A radiative seesaw model in a non-invertible selection rule with the assistance of a non-holomorphic modular $A_4$ symmetry
Shilpa Jangid, Hiroshi Okada

TL;DR
This paper introduces a two-loop neutrino mass model with fermionic and bosonic dark matter candidates, utilizing a non-invertible fusion rule and non-holomorphic modular $A_4$ symmetry to explain neutrino masses, dark matter stability, and lepton flavor phenomena.
Contribution
It presents a novel two-loop neutrino mass model incorporating non-invertible fusion rules and non-holomorphic modular $A_4$ symmetry, linking dark matter stability with lepton sector predictions.
Findings
Fermionic dark matter favored over bosonic due to one-loop mass generation.
Model successfully fits lepton masses, mixing angles, and phases.
Predictions for lepton flavor violation and muon g-2 are consistent with experimental data.
Abstract
We propose a two-loop neutrino mass model where fermionic and bosonic dark matter (DM) candidates are simultaneously connected to the neutrinos. But the fermionic DM candidate is favored compared to the bosonic one due to generating the fermionic DM mass at one-loop level. In order to obtain our desired Lagrangian and Higgs potential, we introduce a gauging TY non-invertible fusion rule with the assistance of a non-holomorphic modular symmetry. The fusion rule forbids the mass of DM candidate at tree level but its mass is generated at one-loop level where the DM mass term dynamically violates the fusion rule. After that, the neutrino mass matrix is induced at one-loop level where a remnant symmetry is still remained. The symmetry assures the stability of our DM candidate. The non-holomorphic modular symmetry plays a role in forbidding the interactions between the…
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Taxonomy
TopicsParticle physics theoretical and experimental studies · Computational Physics and Python Applications · Dark Matter and Cosmic Phenomena
