TL;DR
This paper introduces a novel scotogenic model utilizing non-invertible $Z_M$ symmetries to explain dark matter stability and neutrino mass structure, providing minimalistic content and numerical analysis of lepton mixing.
Contribution
It presents the first scotogenic model based on non-group symmetries, achieving neutrino mass matrix with a one-zero structure and analyzing its phenomenological implications.
Findings
Dark matter stability is explained by non-invertible $Z_M$ symmetries.
Neutrino mass matrix exhibits a one-zero structure.
Numerical analysis aligns with observed lepton mixing angles.
Abstract
In the present work, the scotogenic model is constructed applying non invertible symmetries. The stability of dark matter and the scotogenic structure of the neutrino mass matrix is achieved via the new non-group symmetry. The non-group Scotogenic model is given with minimalistic content giving a one-zero structure of the neutrino mass matrix, and numerical analysis of the lepton mixing angles and physics are presented. Other relevant constraints are also studied.
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