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Gwon, S.; Granger, P.; Yang, G.; Bolognesi, S.; Cai, T.; Danilov, M.; Delbart, A.; De Roeck, A.; Dolan, S.; Eurin, G.; Razakamiandra, R. F.; Fedotov, S.; Fiorentini Aguirre, G.; Flight, R.; Gran, R.; Ha, C.; Jung, C. K.; Jung, K. Y.; Kettell, S.; Khabibullin, M.; Khotjantsev, A.; Kordosky, M.; Kudenko, Y.; Kutter, T.; Maneira, J.; Manly, S.; Martinez Caicedo, D. A.; Mauger, C.; McFarland, K.; McGrew, C.; Mefodev, A.; Mineev, O.; Naples, D.; Olivier, A.; Paolone, V.; Prasad, S.; Riccio, C.; Rodriguez Rondon, J.; Sgalaberna, D.; Sitraka, A.; Siyeon, K.; Skrobova, N.; Su, H.; Suvorov, S.; Teklu, A.; Tzanov, M.; Valencia, E.; Wood, K.; Worcester, E.; Yershov, N.
Physical review. D, 02/2023, Letnik: 107, Številka: 3Journal Article
Neutrino oscillation experiments require a precise measurement of the neutrino energy. However, the kinematic detection of the final-state neutron in the neutrino interaction is missing in current neutrino oscillation experiments. The missing neutron kinematic detection results in a smaller detected neutrino energy than the true neutrino energy. A novel 3D-projection scintillator tracker, which consists of roughly ten million active cubes covered with an optical reflector, is capable of measuring the neutron kinetic energy and direction on an event-by-event basis using the time-of-flight technique thanks to the fast timing, fine granularity, and high light yield. The $\overline{v}$μ interactions tend to produce neutrons in the final state. By measuring the neutron kinetic energy, the $\overline{v}$μ energy can be reconstructed better, allowing a tighter incoming neutrino flux constraint. This article shows the detector's ability to reconstruct neutron kinetic energy and the $\overline{v}$μ flux constraint achieved by selecting the charged-current interactions without mesons or protons in the final state.
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JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
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in: SICRIS
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