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Data-based two-body current contribution to the neutrino-nucleus cross section

Tomasz Bonus, Jan T. Sobczyk, Michał Siemaszko, and Cezary Juszczak
Phys. Rev. C 102, 015502 – Published 13 July 2020

Abstract

A phenomenological model of two-body current (2p2h) contribution to neutrino cross section is introduced. Predictions of the Valencia model for 2p2h [J. Nieves et al., Phys. Rev. C 83, 045501 (2011)] are modified using recent CC0π measurements from T2K and MINERvA experiments. Our results suggest a significant increase of the 2p2h cross section at neutrino energies bigger than 1 GeV and also a redistribution of 2p2h events as function of energy and momentum transfer. This may have a big impact on neutrino energy reconstruction in neutrino oscillation parameters.

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  • Received 3 March 2020
  • Accepted 2 June 2020

DOI:https://doi.org/10.1103/PhysRevC.102.015502

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Particles & FieldsNuclear Physics

Authors & Affiliations

Tomasz Bonus*, Jan T. Sobczyk, Michał Siemaszko, and Cezary Juszczak

  • Institute of Theoretical Physics, University of Wrocław, Plac Maxa Borna 9, 50-204 Wrocław, Poland

  • *tomasz.bonus@ift.uni.wroc.pl
  • jan.sobczyk@uwr.edu.pl

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Vol. 102, Iss. 1 — July 2020

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  • Figure 1
    Figure 1

    Value of χ2 as function of α parameter.

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  • Figure 2
    Figure 2

    The obtained scaling function for α=0.2.

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  • Figure 3
    Figure 3

    Cross section dependence on energy for (a) neutrino and (b) antineutrino.

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  • Figure 4
    Figure 4

    Distribution of 2p2h cross section in the ω/q plane before (left) and after (right) rescaling. From top to bottom: MINERνA neutrino: (a) before and (b) after, MINERνA antineutrino: (c) before and (d) after, T2K neutrino: (e) before and (f) after and T2K antyneutrino: (g) before and (h) after. On all the figures we show d2σdωdq in the units cm2/GeV2.

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  • Figure 5
    Figure 5

    A sample of detail comparison of nuwro predictions before and after rescaling confronted with the experimental data for (a) MINERvA neutrino, (b) MINERvA antineutrino, (c) T2K neutrino, and (d) T2K antineutrino. In all the figures the shaded area shows a sum of contributions from CCQE, RES, and DIS mechanisms.

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