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Muon-Decay Parameters from COHERENT
Phys. Rev. Lett. 135, 131802 – Published 22 September, 2025
DOI: https://doi.org/10.1103/mlhl-v822
Abstract
We demonstrate that measurements of coherent elastic neutrino-nucleus scattering at spallation sources are valuable probes of muon-decay physics. Using COHERENT data we derive the first direct constraint on the Michel parameters governing the energy distribution. We also discuss future sensitivities, the implications for the Lorentz structure of the interactions mediating muon decay, and the application to other neutrino-production mechanisms like pion decay.
Physics Subject Headings (PhySH)
Article Text
References (57)
- D. Z. Freedman, Phys. Rev. D 9, 1389 (1974).
- D. Akimov et al. (COHERENT Collaboration), Science 357, 1123 (2017).
- D. Akimov et al. (COHERENT Collaboration), Phys. Rev. Lett. 126, 012002 (2021).
- D. Akimov et al. (COHERENT Collaboration), Phys. Rev. Lett. 129, 081801 (2022).
- S. Adamski et al. (COHERENT Collaboration), Phys. Rev. Lett. 134, 231801 (2025).
- J. Colaresi, J. I. Collar, T. W. Hossbach, C. M. Lewis, and K. M. Yocum, Phys. Rev. Lett. 129, 211802 (2022).
- Z. Bo et al. (PandaX Collaboration), Phys. Rev. Lett. 133, 191001 (2024).
- E. Aprile et al. (XENON Collaboration), Phys. Rev. Lett. 133, 191002 (2024).
- N. Ackermann et al., Nature (London) 643, 1229 (2025).
- A. A. Aguilar-Arevalo et al. (CCM Collaboration), Phys. Rev. D 106, 012001 (2022).
- V. Zema (COSINUS Collaboration), Nuovo Cimento Soc. Ital. Fis. 42C, 228 (2020).
- J. Barranco, O. Miranda, and T. I. Rashba, J. High Energy Phys. 12 (2005) 021.
- K. Scholberg, Phys. Rev. D 73, 033005 (2006).
- M. Cadeddu, C. Giunti, Y. F. Li, and Y. Y. Zhang, Phys. Rev. Lett. 120, 072501 (2018).
- D. K. Papoulias and T. S. Kosmas, Phys. Rev. D 97, 033003 (2018).
- I. M. Shoemaker, Phys. Rev. D 95, 115028 (2017).
- J. Liao and D. Marfatia, Phys. Lett. B 775, 54 (2017).
- M. Cadeddu, C. Giunti, K. A. Kouzakov, Y.-F. Li, Y.-Y. Zhang, and A. I. Studenikin, Phys. Rev. D 98, 113010 (2018); 101, 059902(E) (2020).
- D. Aristizabal Sierra, V. De Romeri, and N. Rojas, Phys. Rev. D 98, 075018 (2018).
- P. B. Denton, Y. Farzan, and I. M. Shoemaker, J. High Energy Phys. 07 (2018) 037.
- W. Altmannshofer, M. Tammaro, and J. Zupan, J. High Energy Phys. 09 (2019) 083; 11 (2021) 113(E).
- C. Giunti, Phys. Rev. D 101, 035039 (2020).
- P. Coloma, I. Esteban, M. C. Gonzalez-Garcia, and M. Maltoni, J. High Energy Phys. 02 (2020) 023; 12 (2020) 071(E).
- W. Skiba and Q. Xia, J. High Energy Phys. 10 (2022) 102.
- M. Hoferichter, J. Menéndez, and A. Schwenk, Phys. Rev. D 102, 074018 (2020).
- O. G. Miranda, D. K. Papoulias, G. Sanchez Garcia, O. Sanders, M. Tórtola, and J. W. F. Valle, J. High Energy Phys. 05 (2020) 130; 01 (2021) 067(E).
- M. Atzori Corona, M. Cadeddu, N. Cargioli, F. Dordei, C. Giunti, Y. F. Li, C. A. Ternes, and Y. Y. Zhang, J. High Energy Phys. 09 (2022) 164.
- V. De Romeri, O. G. Miranda, D. K. Papoulias, G. Sanchez Garcia, M. Tórtola, and J. W. F. Valle, J. High Energy Phys. 04 (2023) 035.
- V. Bresó-Pla, A. Falkowski, M. González-Alonso, and K. Monsálvez-Pozo, J. High Energy Phys. 05 (2023) 074.
- S. Navas et al. (Particle Data Group), Phys. Rev. D 110, 030001 (2024).
- W. Fetscher, H. J. Gerber, and K. F. Johnson, Phys. Lett. B 173, 102 (1986).
- W. Fetscher, Phys. Rev. D 49, 5945 (1994).
- S. Navas et al. (Particle Data Group), Phys. Rev. D 110, 030001 (2024).
- B. Balke et al., Phys. Rev. D 37, 587 (1988).
- C. A. Gagliardi, R. E. Tribble, and N. J. Williams, Phys. Rev. D 72, 073002 (2005).
- R. P. MacDonald et al. (TWIST Collaboration), Phys. Rev. D 78, 032010 (2008).
- A. Hillairet et al. (TWIST Collaboration), Phys. Rev. D 85, 092013 (2012).
The probability is denoted by in the muon-decay literature. Here, we use because is used to denote the nuclear weak charge, which plays a central role in observables.
- L. Michel, Proc. Phys. Soc. London Sect. A 63, 514 (1950).
We note that a factor is missing in Eq. (57.8) of the PDG review on muon-decay parameters [33] (as well as in previous editions), i.e., in the neutrino energy distribution, cf. Eq. (3).
- B. Armbruster et al. (KARMEN Collaboration), Phys. Rev. Lett. 81, 520 (1998).
- D. Akimov et al. (COHERENT Collaboration), 10.5281/zenodo.3903810 (2020).
- D. Baxter et al., J. High Energy Phys. 02 (2020) 123.
- P. S. Barbeau, Y. Efremenko, and K. Scholberg, Annu. Rev. Nucl. Part. Sci. 73, 41 (2023).
- D. Akimov et al. (COHERENT Collaboration), arXiv:2204.04575.
- H. Abele et al., Phys. Rep. 1023, 1 (2023).
- P. S. Barbeau et al. (COHERENT Collaboration), Phys. Rev. D 109, 092005 (2024).
- H. Jeong, CENNS-750, A ton-scale single phase LAr CEvNS detector, in Talk presented at the 24th International Workshop on Neutrinos From Accelerators (NuFACT 2023) (Seoul, 2023), https://indico.cern.ch/event/1216905/contributions/5456610/attachments/2702673/4691226/20230825%20NuFACT2023%20Haemin.pdf.
- S. Mishra et al., Phys. Lett. B 252, 170 (1990).
- P. Vilain et al. (CHARM-II Collaboration), Phys. Lett. B 364, 121 (1995).
- V. Bresó-Pla, S. Cruz-Alzaga, M. González-Alonso, and S. Prakash, arXiv:2505.01275.
- J. D. Jackson, S. B. Treiman, and H. W. Wyld, Phys. Rev. 106, 517 (1957).
- Y. Aoki et al. (Flavour Lattice Averaging Group (FLAG), arXiv:2411.04268.
- A. Falkowski, M. González-Alonso, and K. Mimouni, J. High Energy Phys. 08 (2017) 123.
- W. Buchmuller and D. Wyler, Nucl. Phys. B268, 621 (1986).
- B. Grzadkowski, M. Iskrzynski, M. Misiak, and J. Rosiek, J. High Energy Phys. 10 (2010) 085.
- A. Falkowski, Eur. Phys. J. C 83, 656 (2023).