https://doi.org/10.1140/epjc/s10052-025-15017-9
Regular Article - Theoretical Physics
Phenomenology of inverse seesaw using
modular symmetry
1
High Energy Physics Research Unit, Department of Physics, Chulalongkorn University, 10330, Bangkok, Thailand
2
Khon Kaen Particle Physics and Cosmology Theory Group (KKPaCT), Department of Physics, Khon Kaen University, 123 Mitraphap Rd, 40002, Khon Kaen, Thailand
3
Theoretical High-Energy Physics and Astrophysics Research Unit (ThEPA), Department of Physics, Srinakharinwirot University, 114 Sukhumvit 23 Rd., Wattana, 10110, Bangkok, Thailand
4
Department of Physics, School of Advanced Sciences, Vellore Institute of Technology, Tiruvalam Rd, Katpadi, 632014, Vellore, Tamil Nadu, India
a
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Received:
3
July
2025
Accepted:
1
November
2025
Published online:
17
November
2025
Abstract
Describing neutrino masses using the inverse seesaw mechanism with discrete flavor symmetry imposed through modular forms provides a testable framework at TeV scales with fewer parameters.
, the smallest finite modular group—naturally requiring only two new sets of heavy neutrinos—offers a unique yet largely unexplored setting for constructing minimal neutrino mass models. In this work, we construct the minimal supersymmetric inverse seesaw model based on the modular
flavor symmetry. In our model, the light neutrino mass matrix depends on 6 real parameters: the complex modulus, an overall scale for light neutrino mass, a real ratio and a complex ratio of Yukawa coupling. Thanks to its minimality, our model offers various definite predictions: the lightest neutrino is massless, the neutrino masses are inverted ordering, the sum of the three light neutrino masses (
) is 100 meV, the effective mass for the end point of the beta decay spectrum is 50 meV, the effective mass for neutrinoless double beta decay (
) is in the range
meV. In particular, the predicted values for
and
from our model are within reach of the next generation experiments. Our model also predicts radiative lepton flavor violating decays
which are compatible with experimental constraints.
Present address: Department of Physics, School of Advanced Sciences, Vellore Institute of Technology, Tiruvalam Rd, Katpadi, Vellore, Tamil Nadu, 632014, India
© The Author(s) 2025
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