Published October 27, 2023
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Search for events in XENON1T associated with gravitational waves
Creators
- Aprile, E.1
- Abe, K.2
- Ahmed Maouloud, S.3
- Althueser, L.4
- Andrieu, B.3
- Angelino, E.5
- Angevaare, J. R.6
- Antochi, V. C.7
- Antón Martin, D.8
- Arneodo, F.9
- Baudis, L.10
- Baxter, A. L.11
- Bazyk, M.12
- Bellagamba, L.13
- Biondi, R.14
- Bismark, A.10
- Brookes, E. J.6
- Brown, A.15
- Bruenner, S.6
- Bruno, G.12
- Grandi, L.8
- Long, J.8
- Pienaar, J.8
- Yuan, L.8
- 1. Columbia University
- 2. University of Tokyo
- 3. Sorbonne Université
- 4. Westfälische Wilhelms-Universität Münster
- 5. University of Torino
- 6. University of Amsterdam
- 7. Stockholm University
- 8. University of Chicago
- 9. New York University
- 10. University of Zürich
- 11. Purdue University
- 12. Université de Nantes
- 13. University of Bologna
- 14. Max-Planck-Institut für Kernphysik
- 15. Universität Freiburg
Description
We perform a blind search for particle signals in the XENON1T dark matter detector that occur close in time to gravitational-wave signals in the LIGO and Virgo observatories. No particle signal is observed in the nuclear recoil and electronic recoil channels within $±500$ seconds of observations of the gravitational-wave signals GW170104, GW170729, GW170817, GW170818, and GW170823. We use this null result to constrain monoenergetic neutrinos and axion-like particles emitted in the closest coalescence GW170817, a binary neutron star merger. We set new upper limits on the fluence (time-integrated flux) of coincident neutrinos down to 17 keV at the 90% confidence level. Furthermore, we constrain the product of the coincident fluence and cross section of axion-like particles to be less than $10^{−29} cm^2/cm^2$ in the [5.5–210] keV energy range at the 90% confidence level.
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PhysRevD.108.072015.pdf
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Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.108.072015
- Other
- oai:uchicago.tind.io:13266
Funding
- National Science Foundation
- Swiss National Science Foundation
- German Ministry for Education and Research
- Max Planck Gesellschaft
- Deutsche Forschungsgemeinschaft
- Helmholtz Association
- Dutch Research Council
- Weizmann Institute of Science
- Israeli Science Foundation
- Binational Science Foundation
- Région des Pays de la Loire
- Knut and Alice Wallenberg Foundation
- Kavli Foundation
- JSPS Kakenhi
- JST FOREST Program
- Tsinghua University Initiative Scientific Research Program
- Istituto Nazionale di Fisica Nucleare
- European Union
- Horizon 2020 research and innovation programme
- Marie Skłodowska-Curie
- 860881-HIDDeN