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
AUTHORS (50)
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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