Skip to main content

Research Repository

Advanced Search

Confirming U(1)Lμ−Lτ as a solution for (g − 2)μ with neutrinos

Amaral, D.W.P.; Cerdeño, D.G.; Cheek, A.; Foldenauer, P.

Confirming U(1)Lμ−Lτ as a solution for (g − 2)μ with neutrinos Thumbnail


Authors

D.W.P. Amaral

D.G. Cerdeño

A. Cheek

P. Foldenauer



Abstract

The recent measurement of the muon anomalous magnetic moment by the Fermilab E989 experiment, when combined with the previous result at BNL, has confirmed the tension with the SM prediction at 4.2σ CL, strengthening the motivation for new physics in the leptonic sector. Among the different particle physics models that could account for such an excess, a gauged U(1)Lμ−Lτ stands out for its simplicity. In this article, we explore how the combination of data from different future probes can help identify the nature of the new physics behind the muon anomalous magnetic moment. In particular, we contrast U(1)Lμ−Lτ with an effective U(1)Lμ-type model. We first show that muon fixed target experiments (such as NA64μ) will be able to measure the coupling of the hidden photon to the muon sector in the region compatible with (g−2)μ, and will have some sensitivity to the hidden photon’s mass. We then study how experiments looking for coherent elastic neutrino-nucleus scattering (CEνNS) at spallation sources will provide crucial additional information on the kinetic mixing of the hidden photon. When combined with NA64μ results, the exclusion limits (or reconstructed regions) of future CEνNS detectors will also allow for a better measurement of the mediator mass. Finally, the observation of nuclear recoils from solar neutrinos in dark matter direct detection experiments will provide unique information about the coupling of the hidden photon to the tau sector. The signal expected for U(1)Lμ−Lτ is larger than for U(1)Lμ with the same kinetic mixing, and future multi-ton liquid xenon proposals (such as DARWIN) have the potential to confirm the former over the latter. We determine the necessary exposure and energy threshold for a potential 5σ discovery of a U(1)Lμ−Lτ boson, and we conclude that the future DARWIN observatory will be able to carry out this measurement if the experimental threshold is lowered to 1keVnr.

Citation

Amaral, D., Cerdeño, D., Cheek, A., & Foldenauer, P. (2021). Confirming U(1)Lμ−Lτ as a solution for (g − 2)μ with neutrinos. The European Physical Journal C, 81(10), Article 861. https://doi.org/10.1140/epjc/s10052-021-09670-z

Journal Article Type Article
Acceptance Date Sep 17, 2021
Online Publication Date Oct 1, 2021
Publication Date 2021-10
Deposit Date Jan 19, 2022
Publicly Available Date Jan 20, 2022
Journal The European Physical Journal C
Print ISSN 1434-6044
Electronic ISSN 1434-6052
Publisher SpringerOpen
Peer Reviewed Peer Reviewed
Volume 81
Issue 10
Article Number 861
DOI https://doi.org/10.1140/epjc/s10052-021-09670-z
Public URL https://durham-repository.worktribe.com/output/1216467

Files

Published Journal Article (2.5 Mb)
PDF

Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/

Copyright Statement
This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder.






You might also like



Downloadable Citations