An $A_4$-Symmetric Double Seesaw for Neutrino Masses and Mixing in Light of JUNO results

TL;DR

This paper proposes an $A_4$-symmetric double seesaw model for neutrino masses that aligns with recent JUNO measurements, providing a predictive framework that connects flavor symmetry, neutrino mixing, and experimental constraints.

Contribution

It introduces a novel $A_4$-based double seesaw mechanism that predicts neutrino mixing patterns and incorporates recent JUNO data to constrain the model parameters.

Findings

The model reproduces the TBM mixing pattern corrected by a (1-3) rotation.

JUNO results significantly restrict the model's parameter space.

The framework offers testable predictions for future neutrino experiments.

Abstract

We discuss a double seesaw mechanism for generating light neutrino masses within the Standard Model extensions that include both right-handed neutrinos and extra gauge-singlet sterile fermions. The flavour structure of the double seesaw framework is invoked by an $A_4$ discrete symmetry which yields predictive textures for the Dirac neutrino mass matrix $M_D$, the mixing matrix $M_{RS}$ connecting right-handed and sterile neutrinos, and the bare Majorana mass matrix $M_S$ for the sterile neutrinos. The interesting feature of the present framework is that the combination of the double seesaw mechanism and $A_4$ flavour alignments yields a leading-order TBM structure, corrected by a single rotation in the (1-3) sector. We also derive analytic expressions for the heavy sterile eigenvalues and for the resulting light neutrino masses, thereby clarifying the role of the symmetry in shaping the neutrino mass hierarchy. We further incorporate the most recent JUNO measurements, which improve the precision of the solar mixing angle $\sin^2\theta_{12} \simeq 0.31$, along with updated constraints on $\sin^2\theta_{13}$. We show that these results significantly restrict the allowed parameter space of the model. In particular, the observed value of $\sin^2\theta_{12}$ constrains the magnitude of the (1--3) rotation and the phases associated with the $A_4$ flavon couplings, while the value of $\sin^2\theta_{13}$ sharpens these restrictions further. Overall, the interplay between double seesaw dynamics, $A_4$ flavour symmetry, and the recent JUNO constraints yields a highly predictive framework for neutrino masses and mixings, offering a coherent explanation for the generation of light neutrino masses and testable predictions for future experiments.