# Sensitivity bounds on heavy neutrino mixing $|U_{\mu N}|^2$ and   $|U_{\tau N}|^2$ from LHCb upgrade

**Authors:** Gorazd Cvetic, C.S.Kim

arXiv: 1904.12858 · 2021-01-01

## TL;DR

This paper evaluates the potential of the LHCb upgrade to set upper bounds on heavy neutrino mixing parameters through meson decay searches involving muons and taus, focusing on decays mediated by on-shell neutrinos around 1 GeV.

## Contribution

It provides new sensitivity bounds on heavy-light neutrino mixing parameters from meson decays at LHCb upgrade, considering both muon and tau channels, and compares their effectiveness.

## Key findings

- Decays involving muons yield strong bounds on $|U_{\mu N}|^2$.
- Tau decay channels can set stringent bounds on $|U_{\tau N}|^2$.
- Sensitivity depends on meson production rates and decay kinematics.

## Abstract

Decays of heavy pseudoscalar mesons $B$, $B_c$, $B_s$ and $D_s$ at LHCb upgrade are considered, which produce either two equal sign muons or taus. In addition, we consider the analogous decays with opposite sign muons or taus. All these decays are considered to be mediated by a heavy on-shell neutrino $N$. Such decays of $B$ mesons, if not detected, will give in general stringent upper bounds on the heavy-light mixing parameter $|U_{\mu N}|^2$ as a function of the neutrino mass $M_N \sim 1$ GeV, principally due to the large expected number of produced mesons $B$. While some of the decays of the other mentioned mesons are attractive due to a weaker CKM-suppression, the expected produced number of such mesons is significantly smaller that that of $B$'s; therefore, the sensitivity bounds from such decays are in general comparable or less restrictive. When $\tau$ pairs are produced, only two types of such decays are significant: $B^{\pm}, B_{c}^{\pm} \to \tau^{\pm} \tau^{\pm} \pi^{\mp}$ (and $\tau^{\pm} \tau^{\mp} \pi^{\pm}$), giving us stringent upper bounds on $|U_{\tau N}|^2$; the other decays with a pair of $\tau$, such as $B^0 \to D^{(*)-} \tau^+ \tau^+ \pi^-$ (and $D^{(*)-} \tau^+ \tau^- \pi^+$), are prohibited or very suppressed by kinematics.

## Full text

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## Figures

10 figures with captions in the complete paper: https://tomesphere.com/paper/1904.12858/full.md

## References

58 references — full list in the complete paper: https://tomesphere.com/paper/1904.12858/full.md

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Source: https://tomesphere.com/paper/1904.12858