Fermion masses and mixings in a U(1)X model based on the Σ(18) discrete symmetry

Author:

Vien V V12,Hernández A E Cárcamo3,Long H N4

Affiliation:

1. Theoretical Particle Physics and Cosmology Research Group, Advanced Institute of Materials Science, Ton Duc Thang University, Ho Chi Minh City, Vietnam

2. Faculty of Applied Sciences, Ton Duc Thang University, Ho Chi Minh City, Vietnam

3. Departamento de Física, Universidad Técnica Federico Santa María, Casilla 110-V, Valparaíso, Chile, and Millennium Institute for Subatomic Physics at the High-Energy Frontier, SAPHIR, Chile

4. Institute of Physics, Vietnam Academy of Science and Technology, 10 Dao Tan, Ba Dinh, Hanoi, Vietnam

Abstract

Abstract We have built a renormalizable $U(1)_X$ model with a $\Sigma (18)\times Z_4$ symmetry, whose spontaneous breaking yields the observed standard model (SM) fermion masses and fermionic mixing parameters. The tiny masses of the light active neutrinos are produced by the type I seesaw mechanism mediated by very heavy right-handed Majorana neutrinos. To the best of our knowledge, this model is the first implementation of the $\Sigma (18)$ flavor symmetry in a renormalizable $U(1)_X$ model. Our model allows a successful fit for the SM fermion masses, fermionic mixing angles, and CP phases for both quark and lepton sectors. The obtained values for the physical observables of both quark and lepton sectors are in accordance with the experimental data. We obtain an effective neutrino mass parameter of $\langle m_{ee}\rangle=1.51\times 10^{-3}\, \mathrm{eV}$ for normal ordering (NO) and $\langle m_{ee}\rangle =4.88\times 10^{-2} \, \mathrm{eV}$ for inverted ordering (IO), which are well consistent with the recent experimental limits on neutrinoless double beta decay.

Funder

SCOAP

Publisher

Oxford University Press (OUP)

Subject

General Physics and Astronomy

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