e-{\mu} Discrimination at High Energy in the JUNO Detector

G. Settanta, S. Mari, C. Martellini, P. Montini
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引用次数: 3

Abstract

Cosmic Ray and neutrino oscillation physics can be studied by using atmospheric neutrinos. JUNO (Jiangmen Underground Neutrino Observatory) is a large liquid scintillator detector with low energy detection threshold and excellent energy resolution. The detector performances allow the atmospheric neutrino oscillation measurements. In this work, a discrimination algorithm for different reaction channels of neutrino-nucleon interactions in the JUNO liquid scintillator, in the GeV/sub-GeV energy region, is presented. The atmospheric neutrino flux is taken as reference, considering $\overset{(-)}{\nu_\mu}$ and $\overset{(-)}{\nu_e}$. The different temporal behaviour of the classes of events have been exploited to build a time profile-based discrimination algorithm. The results show a good selection power for $\overset{(-)}{\nu_e}$ CC events, while the $\overset{(-)}{\nu_\mu}$ CC component suffers of an important contamination from NC events at low energy, which is under study. Preliminary results are presented.
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朱诺探测器高能e-{\mu}鉴别
利用大气中微子可以研究宇宙射线和中微子振荡物理。JUNO(江门地下中微子天文台)是一种大型液体闪烁探测器,具有低能量探测阈值和优异的能量分辨率。探测器的性能允许对大气中微子振荡进行测量。本文提出了一种针对JUNO液体闪烁体在GeV/亚GeV能量区域中中微子-核子相互作用不同反应通道的判别算法。以大气中微子通量为参考,考虑$\overset{(-)}{\nu_\mu}$和$\overset{(-)}{\nu_e}$。事件类的不同时间行为已被利用来建立一个基于时间轮廓的区分算法。结果表明,对$\overset{(-)}{\nu_e}$ CC事件具有良好的选择能力,而$\overset{(-)}{\nu_\mu}$ CC分量在低能量时受到NC事件的严重污染,目前正在研究中。给出了初步结果。
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