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Constraining axial non-standard interactions of neutrinos with long baseline experiments

Yasaman Farzan, Saeed Abbaslu

TL;DR

This work addresses the possibility that axial non-standard neutrino interactions, encoded in $\epsilon^{Aq}_{\alpha\beta}$, may reveal new physics beyond the standard framework even when vector NSI are constrained. It introduces a UV model with a new $\mathrm{U}(1)$ gauge symmetry that yields $\epsilon^{Au}_{\tau\tau}=\epsilon^{Ad}_{\tau\tau}$ of order unity and analyzes how these axial NSI modify neutral-current neutrino-nucleus scattering across quasi-elastic, resonance, and deep-inelastic regimes, using NuWro cross sections and form-factor inputs. A Cobaya-based MCMC analysis of MINOS(+) NC data provides current bounds, while DUNE projections show potential improvements for $\epsilon^{Aq}_{e\tau}$ and $\epsilon^{Aq}_{\tau\tau}$, though $\epsilon^{Aq}_{ee}$ remains weakly constrained due to SM suppression of electron-flavor channels. The results demonstrate that axial NSI can be probed by long-baseline NC measurements, offering a complementary window to oscillation and CE$\nu$NS constraints and linking to collider and dark-matter phenomenology through the proposed $Z'$ model.

Abstract

Thanks to a number of neutrino oscillation and Coherent Elastic neutrino Nucleus Scattering (CE$ν$NS) experiments, the vector Non-Standard Interactions (NSI) of neutrinos have been well studied and constrained. We show that the long-sought-after new physics may hide in the ``axial" non-standard interactions rather than in the vector NSI. We then show how by studying neutral current scattering events in the detectors of long baseline experiments, MINOS, MINOS$+$ and DUNE, the impact of the axial NSI can be discovered.

Constraining axial non-standard interactions of neutrinos with long baseline experiments

TL;DR

This work addresses the possibility that axial non-standard neutrino interactions, encoded in , may reveal new physics beyond the standard framework even when vector NSI are constrained. It introduces a UV model with a new gauge symmetry that yields of order unity and analyzes how these axial NSI modify neutral-current neutrino-nucleus scattering across quasi-elastic, resonance, and deep-inelastic regimes, using NuWro cross sections and form-factor inputs. A Cobaya-based MCMC analysis of MINOS(+) NC data provides current bounds, while DUNE projections show potential improvements for and , though remains weakly constrained due to SM suppression of electron-flavor channels. The results demonstrate that axial NSI can be probed by long-baseline NC measurements, offering a complementary window to oscillation and CENS constraints and linking to collider and dark-matter phenomenology through the proposed model.

Abstract

Thanks to a number of neutrino oscillation and Coherent Elastic neutrino Nucleus Scattering (CENS) experiments, the vector Non-Standard Interactions (NSI) of neutrinos have been well studied and constrained. We show that the long-sought-after new physics may hide in the ``axial" non-standard interactions rather than in the vector NSI. We then show how by studying neutral current scattering events in the detectors of long baseline experiments, MINOS, MINOS and DUNE, the impact of the axial NSI can be discovered.
Paper Structure (6 sections, 19 equations, 1 figure, 1 table)

This paper contains 6 sections, 19 equations, 1 figure, 1 table.

Figures (1)

  • Figure 1: $\Delta\chi^2_{NC}$ versus the NSI couplings for the isospin singlet (left) and the isospin violating couplings (right) for the $ee$, $e\tau$, and $\tau\tau$ components. In each panel, only one NSI coupling is set nonzero. The horizontal red lines show $\Delta \chi^2_{NC}=2.7$, which corresponds to 90 % C.L. with one degree of freedom. The blue solid lines depict the bounds forecasted for the DUNE experiment assuming zero uncertainty Abbaslu:2023vqk. The dashed (dotted) blue curves show the forecasted bounds for the DUNE experiment with $\sigma_{\epsilon}=0.1$ and $\sigma_{\omega}=0$ (with $\sigma_{\epsilon}=0.1$ and $\sigma_{\omega}=0.02$) Abbaslu:2023vqk. The solid black lines show the bounds based on the MINOS and MINOS+ NC data Abbaslu:2025fwt. The green bands represent the 90 % C.L. bounds obtained by dominated the SNO neutral current data Coloma:2023ixt.