Authors

A. Agarwal, University of Pennsylvania
H. Budd, University of Rochester
J. Capó, Institut de Física d'Altes Energies, Bellaterra
P. Chong, University of Pennsylvania
G. Christodoulou, Organisation Européenne pour la Recherche Nucléaire
M. Danilov, P.N. Lebedev Physical Institute of the Russian Academy of Sciences
A. Dergacheva, Institute for Nuclear Research of the Russian Academy of Sciences
A. De Roeck, Organisation Européenne pour la Recherche Nucléaire
N. Dokania, Stony Brook University
D. Douqa, Université de Genève
K. Dugas, Louisiana State University
S. Fedotov, Institute for Nuclear Research of the Russian Academy of Sciences
S. Gwon, Chung-Ang University
R. Howell, University of Rochester
K. Iwamoto, The University of Tokyo
C. Jesús-Valls, Institut de Física d'Altes Energies, Bellaterra
C. K. Jung, Stony Brook University
S. P. Kasetti, Louisiana State University
M. Khabibullin, Institute for Nuclear Research of the Russian Academy of Sciences
A. Khotjantsev, Institute for Nuclear Research of the Russian Academy of Sciences
T. Kikawa, Kyoto University
U. Kose, Organisation Européenne pour la Recherche Nucléaire
Y. Kudenko, Institute for Nuclear Research of the Russian Academy of Sciences
S. Kuribayashi, Kyoto University
T. Kutter, Louisiana State University
D. Last, University of Pennsylvania
L. S. Lin, University of Pennsylvania
S. Lin, Louisiana State University
T. Lux, Institut de Física d'Altes Energies, Bellaterra
S. Manly, University of Rochester
D. A. Martinez Caicedo, South Dakota School of Mines & Technology
S. Martynenko, Stony Brook University
T. Matsubara, High Energy Accelerator Research Organization, Tsukuba

Document Type

Article

Publication Date

5-10-2023

Abstract

In order to extract neutrino oscillation parameters, long-baseline neutrino oscillation experiments rely on detailed models of neutrino interactions with nuclei. These models constitute an important source of systematic uncertainty, partially because detectors to date have been blind to final state neutrons. Three-dimensional projection scintillator trackers comprise components of the near detectors of the next generation long-baseline neutrino experiments. Due to the good timing resolution and fine granularity, this technology is capable of measuring neutron kinetic energy in neutrino interactions on an event-by-event basis and will provide valuable data for refining neutrino interaction models and ways to reconstruct neutrino energy. Two prototypes have been exposed to the neutron beamline at Los Alamos National Laboratory (LANL) in both 2019 and 2020, with neutron energies between 0 and 800 MeV. In order to demonstrate the capability of neutron detection, the total neutron-scintillator cross section as a function of neutron energy is measured and compared to external measurements. The measured total neutron cross section in scintillator between 98 and 688 MeV is 0.36 ± 0.05 barn.

Publication Source (Journal or Book title)

Physics Letters Section B Nuclear Elementary Particle and High Energy Physics

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