# Effective Theory of Flavor for Minimal Mirror Twin Higgs

**Authors:** Riccardo Barbieri, Lawrence J. Hall, Keisuke Harigaya

arXiv: 1706.05548 · 2017-10-25

## TL;DR

This paper develops a constrained minimal mirror twin Higgs model incorporating flavor hierarchies via suppression factors, predicting mirror sector spectra and dark matter properties, with testable experimental implications.

## Contribution

It introduces a new minimal mirror twin Higgs framework with flavor hierarchies tied to a single parameter, linking fermion masses, dark matter, and Higgs phenomenology.

## Key findings

- Mirror quark and lepton spectra are predicted in terms of the flavor suppression ratio.
- Mirror QCD scale and decoupling temperature are constrained by flavor structure.
- Dark matter candidates are constrained and testable by upcoming experiments.

## Abstract

We consider two copies of the Standard Model, interchanged by an exact parity symmetry, P. The observed fermion mass hierarchy is described by suppression factors $\epsilon^{n_i}$ for charged fermion $i$, as can arise in Froggatt-Nielsen and extra-dimensional theories of flavor. The corresponding flavor factors in the mirror sector are $\epsilon'^{n_i}$, so that spontaneous breaking of the parity P arises from a single parameter $\epsilon'/\epsilon$, yielding a tightly constrained version of Minimal Mirror Twin Higgs, introduced in our previous paper. Models are studied for simple values of $n_i$, including in particular one with SU(5)-compatibility, that describe the observed fermion mass hierarchy. The entire mirror quark and charged lepton spectrum is broadly predicted in terms of $\epsilon'/\epsilon$, as are the mirror QCD scale and the decoupling temperature between the two sectors. Helium-, hydrogen- and neutron-like mirror dark matter candidates are constrained by self-scattering and relic ionization. In each case, the allowed parameter space can be fully probed by proposed direct detection experiments. Correlated predictions are made as well for the Higgs signal strength and the amount of dark radiation.

## Full text

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## Figures

41 figures with captions in the complete paper: https://tomesphere.com/paper/1706.05548/full.md

## References

64 references — full list in the complete paper: https://tomesphere.com/paper/1706.05548/full.md

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Source: https://tomesphere.com/paper/1706.05548