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RELICS: a REactor neutrino LIquid xenon Coherent elastic Scattering experiment

Authors :
Cai, Chang
Chen, Guocai
Chen, Jiangyu
Fang, Rundong
Gao, Fei
Guo, Xiaoran
Guo, Jiheng
He, Tingyi
Jia, Chengjie
Jin, Gaojun
Jing, Yipin
Ju, Gaojun
Lei, Yang
Li, Jiayi
Li, Kaihang
Li, Meng
Li, Minhua
Li, Shengchao
Li, Siyin
Li, Tao
Lin, Qing
Liu, Jiajun
Liu, Minghao
Lv, Sheng
Luo, Guang
Ma, Jian
Shen, Chuanping
Song, Mingzhuo
Tong, Lijun
Wang, Xiaoyu
Wang, Wei
Wang, Xiaoping
Wang, Zihu
Wei, Yuehuan
Weng, Liming
Xiao, Xiang
Xie, Lingfeng
Xu, Dacheng
Yang, Jijun
Yang, Litao
Yang, Long
Ye, Jingqiang
Yu, Jiachen
Yue, Qian
Yue, Yuyong
Zhang, Bingwei
Zhang, Shuhao
Zhao, Yifei
Zhu, Chenhui
Publication Year :
2024

Abstract

Coherent elastic neutrino-nucleus scattering (CEvNS) provides a unique probe for neutrino properties Beyond the Standard Model (BSM) physics. REactor neutrino LIquid xenon Coherent Scattering experiment (RELICS), a proposed reactor neutrino program using liquid xenon time projection chamber (LXeTPC) technology, aims to investigate the CEvNS process of antineutrinos off xenon atomic nuclei. In this work, the design of the experiment is studied and optimized based on Monte Carlo (MC) simulations. To achieve a sufficiently low energy threshold for CEvNS detection, an ionization-only analysis channel is adopted for RELICS. A high emission rate of delayed electrons after a big ionization signal is the major background, leading to an analysis threshold of 120 photo-electrons in the CEvNS search. The second largest background, nuclear recoils induced by cosmic-ray neutrons, is suppressed via a passive water shield. The physics potential of RELICS is explored with a 32 kg-yr exposure at a baseline of 25 m from a reactor core with a 3 GW thermal power. In an energy range of 120 to 240 PE, we expect 4902.4 CEvNS and 1318.4 background events. The sensitivity of RELICS to the weak mixing angle is investigated at a low momentum transfer. Our study shows that RELICS can further improve the constraints on the non-standard neutrino interaction (NSI) compared to the current best results.

Subjects

Subjects :
High Energy Physics - Experiment

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.2405.05554
Document Type :
Working Paper