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4 Pith papers cite this work. Polarity classification is still indexing.

4 Pith papers citing it

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hep-ph 4

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2026 3 2025 1

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UNVERDICTED 4

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representative citing papers

Dirac one-loop seesaw in a non-invertible fusion rule

hep-ph · 2026-04-13 · unverdicted · novelty 6.0

A one-loop Dirac neutrino mass model stabilized by a non-invertible fusion rule from Z3 x Z3' accommodates oscillation data and provides a viable bosonic dark matter candidate.

Zee models with a non-invertible $Z_M$ symmetry

hep-ph · 2026-05-22 · unverdicted · novelty 5.0

Zee models are classified under non-invertible Z_M symmetries; viable candidates are identified from data consistency, and a Z_7 benchmark yields numerical predictions for neutrino parameters and CLFV rates.

LFV decays in a 3-4-1 model with minimal inverse seesaw neutrinos

hep-ph · 2026-04-09 · unverdicted · novelty 5.0

In a 3-4-1 model with minimal inverse seesaw, strong correlations are predicted between (g-2) anomalies and LFV decay rates, with the tau to muon gamma decay bound limiting the muon anomaly deviation to 10^{-9}.

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Showing 3 of 3 citing papers after filters.

  • Dirac one-loop seesaw in a non-invertible fusion rule hep-ph · 2026-04-13 · unverdicted · none · ref 94

    A one-loop Dirac neutrino mass model stabilized by a non-invertible fusion rule from Z3 x Z3' accommodates oscillation data and provides a viable bosonic dark matter candidate.

  • Zee models with a non-invertible $Z_M$ symmetry hep-ph · 2026-05-22 · unverdicted · none · ref 65

    Zee models are classified under non-invertible Z_M symmetries; viable candidates are identified from data consistency, and a Z_7 benchmark yields numerical predictions for neutrino parameters and CLFV rates.

  • LFV decays in a 3-4-1 model with minimal inverse seesaw neutrinos hep-ph · 2026-04-09 · unverdicted · none · ref 59

    In a 3-4-1 model with minimal inverse seesaw, strong correlations are predicted between (g-2) anomalies and LFV decay rates, with the tau to muon gamma decay bound limiting the muon anomaly deviation to 10^{-9}.