - Allocca, A.

AU - Al-Shammari, S.

AU - Altin, P. A.

AU - Alvarez-Lopez, S.

AU - Amato, A.

AU - Amez-Droz, L.

AU - Amorosi, A.

AU - Amra, C.

AU - Ananyeva, A.

AU - Anderson, S. B.

AU - Anderson, W. G.

AU - Andia, M.

AU - Ando, M.

AU - Andrade, T.

AU - Andres, N.

AU - Andrés-Carcasona, M.

AU - Andrić, T.

AU - Anglin, J.

AU - Ansoldi, S.

AU - Antelis, J. M.

AU - Antier, S.

AU - Aoumi, M.

AU - Appavuravther, E. Z.

AU - Appert, S.

AU - Apple, S. K.

AU - Arai, K.

AU - Araya, A.

AU - Chaty, S.

PY - 2024/12/1

Y1 - 2024/12/1

N2 - The magnetar SGR 1935+2154 is the only known Galactic source of fast radio bursts (FRBs). FRBs from SGR 1935 +2154 were first detected by the Canadian Hydrogen Intensity Mapping Experiment (CHIME)/FRB and the Survey for Transient Astronomical Radio Emission 2 in 2020 April, after the conclusion of the LIGO, Virgo, and KAGRA Collaborations’ O3 observing run. Here, we analyze four periods of gravitational wave (GW) data from the GEO600 detector coincident with four periods of FRB activity detected by CHIME/FRB, as well as X-ray glitches and X-ray bursts detected by NICER and NuSTAR close to the time of one of the FRBs. We do not detect any significant GW emission from any of the events. Instead, using a short-duration GW search (for bursts <1 s) we derive 50% (90%) upper limits of 1048 (1049) erg for GWs at 300 Hz and 1049 (1050) erg at 2 kHz, and constrain the GW-to-radio energy ratio to <1014−1016. We also derive upper limits from a long-duration search for bursts with durations between 1 and 10 s. These represent the strictest upper limits on concurrent GW emission from FRBs.

AB - The magnetar SGR 1935+2154 is the only known Galactic source of fast radio bursts (FRBs). FRBs from SGR 1935 +2154 were first detected by the Canadian Hydrogen Intensity Mapping Experiment (CHIME)/FRB and the Survey for Transient Astronomical Radio Emission 2 in 2020 April, after the conclusion of the LIGO, Virgo, and KAGRA Collaborations’ O3 observing run. Here, we analyze four periods of gravitational wave (GW) data from the GEO600 detector coincident with four periods of FRB activity detected by CHIME/FRB, as well as X-ray glitches and X-ray bursts detected by NICER and NuSTAR close to the time of one of the FRBs. We do not detect any significant GW emission from any of the events. Instead, using a short-duration GW search (for bursts <1 s) we derive 50% (90%) upper limits of 1048 (1049) erg for GWs at 300 Hz and 1049 (1050) erg at 2 kHz, and constrain the GW-to-radio energy ratio to <1014−1016. We also derive upper limits from a long-duration search for bursts with durations between 1 and 10 s. These represent the strictest upper limits on concurrent GW emission from FRBs.

U2 - 10.3847/1538-4357/ad8de0

DO - 10.3847/1538-4357/ad8de0

M3 - Article

AN - SCOPUS:85213701609

SN - 0004-637X

VL - 977

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

M1 - 20

ER -

A Search Using GEO600 for Gravitational Waves Coincident with Fast Radio Bursts from SGR 1935+2154

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