Neutron detection and application with a novel 3D-projection scintillator tracker in the future long-baseline neutrino oscillation experiments

Physics - Instrumentation and Detectors kinetic interaction FOS: Physical sciences n final state meson time-of-flight Atomic 7. Clean energy charged current High Energy Physics - Experiment neutrino High Energy Physics - Experiment (hep-ex) 03 medical and health sciences Particle and Plasma Physics High Energy Physics - Phenomenology (hep-ph) 0302 clinical medicine Affordable and Clean Energy optical [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] Nuclear tracking detector [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] scintillation counter Quantum Physics Molecular Particle and High Energy Physics Instrumentation and Detectors (physics.ins-det) oscillation Nuclear and Plasma Physics Nuclear & Particles Physics current Synchrotrons and Accelerators flux High Energy Physics - Phenomenology Particle and high energy physics kinematics Mathematical physics [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph] Physical Sciences Astronomical sciences Astronomical and Space Sciences energy
DOI: 10.1103/physrevd.107.032012 Publication Date: 2023-02-27T16:44:13Z
ABSTRACT
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 feed-down of the detected neutrino energy compared to the true neutrino energy. A novel 3D\textcolor{black}{-}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 $\barν_μ$ interactions tend to produce neutrons in the final state. By inferring the neutron kinetic energy, the $\barν_μ$ energy can be reconstructed better, allowing a tighter incoming neutrino flux constraint. This paper shows the detector's ability to reconstruct neutron kinetic energy and the $\barν_μ$ flux constraint achieved by selecting the charged-current interactions without mesons or protons in the final state.
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