Residual Symmetries and Scalar Multiplet Vacuum Alignment in Non-Abelian Flavour Models
Ivo de Medeiros Varzielas, Ming-Shau Liu, Amartya Sengupta, and Jim Talbert

TL;DR
This paper explores how residual flavor symmetries are preserved or broken in non-Abelian flavor models through scalar vacuum alignments, revealing a mechanism for understanding fine-tuning issues and phenomenological implications.
Contribution
It establishes a one-to-one correspondence between residual symmetry preservation and vacuum alignment corrections in non-Abelian flavor models, with applications to realistic models.
Findings
Residual symmetries correspond to special scalar vacuum alignments.
Additional operators can perturb these alignments, breaking residual symmetries.
The framework applies to models based on S4, A4, and Δ(27) symmetries.
Abstract
We demonstrate that, upon minimizing a renormalizable, single-scalar potential invariant under a non-Abelian symmetry, special orientations in the associated vacuum alignment of the scalar multiplet correspond to the preservation of a discrete residual flavour symmetry in the broken phase of the theory. Conversely, we show that these special scalar alignments are perturbed when additional Lagrangian operators (e.g. renormalizable, multi-flavon operators and/or effective, higher-dimensional operators) are present that break said residual symmetry, leading to a vacuum reorientation and phenomenological consequences. We therefore construct a one-to-one correspondence principle between broken residual symmetries and vacuum alignment corrections, providing a mechanism to identify (and correct) a subtle but persistent form of phenomenologically relevant fine-tuning embedded in -- but often…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsBlack Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories · Cosmology and Gravitation Theories
