Neutrino oscillation studies in JUNO

Wenjie Wu
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引用次数: 1

Abstract

Neutrino oscillation is the first observed phenomenon beyond the Standard Model, which can be interpreted in the framework of three neutrino mixings. It is governed by three mixing angles, two mass-squared differences, and one Dirac CP violation phase. The neutrino mass ordering, CP violation phase and the octant of θ 23 remain unknown and could be measured by next-generation neutrino oscillation experiments. Jiangmen Underground Neutrino Observatory (JUNO) consists of a 20 kiloton liquid scintillator detector, which primarily aims to determine the neutrino mass ordering by measuring the reactor antineutrino oscillation pattern at a baseline of about 53 km. A 3 − 4 σ significance to resolve mass orderings could be reached after 6 years of operation benefiting from its unprecedented 3% energy resolution at 1 MeV. Besides, JUNO is able to perform measurements at an accuracy of better than 1% to oscillation parameters sin 2 θ 12 , ∆ m 2 21 and ∆ m 2 32 . In this talk, neutrino oscillation studies in JUNO will be reviewed.
朱诺号上的中微子振荡研究
中微子振荡是第一个被观测到的超越标准模型的现象,它可以用三种中微子混合的框架来解释。它由三个混合角、两个质量平方差和一个狄拉克CP破坏相控制。中微子的质量序、CP违和相和θ 23的八次方尚不清楚,可以通过下一代中微子振荡实验来测量。江门地下中微子天文台(JUNO)由一个2万吨级的液体闪烁体探测器组成,其主要目的是通过测量反应堆在约53公里基线处的反中微子振荡模式来确定中微子的质量顺序。在运行6年后,由于其在1mev下前所未有的3%能量分辨率,可以达到3−4 σ的显著性。此外,朱诺能够以优于1%的精度对振荡参数sin 2 θ 12、∆m 2 21和∆m 2 32进行测量。在这次演讲中,将回顾JUNO上的中微子振荡研究。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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