Partial Compositeness: from Anarchy to Symmetry

TL;DR

This paper explores how combining emergent IR flavor symmetries with UV-driven hierarchies in composite Higgs models can reconcile flavor constraints with collider accessibility, impacting neutrino physics and CP violation.

Contribution

It proposes a novel framework where IR emergent flavor symmetries and UV renormalization group flow generate realistic flavor hierarchies in composite Higgs theories.

Findings

IR flavor symmetries emerge near the compositeness scale

Flavor hierarchies are generated by UV RG flow

Implications for collider and neutrino phenomenology

Abstract

Within the Composite Higgs paradigm, Partial Compositeness has emerged as an elegant mechanism for generating large flavor hierarchies such as are observed in the quark and lepton masses and mixings. This mechanism exploits the strong renormalization group effects of the compositeness dynamics when these are {\it not} flavor-symmetric. Despite its remarkable properties, at this point it is stringently constrained by the body of flavor- and CP-violation tests, so that the compositeness scale must be at least $O(100)$ TeV, beyond the direct reach of proposed colliders. On the other hand, Composite Higgs theories with flavor-symmetric strong dynamics, but with realistic flavor-violating hierarchies introduced in an ad hoc manner, can extend the GIM mechanism of the standard model and thereby be far less constrained, at the edge of LHC reach and well within reach of future colliders. We show how the best features of both these types of dynamics can be combined if flavor-symmetries of the strong composite dynamics are emergent in the IR near the compositeness scale but absent in the far UV. In this case, flavor hierarchies can be generated by the renormalization group flow in the UV, followed by an IR stage in which the dynamics flows towards accidental flavor and CP symmetries. We point out how the collider and low-energy phenomenology is significantly impacted by the IR stage. Our analysis includes a discussion of the distinctive features of the small neutrino masses and their large mixings.