New modular fixed point models and their phenomenological implications for JUNO, T2HK and DUNE
Er-Hao Shang, Jun-Nan Lu, Gui-Jun Ding, Stephen F. King
TL;DR
This work extends the modular Littlest Seesaw framework to two finite modular groups, $S'_4$ and $A_5$, by exploiting three fixed points in the modulus to constrain the Dirac neutrino structure via triplet modular forms. The authors perform an exhaustive scan of 4 viable $S'_4$ cases (A–D) and 14 $A_5$ cases (I–XIV), obtaining highly predictive neutrino mass matrices with a massless lightest neutrino ($m_1=0$) and a fixed first column of the PMNS matrix, yielding new sum rules that relate solar and reactor angles beyond TM1. Confronting these models with the latest global neutrino fits and JUNO results, several cases are already favored, while JUNO’s precision will decisively test many remaining scenarios; DUNE and T2HK will further discriminate among them via $\sin^2\theta_{23}$ and $\delta_{CP}$. The framework predicts a normal hierarchy with $m_{\beta\beta}$ in the few meV range, and a largely testable structure for future neutrinoless double-beta decay experiments. Overall, modular fixed-point models offer a highly predictive and testable path to leptonic flavor, with clear experimental benchmarks for upcoming neutrino facilities.
Abstract
We perform a general analysis of minimal modular fixed point models based on two right-handed neutrinos (2RHNs) and three modular fixed points, and find that the only viable possibilities are based on modular $S_4'$ and $A_5$ symmetry. Such models are highly predictive, with neutrino masses and the lepton mixing mixing matrix being fixed by three real parameters, as in the Littlest Seesaw Models. We perform an exhaustive scan over all possible models in this class and find many viable fixed points and modular form alignments, after confronting them with the latest neutrino oscillation global fits. The resulting models have the new feature that the two Dirac columns take more general forms than traditional Littlest Seesaw models, resulting in new sum rule relations between the solar and reactor angles, beyond those associated with TM1 (where the first column of the tri-bimaximal mixing matrix is preserved), which are compared to present and future projected JUNO results. We also compare the predictions of these models for the atmospheric angle and CP violating phase to current global fits and future T2HK and DUNE sensitivities.
