학술논문
A First Search for Solar $^8$B Neutrino in the PandaX-4T Experiment using Neutrino-Nucleus Coherent Scattering
Document Type
Working Paper
Author
Ma, Wenbo; Abdukerim, Abdusalam; Cheng, Chen; Bo, Zihao; Chen, Wei; Chen, Xun; Chen, Yunhua; Cheng, Zhaokan; Cui, Xiangyi; Fan, Yingjie; Fang, Deqing; Fu, Changbo; Fu, Mengting; Geng, Lisheng; Giboni, Karl; Gu, Linhui; Guo, Xuyuan; Han, Chencheng; Han, Ke; He, Changda; He, Jinrong; Huang, Di; Huang, Yanlin; Huang, Zhou; Hou, Ruquan; Ji, Xiangdong; Ju, Yonglin; Li, Chenxiang; Li, Jiafu; Li, Mingchuan; Li, Shu; Li, Shuaijie; Lin, Qing; Liu, Jianglai; Lu, Xiaoying; Luo, Lingyin; Luo, Yunyang; Ma, Yugang; Mao, Yajun; Shaheed, Nasir; Meng, Yue; Ning, Xuyang; Qi, Ningchun; Qian, Zhicheng; Ren, Xiangxiang; Shang, Changsong; Shang, Xiaofeng; Shen, Guofang; Si, Lin; Sun, Wenliang; Tan, Andi; Tao, Yi; Wang, Anqing; Wang, Meng; Wang, Qiuhong; Wang, Shaobo; Wang, Siguang; Wang, Wei; Wang, Xiuli; Wang, Zhou; Wei, Yuehuan; Wu, Mengmeng; Wu, Weihao; Xia, Jingkai; Xiao, Mengjiao; Xiao, Xiang; Xie, Pengwei; Yan, Binbin; Yan, Xiyu; Yang, Jijun; Yang, Yong; Yu, Chunxu; Yuan, Jumin; Yuan, Ying; Yuan, Zhe; Zeng, Xinning; Zhang, Dan; Zhang, Minzhen; Zhang, Peng; Zhang, Shibo; Zhang, Shu; Zhang, Tao; Zhang, Yingxin; Zhang, Yuanyuan; Zhao, Li; Zheng, Qibin; Zhou, Jifang; Zhou, Ning; Zhou, Xiaopeng; Zhou, Yong; Zhou, Yubo
Source
Physical Review Letters 130, 021802 (2023)
Subject
Language
Abstract
A search for interactions from solar $^8$B neutrinos elastically scattering off xenon nuclei using PandaX-4T commissioning data is reported. The energy threshold of this search is further lowered compared with the previous search for dark matter, with various techniques utilized to suppress the background that emerges from data with the lowered threshold. A blind analysis is performed on the data with an effective exposure of 0.48 tonne$\cdot$year, and no significant excess of events is observed. Among results obtained using the neutrino-nucleus coherent scattering, our results give the best constraint on the solar $^8$B neutrino flux. We further provide a more stringent limit on the cross section between dark matter and nucleon in the mass range from 3 to 9 GeV/c$^2$.
Comment: 5 pages, 4 figures
Comment: 5 pages, 4 figures