# Anomaly-Free Models for Flavour Anomalies

**Authors:** John Ellis, Malcolm Fairbairn, Patrick Tunney

arXiv: 1705.03447 · 2018-04-18

## TL;DR

This paper investigates anomaly-free U(1)' gauge models that could explain flavour anomalies, focusing on anomaly cancellation conditions, dark matter couplings, and implications for LHC Z' searches.

## Contribution

It identifies new anomaly-free models with specific charge assignments and dark matter couplings that can evade current experimental constraints.

## Key findings

- Anomaly cancellation constrains U(1)' charge assignments.
- Certain models suppress Z' couplings to first- and second-generation quarks.
- Models with axial dark matter couplings weaken direct detection constraints.

## Abstract

We explore the constraints imposed by the cancellation of triangle anomalies on models in which the flavour anomalies reported by LHCb and other experiments are due to an extra U(1)' gauge boson Z'. We assume universal and rational U(1)' charges for the first two generations of left-handed quarks and of right-handed up-type quarks but allow different charges for their third-generation counterparts. If the right-handed charges vanish, cancellation of the triangle anomalies requires all the quark U(1)' charges to vanish, if there are either no exotic fermions or there is only one Standard Model singlet dark matter (DM) fermion. There are non-trivial anomaly-free models with more than one such `dark' fermion, or with a single DM fermion if right-handed up-type quarks have non-zero U(1)' charges. In some of the latter models the U(1)' couplings of the first- and second-generation quarks all vanish, weakening the LHC Z' constraint, and in some other models the DM particle has purely axial couplings, weakening the direct DM scattering constraint. We also consider models in which anomalies are cancelled via extra vector-like leptons, showing how the prospective LHC Z' constraint may be weakened because the $Z^\prime \to \mu^+ \mu^-$ branching ratio is suppressed relative to other decay modes.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1705.03447/full.md

## Figures

1 figure with captions in the complete paper: https://tomesphere.com/paper/1705.03447/full.md

## References

38 references — full list in the complete paper: https://tomesphere.com/paper/1705.03447/full.md

---
Source: https://tomesphere.com/paper/1705.03447