Measurement of Solar $pp$ Neutrino Flux using Electron Recoil Data from PandaX-4T Commissioning Run

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Main Authors: PandaX Collaboration, Lu, Xiaoying, Abdukerim, Abdusalam, Bo, Zihao, Chen, Wei, Chen, Xun, Chen, Yunhua, Cheng, Chen, Cheng, Zhaokan, Cui, Xiangyi, Fan, Yingjie, Fang, Deqing, Geng, Lisheng, Giboni, Karl, Guo, Xuyuan, Han, Chencheng, Han, Ke, He, Changda, He, Jinrong, Huang, Di, Huang, Junting, Huang, Zhou, Hou, Ruquan, Hou, Yu, Ji, Xiangdong, Ju, Yonglin, Li, Chenxiang, Li, Jiafu, Li, Mingchuan, Li, Shuaijie, Li, Tao, Lin, Qing, Liu, Jianglai, Lu, Congcong, Luo, Lingyin, Luo, Yunyang, Ma, Wenbo, Ma, Yugang, Mao, Yajun, Meng, Yue, Ning, Xuyang, Pang, Binyu, Qi, Ningchun, Qian, Zhicheng, Ren, Xiangxiang, Shaheed, Nasir, Shang, Xiaofeng, Shao, Xiyuan, Shen, Guofang, Shen, Manbin, Si, Lin, Sun, Wenliang, Tao, Yi, Wang, Anqing, Wang, Meng, Wang, Qiuhong, Wang, Shaobo, Wang, Siguang, Wang, Wei, Wang, Xiuli, Wang, Xu, Wang, Zhou, Wei, Yuehuan, Wu, Mengmeng, Wu, Weihao, Wu, Yuan, Xiao, Mengjiao, Xiao, Xiang, Xiong, Kaizhi, Yan, Binbin, Yan, Xiyu, Yang, Yong, Yu, Chunxu, Yuan, Ying, Yuan, Zhe, Yun, Youhui, Zeng, Xinning, Zhang, Minzhen, Zhang, Peng, Zhang, Shibo, Zhang, Shu, Zhang, Tao, Zhang, Wei, Zhang, Yang, Zhang, Yingxin, Zhang, Yuanyuan, Zhao, Li, Zhou, Jifang, Zhou, Ning, Zhou, Xiaopeng, Zhou, Yubo, Zhou, Zhizhen
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Published: 2024
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author PandaX Collaboration
Lu, Xiaoying
Abdukerim, Abdusalam
Bo, Zihao
Chen, Wei
Chen, Xun
Chen, Yunhua
Cheng, Chen
Cheng, Zhaokan
Cui, Xiangyi
Fan, Yingjie
Fang, Deqing
Geng, Lisheng
Giboni, Karl
Guo, Xuyuan
Han, Chencheng
Han, Ke
He, Changda
He, Jinrong
Huang, Di
Huang, Junting
Huang, Zhou
Hou, Ruquan
Hou, Yu
Ji, Xiangdong
Ju, Yonglin
Li, Chenxiang
Li, Jiafu
Li, Mingchuan
Li, Shuaijie
Li, Tao
Lin, Qing
Liu, Jianglai
Lu, Congcong
Luo, Lingyin
Luo, Yunyang
Ma, Wenbo
Ma, Yugang
Mao, Yajun
Meng, Yue
Ning, Xuyang
Pang, Binyu
Qi, Ningchun
Qian, Zhicheng
Ren, Xiangxiang
Shaheed, Nasir
Shang, Xiaofeng
Shao, Xiyuan
Shen, Guofang
Shen, Manbin
Si, Lin
Sun, Wenliang
Tao, Yi
Wang, Anqing
Wang, Meng
Wang, Qiuhong
Wang, Shaobo
Wang, Siguang
Wang, Wei
Wang, Xiuli
Wang, Xu
Wang, Zhou
Wei, Yuehuan
Wu, Mengmeng
Wu, Weihao
Wu, Yuan
Xiao, Mengjiao
Xiao, Xiang
Xiong, Kaizhi
Yan, Binbin
Yan, Xiyu
Yang, Yong
Yu, Chunxu
Yuan, Ying
Yuan, Zhe
Yun, Youhui
Zeng, Xinning
Zhang, Minzhen
Zhang, Peng
Zhang, Shibo
Zhang, Shu
Zhang, Tao
Zhang, Wei
Zhang, Yang
Zhang, Yingxin
Zhang, Yuanyuan
Zhao, Li
Zhou, Jifang
Zhou, Ning
Zhou, Xiaopeng
Zhou, Yubo
Zhou, Zhizhen
author_facet PandaX Collaboration
Lu, Xiaoying
Abdukerim, Abdusalam
Bo, Zihao
Chen, Wei
Chen, Xun
Chen, Yunhua
Cheng, Chen
Cheng, Zhaokan
Cui, Xiangyi
Fan, Yingjie
Fang, Deqing
Geng, Lisheng
Giboni, Karl
Guo, Xuyuan
Han, Chencheng
Han, Ke
He, Changda
He, Jinrong
Huang, Di
Huang, Junting
Huang, Zhou
Hou, Ruquan
Hou, Yu
Ji, Xiangdong
Ju, Yonglin
Li, Chenxiang
Li, Jiafu
Li, Mingchuan
Li, Shuaijie
Li, Tao
Lin, Qing
Liu, Jianglai
Lu, Congcong
Luo, Lingyin
Luo, Yunyang
Ma, Wenbo
Ma, Yugang
Mao, Yajun
Meng, Yue
Ning, Xuyang
Pang, Binyu
Qi, Ningchun
Qian, Zhicheng
Ren, Xiangxiang
Shaheed, Nasir
Shang, Xiaofeng
Shao, Xiyuan
Shen, Guofang
Shen, Manbin
Si, Lin
Sun, Wenliang
Tao, Yi
Wang, Anqing
Wang, Meng
Wang, Qiuhong
Wang, Shaobo
Wang, Siguang
Wang, Wei
Wang, Xiuli
Wang, Xu
