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  • Letter
  • Open Access

Uncertainties on the ν(−)e/ν(−)μ and νe/ν¯e cross-section ratio from the modeling of nuclear effects at 0.2 to 1.2 GeV neutrino energies and their impact on neutrino oscillation experiments

T. Dieminger1,*, S. Dolan2,†, D. Sgalaberna1,‡, A. Nikolakopoulos3, T. Dealtry4, S. Bolognesi5, L. Pickering6, and A. Rubbia1

  • 1ETH Zurich, Institute for Particle physics and Astrophysics, CH-8093 Zurich, Switzerland
  • 2European Organization for Nuclear Research (CERN), 1211 Geneva 23, Switzerland
  • 3Theoretical Physics Department, Fermilab, Batavia, Illinois 60510, USA
  • 4Lancaster University, Physics Department, Lancaster LA1 4YB, United Kingdom
  • 5IRFU, CEA, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France
  • 6Royal Holloway University of London, Department of Physics, Egham, Surrey TW20 0EX, United Kingdom

  • *tilld@ethz.ch
  • †Stephen.Joseph.Dolan@cern.ch
  • ‡davide.sgalaberna@cern.ch

Phys. Rev. D 108, L031301 – Published 14 August, 2023

DOI: https://doi.org/10.1103/PhysRevD.108.L031301

Abstract

The potential for mismodeling of νμ/νe, ν¯μ/ν¯e, and νe/ν¯e cross-section ratios due to nuclear effects is quantified by considering model spread within the full kinematic phase space for charged-current quasielastic interactions. Its impact is then propagated to simulated experimental configurations based on the Hyper-K and ESSνSB experiments. Although significant discrepancies between theoretical models is confirmed, it is found that these largely lie in regions of phase space that contribute only a very small portion of the flux-integrated cross sections. Overall, a systematic uncertainty on the oscillated flux-averaged νe/ν¯e cross-section ratio is found to be ∼2 and ∼4% for Hyper-K and ESSνSB, respectively.

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