Abelian symmetries as the source of the small neutrino-related flavor parameters
Shahar Amitai

TL;DR
The paper investigates whether Abelian symmetries can explain the small neutrino flavor parameters, concluding that it is unlikely due to the need for unnaturally small coefficients in the Froggatt-Nielsen mechanism.
Contribution
It demonstrates that Abelian symmetries are unlikely to be the source of small neutrino parameters within the Froggatt-Nielsen framework.
Findings
Abelian symmetries cannot naturally explain small neutrino parameters
Small coefficients are required for symmetry-breaking parameters
Froggatt-Nielsen mechanism is insufficient without fine-tuning
Abstract
There are four neutrino-related flavor parameters that have been measured: The three mixing angles s_{23}, s_{12}, s_{13}, and the ratio of mass-squared differences r_{23}. Of these, the first two are order one. On the other hand, s_{13} and r_{23} can be either order-one parameters that are accidentally somewhat small, or they are small for a reason, for example, they vanish in the limit of a symmetry that is broken by small parameters. We show that in the latter case, the Froggatt-Nielsen mechanism could explain the smallness of s_{13} and r_{23} only if some order-one coefficients are as small as the symmetry-breaking parameters. It is thus very unlikely that an Abelian symmetry is responsible for the smallness of s_{13} and r_{23}.
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Taxonomy
TopicsNeutrino Physics Research · Astrophysics and Cosmic Phenomena · Particle physics theoretical and experimental studies
