三维中微子探测器supergd的时间分辨率研究

IF 0.4 4区 物理与天体物理 Q4 PHYSICS, NUCLEAR
M. Kolupanova, A. Mefodev
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引用次数: 0

摘要

时间分辨率是探测器的重要参数。高时间分辨率对于粒子识别和在短时间和空间间隔内事件重建的准确性是必要的,因为它允许在探测器内测量介子反中微子相互作用中的中子截面。它对于恢复相互作用的完整运动学,改善中微子能量的重建,从而减少振荡分析中的系统不确定性至关重要。本研究介绍了作为T2K实验升级探测器ND280复合物的主动目标研制的supergd探测器进行时间分辨率测量的结果。选择完全穿过探测器活动区域的直线宇宙轨迹进行时间校准。所开发的算法计算与电缆长度、到MPPC的距离和时间行走效应相关的时延。在40个光电子的阈值下,使用来自上游和侧光纤的轨迹中命中的时间分布相对于每个事件的平均时间测量的时间分辨率的初步结果为\(\sigma=1.12\) ns。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

The Study of the Time Resolution of the 3D Neutrino Detector SuperFGD

The Study of the Time Resolution of the 3D Neutrino Detector SuperFGD

Time resolution is important parameter of the detector. High time resolution is necessary for particle identification and the accuracy of the event reconstruction at short time and space intervals as it allows for measuring neutron cross-sections in muon antineutrino interactions within the detector. It is critical for restoring the complete kinematics of the interaction, improving the reconstruction of neutrino energy, and consequently reducing systematic uncertainties in oscillation analysis. This research presents the results of time resolution measurements made with the SuperFGD detector which was developed as an active target of the upgraded detector ND280 complex of the T2K experiment. Straight cosmic tracks passing entirely through the active region of the detector were selected for time calibration. The developed algorithm calculates time delays associated with cable length, the distance from the MPPC and time-walk effect. Preliminary result of the time resolution measured using the time distribution of hits in the track from both upstream and side fibers with respect to the average time of each event is \(\sigma=1.12\) ns for a threshold of 40 photoelectrons.

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来源期刊
Physics of Atomic Nuclei
Physics of Atomic Nuclei 物理-物理:核物理
CiteScore
0.60
自引率
25.00%
发文量
56
审稿时长
3-6 weeks
期刊介绍: Physics of Atomic Nuclei is a journal that covers experimental and theoretical studies of nuclear physics: nuclear structure, spectra, and properties; radiation, fission, and nuclear reactions induced by photons, leptons, hadrons, and nuclei; fundamental interactions and symmetries; hadrons (with light, strange, charm, and bottom quarks); particle collisions at high and superhigh energies; gauge and unified quantum field theories, quark models, supersymmetry and supergravity, astrophysics and cosmology.
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