# Detecting the $L_{\mu}-L_{\tau}$ gauge boson at Belle II

**Authors:** Takeshi Araki, Shihori Hoshino, Toshihiko Ota, Joe Sato, and Takashi, Shimomura

arXiv: 1702.01497 · 2017-03-10

## TL;DR

This paper evaluates Belle II's potential to detect a light $L_{}-L_{}$ gauge boson, which could explain muon magnetic moment anomalies and cosmic neutrino gaps, through missing energy signals.

## Contribution

It provides the first detailed sensitivity analysis of Belle II for the $L_{}-L_{}$ gauge boson, highlighting its unique enhancement features over dark photon models.

## Key findings

- Belle II can probe $Z'$ with mass up to 1 GeV.
- Sensitivity extends to gauge coupling $g_{Z'} 	extgreater 8 	imes 10^{-4}$.
- Half of the parameter space explaining muon g-2 discrepancy is accessible.

## Abstract

We discuss the feasibility of detecting the gauge boson of the $U(1)_{L_{\mu}-L_{\tau}}$ symmetry, which possesses a mass in the range between MeV and GeV, at the Belle-II experiment. The kinetic mixing between the new gauge boson $Z'$ and photon is forbidden at the tree level and is radiatively induced. The leptonic force mediated by such a light boson is motivated by the discrepancy in muon anomalous magnetic moment and also the gap in the energy spectrum of cosmic neutrino. Defining the process $e^{+} e^{-} \rightarrow \gamma Z' \rightarrow \gamma \nu \bar{\nu}~(missing~energy)$ to be the signal, we estimate the numbers of the signal and the background events and show the parameter region to which the Belle-II experiment will be sensitive. The signal process in the $L_{\mu}-L_{\tau}$ model is enhanced with a light $Z'$, which is a characteristic feature differing from the dark photon models with a constant kinetic mixing. We find that the Belle-II experiment with the design luminosity will be sensitive to the $Z'$ with the mass $M_{Z'} \lesssim 1 $ GeV and the new gauge coupling $g_{Z'} \gtrsim 8\cdot 10^{-4}$, which covers a half of the unconstrained parameter region that explains the discrepancy in muon anomalous magnetic moment. The possibilities to improve the significance of the detection are also discussed.

## Full text

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## Figures

13 figures with captions in the complete paper: https://tomesphere.com/paper/1702.01497/full.md

## References

103 references — full list in the complete paper: https://tomesphere.com/paper/1702.01497/full.md

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Source: https://tomesphere.com/paper/1702.01497