# Testing Leptoquark and $Z^{\prime}$ Models via $B\to   K_{1}(1270,1400)\mu^{+}\mu^{-}$ Decays

**Authors:** Zhuo-Ran Huang, Muhammad Ali Paracha, Ishtiaq Ahmed, Cai-Dian L\"u

arXiv: 1812.03491 · 2019-10-09

## TL;DR

This paper investigates how new physics models, specifically leptoquark and Z' models, could explain anomalies in B meson decays involving muons, and proposes specific ratios of decay rates as tools to distinguish these models from the Standard Model.

## Contribution

It introduces the use of LFU ratios in B to K1(1270,1400) decays to differentiate between NP models and the SM, highlighting their sensitivity and insensitivity to certain parameters.

## Key findings

- LFU ratios $R_{K_1^{(L,T)}(1270)}$ can distinguish NP models from SM.
- Ratios $R_{K_1^{(L,T)}(1400)}$ depend on NP effects and mixing angles.
- The ratio $R_	ext{mu}(K_1)$ can help determine the mixing angle $	heta_{K_1}$.

## Abstract

The measurements of $R_{K^{(*)}}=\mathcal B(B\to K^{(*)}\mu^{+}\mu^{-})/\mathcal B(B\to K^{(*)}e^{+}e^{-})$ in recent years have hinted lepton flavor non-universality and thus drawn widespread attentions. If these anomalies are induced by new physics (NP), deviations from the SM predictions may also be found in other channels via the same process at the quark level. In this work, we study in $B\to K_{1}(1270,1400)\mu^{+}\mu^{-}$ decays the effects of two popular classes of NP models which can address the $b\to s$ anomalies, i.e. the leptoquark models and the $Z^{\prime}$ models. By assuming that NP only affects the $b\to s\mu^+\mu^-$ transition, we find that the unpolarized and polarized lepton flavor universality (LFU) ratios $R_{K_1^{(L,T)}(1270)}$ are useful to distinguish among the NP models (scenarios) and the SM because they are sensitive to the NP effects and insensitive to the mixing angle $\theta_{K_1}$, while the $R_{K_1^{(L,T)}(1400)}$ are sensitive to both NP and $\theta_{K_1}$. Another ratio $R_\mu(K_1)=\mathcal B(B\to K_1(1400)\mu^+\mu^-)/\mathcal B(B\to K_1(1270)\mu^+\mu^-)$ is shown to depend weekly on the effects from the NP models (scenarios) under consideration, and thus can be used to determine the $\theta_{K_1}$ and complement the $R_{K_1^{(L,T)}}$ in the probe for NP.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1812.03491/full.md

## Figures

26 figures with captions in the complete paper: https://tomesphere.com/paper/1812.03491/full.md

## References

83 references — full list in the complete paper: https://tomesphere.com/paper/1812.03491/full.md

---
Source: https://tomesphere.com/paper/1812.03491