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

The LIGO Scientific Collaboration; The Virgo Collaboration; the KAGRA Collaboration; M. Carlassara; P. Chakraborty; K. Danzmann; M. Heurs; N. Johny; N. Knust; H. Lück; M. Matiushechkina; H. Vahlbruch; D. Wilken; B. Willke; Tomislav Andric; Fabio Bergamin; Aparna Bisht; Nina Bode; Andreas Borchers; Marc Brinkmann; Eike Brockmueller; Jonathan Joseph Carter; Shrobana Ghosh; S. Hochheim; Wolfgang Kastaun; Fawad Khan; Philip Koch; G. Kuehn; Kristopher Kruska; Volker Kringel; J. Lehmann; James Lough; R. R. Maciy; M. Ma'arif; Fabian Meylahn; S. L. Nadji; M. Nery; F. Ohme; G. Pascale; B. F. Schutz; Bernd Wolfgang Schulte; M. Schneewind; J.  Venneberg; J. von Wrangel; Z. Wang; Michael Weinert; F. Wellmann; D. S. Wu

doi:10.3847/1538-4357/ad8de0

Details

Original language	English
Article number	255
Journal	Astrophysical Journal
Volume	977
Issue number	2
Publication status	Published - 18 Dec 2024

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’ 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.

ASJC Scopus subject areas

Physics and Astronomy(all)
Astronomy and Astrophysics
Earth and Planetary Sciences(all)
Space and Planetary Science

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A Search Using GEO600 for Gravitational Waves Coincident with Fast Radio Bursts from SGR 1935+2154. / The LIGO Scientific Collaboration; The Virgo Collaboration; the KAGRA Collaboration et al.
In: Astrophysical Journal, Vol. 977, No. 2, 255, 18.12.2024.

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

The LIGO Scientific Collaboration, The Virgo Collaboration, the KAGRA Collaboration, Carlassara, M, Chakraborty, P, Danzmann, K, Heurs, M, Johny, N, Knust, N, Lück, H, Matiushechkina, M, Vahlbruch, H, Wilken, D, Willke, B, Andric, T, Bergamin, F, Bisht, A, Bode, N, Borchers, A, Brinkmann, M, Brockmueller, E, Carter, JJ, Ghosh, S, Hochheim, S, Kastaun, W, Khan, F, Koch, P, Kuehn, G, Kruska, K, Kringel, V, Lehmann, J, Lough, J, Maciy, RR, Ma'arif, M, Meylahn, F, Nadji, SL, Nery, M, Ohme, F, Pascale, G, Schutz, BF, Schulte, BW, Schneewind, M, Venneberg, J, von Wrangel, J, Wang, Z, Weinert, M, Wellmann, F & Wu, DS 2024, 'A Search Using GEO600 for Gravitational Waves Coincident with Fast Radio Bursts from SGR 1935+2154', Astrophysical Journal, vol. 977, no. 2, 255. https://doi.org/10.3847/1538-4357/ad8de0

The LIGO Scientific Collaboration, The Virgo Collaboration, the KAGRA Collaboration, Carlassara, M., Chakraborty, P., Danzmann, K., Heurs, M., Johny, N., Knust, N., Lück, H., Matiushechkina, M., Vahlbruch, H., Wilken, D., Willke, B., Andric, T., Bergamin, F., Bisht, A., Bode, N., Borchers, A., ... Wu, D. S. (2024). A Search Using GEO600 for Gravitational Waves Coincident with Fast Radio Bursts from SGR 1935+2154. Astrophysical Journal, 977(2), Article 255. https://doi.org/10.3847/1538-4357/ad8de0

The LIGO Scientific Collaboration, The Virgo Collaboration, the KAGRA Collaboration, Carlassara M, Chakraborty P, Danzmann K et al. A Search Using GEO600 for Gravitational Waves Coincident with Fast Radio Bursts from SGR 1935+2154. Astrophysical Journal. 2024 Dec 18;977(2):255. doi: 10.3847/1538-4357/ad8de0

The LIGO Scientific Collaboration ; The Virgo Collaboration ; the KAGRA Collaboration et al. / A Search Using GEO600 for Gravitational Waves Coincident with Fast Radio Bursts from SGR 1935+2154. In: Astrophysical Journal. 2024 ; Vol. 977, No. 2.

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@article{e308ed6ecd5e475d808ba4726bc43223,

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} and {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 M. Carlassara and P. Chakraborty and S. Danilishin and K. Danzmann and A. Dasgupta and M. Heurs and N. Johny and J. Junker and N. Knust and H. L{\"u}ck and M. Matiushechkina and H. Vahlbruch and D. Wilken and B. Willke and Tomislav Andric and Fabio Bergamin and Aparna Bisht and Nina Bode and Andreas Borchers and Marc Brinkmann and Eike Brockmueller and Carter, {Jonathan Joseph} and Shrobana Ghosh and S. Hochheim and Wolfgang Kastaun and Fawad Khan and Philip Koch and G. Kuehn and Kristopher Kruska and Volker Kringel and J. Lehmann and James Lough and Maciy, {R. R.} and M. Ma'arif and Fabian Meylahn and Nadji, {S. L.} and M. Nery and F. Ohme and G. Pascale and Schutz, {B. F.} and Schulte, {Bernd Wolfgang} and M. Schneewind and J. Venneberg and {von Wrangel}, J. and Z. Wang and Michael Weinert and F. Wellmann and Wu, {D. S.}",

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

year = "2024",

month = dec,

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language = "English",

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

AU - The LIGO Scientific Collaboration

AU - The Virgo Collaboration

AU - 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.

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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 - Carlassara, M.

AU - Chakraborty, P.

AU - Danilishin, S.

AU - Danzmann, K.

AU - Dasgupta, A.

AU - Heurs, M.

AU - Johny, N.

AU - Junker, J.

AU - Knust, N.

AU - Lück, H.

AU - Matiushechkina, M.

AU - Vahlbruch, H.

AU - Wilken, D.

AU - Willke, B.

AU - Andric, Tomislav

AU - Bergamin, Fabio

AU - Bisht, Aparna

AU - Bode, Nina

AU - Borchers, Andreas

AU - Brinkmann, Marc

AU - Brockmueller, Eike

AU - Carter, Jonathan Joseph

AU - Ghosh, Shrobana

AU - Hochheim, S.

AU - Kastaun, Wolfgang

AU - Khan, Fawad

AU - Koch, Philip

AU - Kuehn, G.

AU - Kruska, Kristopher

AU - Kringel, Volker

AU - Lehmann, J.

AU - Lough, James

AU - Maciy, R. R.

AU - Ma'arif, M.

AU - Meylahn, Fabian

AU - Nadji, S. L.

AU - Nery, M.

AU - Ohme, F.

AU - Pascale, G.

AU - Schutz, B. F.

AU - Schulte, Bernd Wolfgang

AU - Schneewind, M.

AU - Venneberg, J.

AU - von Wrangel, J.

AU - Wang, Z.

AU - Weinert, Michael

AU - Wellmann, F.

AU - Wu, D. S.

PY - 2024/12/18

Y1 - 2024/12/18

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.

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JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

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Research@Leibniz University

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

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