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Theoretical and experimental constraints in the μ−τ four-lepton sector of the SMEFT: Implications to neutrino self-interactions

Aadarsh Singh1, Giancarlo D’Ambrosio2,1, and Sudhir K. Vempati1

Phys. Rev. D 114, 035038 – Published 27 August, 2026

DOI: https://doi.org/10.1103/8z45-8cw5

Abstract

We study the dimension-six SMEFT four-lepton operators in the μ–τ sector. These operators control both charged-lepton scattering and neutrino self-interactions, the latter being weakly constrained by direct laboratory probes despite their importance for cosmological tensions. We compare three classes of constraints on the Warsaw-basis coefficients [Cℓℓ]2222, [Cℓℓ]2233, and [Cℓℓ]2332. We use perturbative unitarity from 2→2 partial-wave analysis, spin-summing positivity sum rules, and the experimental bounds from NA64μ and the global fit [Adam Falkowski et al., Compilation of low-energy constraints on 4-fermion operators in the SMEFT, J. High Energy Phys. 08 (2017) 123.]. We find that the global fit dominates for [Cℓℓ]2222 and [Cℓℓ]2332, while NA64μ provides the leading bound on [Cℓℓ]2233, with the unitarity line for this direction entering the range of collider energies near 200 GeV. Renormalization-group running between 1 GeV and 30 TeV modifies these coefficients by up to 10%. Translating these bounds onto the effective four-neutrino coupling Geff, we find values many orders of magnitude smaller than the strongly interacting regime motivated by the Hubble tension; this excludes heavy-mediator UV completions of strong νμ–νμ and νμ–ντ self-interactions within the validity of the dimension-six SMEFT and in the absence of tuned cancellations between operators, while leaving the cosmologically motivated light-mediator scenarios unconstrained by this analysis. Finally, we comment on the bounds these coefficients place on a leptophilic Lμ−Lτ Z′ UV completion. Our SMEFT-based current and projected NA64μ bounds reproduce the dedicated Z′ analyses already available in the literature. We also present a complementary analysis for the e–μ sector using projected JUNO sensitivities.

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