Wang, Zhou
Wei, Yuehuan
Wu, Mengmeng
Wu, Weihao
Wu, Yuan
Xiao, Mengjiao
Xiao, Xiang
Xiong, Kaizhi
Yan, Binbin
Yan, Xiyu
Yang, Yong
Yu, Chunxu
Yuan, Ying
Yuan, Zhe
Yun, Youhui
Zeng, Xinning
Zhang, Minzhen
Zhang, Peng
Zhang, Shibo
Zhang, Shu
Zhang, Tao
Zhang, Wei
Zhang, Yang
Zhang, Yingxin
Zhang, Yuanyuan
Zhao, Li
Zhou, Jifang
Zhou, Ning
Zhou, Xiaopeng
Zhou, Yubo
Zhou, Zhizhen
contents The proton-proton ($pp$) fusion chain dominates the neutrino production from the Sun. The uncertainty of the predicted $pp$ neutrino flux is at the sub-percent level, whereas that of the best measurement is $\mathcal{O}(10\%)$. In this paper, we present the first result to measure the solar $pp$ neutrinos in the electron recoil energy range from 24 to 144 keV, using the PandaX-4T commissioning data with 0.63 tonne$\times$year exposure. The $pp$ neutrino flux is determined to be $(8.0 \pm 3.9 \,{\rm{(stat)}} \pm 10.0 \,{\rm{(syst)}} )\times 10^{10}\, $$\rm{s}^{-1} \rm{cm}^{-2}$, consistent with Standard Solar Model and existing measurements, corresponding to a flux upper limit of $23.3\times 10^{10}\, $$\rm{s}^{-1} \rm{cm}^{-2}$ at 90\% C.L..
format Preprint
id arxiv_https___arxiv_org_abs_2401_07045
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Measurement of Solar $pp$ Neutrino Flux using Electron Recoil Data from PandaX-4T Commissioning Run
PandaX Collaboration
Lu, Xiaoying
Abdukerim, Abdusalam
Bo, Zihao
Chen, Wei
Chen, Xun
Chen, Yunhua
Cheng, Chen
Cheng, Zhaokan
Cui, Xiangyi
Fan, Yingjie
Fang, Deqing
Geng, Lisheng
Giboni, Karl
Guo, Xuyuan
Han, Chencheng
Han, Ke
He, Changda
He, Jinrong
Huang, Di
Huang, Junting
Huang, Zhou
Hou, Ruquan
Hou, Yu
Ji, Xiangdong
Ju, Yonglin
Li, Chenxiang
Li, Jiafu
Li, Mingchuan
Li, Shuaijie
Li, Tao
Lin, Qing
Liu, Jianglai
Lu, Congcong
Luo, Lingyin
Luo, Yunyang
Ma, Wenbo
Ma, Yugang
Mao, Yajun
Meng, Yue
Ning, Xuyang
Pang, Binyu
Qi, Ningchun
Qian, Zhicheng
Ren, Xiangxiang
Shaheed, Nasir
Shang, Xiaofeng
Shao, Xiyuan
Shen, Guofang
Shen, Manbin
Si, Lin
Sun, Wenliang
Tao, Yi
Wang, Anqing
Wang, Meng
Wang, Qiuhong
Wang, Shaobo
Wang, Siguang
Wang, Wei
Wang, Xiuli
Wang, Xu
Wang, Zhou
Wei, Yuehuan
Wu, Mengmeng
Wu, Weihao
Wu, Yuan
Xiao, Mengjiao
Xiao, Xiang
Xiong, Kaizhi
Yan, Binbin
Yan, Xiyu
Yang, Yong
Yu, Chunxu
Yuan, Ying
Yuan, Zhe
Yun, Youhui
Zeng, Xinning
Zhang, Minzhen
Zhang, Peng
Zhang, Shibo
Zhang, Shu
Zhang, Tao
Zhang, Wei
Zhang, Yang
Zhang, Yingxin
Zhang, Yuanyuan
Zhao, Li
Zhou, Jifang
Zhou, Ning
Zhou, Xiaopeng
Zhou, Yubo
Zhou, Zhizhen
High Energy Physics - Experiment
The proton-proton ($pp$) fusion chain dominates the neutrino production from the Sun. The uncertainty of the predicted $pp$ neutrino flux is at the sub-percent level, whereas that of the best measurement is $\mathcal{O}(10\%)$. In this paper, we present the first result to measure the solar $pp$ neutrinos in the electron recoil energy range from 24 to 144 keV, using the PandaX-4T commissioning data with 0.63 tonne$\times$year exposure. The $pp$ neutrino flux is determined to be $(8.0 \pm 3.9 \,{\rm{(stat)}} \pm 10.0 \,{\rm{(syst)}} )\times 10^{10}\, $$\rm{s}^{-1} \rm{cm}^{-2}$, consistent with Standard Solar Model and existing measurements, corresponding to a flux upper limit of $23.3\times 10^{10}\, $$\rm{s}^{-1} \rm{cm}^{-2}$ at 90\% C.L..
title Measurement of Solar $pp$ Neutrino Flux using Electron Recoil Data from PandaX-4T Commissioning Run
topic High Energy Physics - Experiment
url https://arxiv.org/abs/2401.07045