论文标题

大气中微子在大型液体阶层检测器上引起的中性背景:ii。原位测量方法

Neutral-current background induced by atmospheric neutrinos at large liquid-scintillator detectors: II. Methodology for in situ measurements

论文作者

Cheng, Jie, Li, Yu-Feng, Lu, Hao-Qi, Wen, Liang-Jian

论文摘要

在寻找弥漫性超新星中微子背景和核子衰减时,未来的大型液体阶层(LS)探测器与水 - 切伦科夫探测器具有竞争力,并与水 - 切伦科夫探测器互补。在同伴论文中,我们对LS检测器中的$^{\ rm c} $ nuclei对大气中微子相互作用引起的中性 - 电流(NC)背景进行了系统的计算,这些探测器中预计这对于对扩散超级neprino中子背景和成核的实验搜索至关重要。在本文中,我们对NC背景的测量进行了系统的研究,并评估了相关的不确定性。我们首先利用NC背景的特征,特别是中子和亲的多重性,以及可能与不稳定残留核的关联。事实证明,中子多样性分布非常强大,可以区分不同的模型。然后,我们开发了一种最大似然方法,以允许{\ it原位测量NC相互作用与三连合签名。最后,提出了一种数据驱动的方法来评估搜索弥漫性超新星中微子背景时NC背景的不确定性。我们得出的结论是,未来的大型LS实验(例如Juno(Jiangmen Underground Neutminino天文台))将能够为全球数据设置做出独特的贡献,以改善$^{12} $ c的大气中微子NC相互作用的预测。

Future large liquid-scintillator (LS) detectors are competitive with and complementary to the water-Cherenkov detectors on the searches for diffuse supernova neutrino background and nucleon decay. In a companion paper, we have performed a systematic calculation of the neutral-current (NC) background induced by atmospheric neutrino interactions on $^{12}{\rm C}$ nuclei in LS detectors, which are expected to be crucially important for the experimental searches for the diffuse supernova neutrino background and nucleon decay. In this paper, we perform a systematic study on the measurement of the NC background and evaluate the associated uncertainties. We first exploit the characteristics of the NC background, in particular, the multiplicities of neutrons and pions, and the possible association with unstable residual nuclei. It turns out that the neutron multiplicity distribution is very powerful to discriminate among different models. Then, we develop a maximum-likelihood method to allow an {\it in situ} measurement of the NC interactions with a triple-coincidence signature. Finally, a data-driven approach is proposed to evaluate the uncertainty of the NC background in the search for the diffuse supernova neutrino background. We conclude that future large LS experiments like JUNO (Jiangmen Underground Neutrino Observatory) will be able to make a unique contribution to the worldwide data set to improve the prediction of atmospheric neutrino NC interactions on $^{12}$C.

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