Detecting Neutrinos from Supernova Bursts in PandaX-4T

Fuente: arXiv
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Auteurs principaux: Pang, Binyu, Abdukerim, Abdusalam, Bo, Zihao, Chen, Wei, Chen, Xun, Cheng, Chen, 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, 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, Lu, Xiaoying, Luo, Lingyin, Luo, Yunyang, Ma, Wenbo, Ma, Yugang, Mao, Yajun, Meng, Yue, Ning, Xuyang, Qi, Ningchun, Qian, Zhicheng, Ren, Xiangxiang, Shaheed, Nasir, Shang, Xiaofeng, Shao, Xiyuan, 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, Yao, Yukun, Yu, Chunxu, Yuan, Ying, Yuan, Zhe, Zeng, Xinning, Zhang, Dan, Zhang, Minzhen, Zhang, Peng, Zhang, Shibo, Zhang, Shu, Zhang, Tao, Zhang, Wei, Zhang, Yang, Zhang, Yingxin, Zhang, Yuanyuan, Zhao, Li, Zheng, Qibin, Zhou, Jifang, Zhou, Ning, Zhou, Xiaopeng, Zhou, Yong, Zhou, Yubo
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Publié: 2024
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_version_ 1866913260656132096
author Pang, Binyu
Abdukerim, Abdusalam
Bo, Zihao
Chen, Wei
Chen, Xun
Cheng, Chen
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, 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
Lu, Xiaoying
Luo, Lingyin
Luo, Yunyang
Ma, Wenbo
Ma, Yugang
Mao, Yajun
Meng, Yue
Ning, Xuyang
Qi, Ningchun
Qian, Zhicheng
Ren, Xiangxiang
Shaheed, Nasir
Shang, Xiaofeng
Shao, Xiyuan
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
Yao, Yukun
Yu, Chunxu
Yuan, Ying
Yuan, Zhe
Zeng, Xinning
Zhang, Dan
Zhang, Minzhen
Zhang, Peng
Zhang, Shibo
Zhang, Shu
Zhang, Tao
Zhang, Wei
Zhang, Yang
Zhang, Yingxin
Zhang, Yuanyuan
Zhao, Li
Zheng, Qibin
Zhou, Jifang
Zhou, Ning
Zhou, Xiaopeng
Zhou, Yong
Zhou, Yubo
author_facet Pang, Binyu
Abdukerim, Abdusalam
Bo, Zihao
Chen, Wei
Chen, Xun
Cheng, Chen
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, 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
Lu, Xiaoying
Luo, Lingyin
Luo, Yunyang
Ma, Wenbo
Ma, Yugang
Mao, Yajun
Meng, Yue
Ning, Xuyang
Qi, Ningchun
Qian, Zhicheng
Ren, Xiangxiang
Shaheed, Nasir
Shang, Xiaofeng
Shao, Xiyuan
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
Yao, Yukun
Yu, Chunxu
Yuan, Ying
Yuan, Zhe
Zeng, Xinning
Zhang, Dan
Zhang, Minzhen
Zhang, Peng
Zhang, Shibo
Zhang, Shu
Zhang, Tao
Zhang, Wei
Zhang, Yang
Zhang, Yingxin
Zhang, Yuanyuan
Zhao, Li
Zheng, Qibin
Zhou, Jifang
Zhou, Ning
Zhou, Xiaopeng
Zhou, Yong
Zhou, Yubo
contents Neutrinos from core-collapse supernovae are essential for the understanding of neutrino physics and stellar evolution. The dual-phase xenon dark matter detectors can provide a way to track explosions of galactic supernovae by detecting neutrinos through coherent elastic neutrino-nucleus scatterings. In this study, a variation of progenitor masses as well as explosion models are assumed to predict the neutrino fluxes and spectra, which result in the number of expected neutrino events ranging from 6.6 to 13.7 at a distance of 10 kpc over a 10-second duration with negligible backgrounds at PandaX-4T. Two specialized triggering alarms for monitoring supernova burst neutrinos are built. The efficiency of detecting supernova explosions at various distances in the Milky Way is estimated. These alarms will be implemented in the real-time supernova monitoring system at PandaX-4T in the near future, providing the astronomical communities with supernova early warnings.
format Preprint
id arxiv_https___arxiv_org_abs_2403_06220
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Detecting Neutrinos from Supernova Bursts in PandaX-4T
Pang, Binyu
Abdukerim, Abdusalam
Bo, Zihao
Chen, Wei
Chen, Xun
Cheng, Chen
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, 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
Lu, Xiaoying
Luo, Lingyin
Luo, Yunyang
Ma, Wenbo
Ma, Yugang
Mao, Yajun
Meng, Yue
Ning, Xuyang
Qi, Ningchun
Qian, Zhicheng
Ren, Xiangxiang
Shaheed, Nasir
Shang, Xiaofeng
Shao, Xiyuan
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
Yao, Yukun
Yu, Chunxu
Yuan, Ying
Yuan, Zhe
Zeng, Xinning
Zhang, Dan
Zhang, Minzhen
Zhang, Peng
Zhang, Shibo
Zhang, Shu
Zhang, Tao
Zhang, Wei
Zhang, Yang
Zhang, Yingxin
Zhang, Yuanyuan
Zhao, Li
Zheng, Qibin
Zhou, Jifang
Zhou, Ning
Zhou, Xiaopeng
Zhou, Yong
Zhou, Yubo
High Energy Physics - Experiment
Instrumentation and Detectors
Neutrinos from core-collapse supernovae are essential for the understanding of neutrino physics and stellar evolution. The dual-phase xenon dark matter detectors can provide a way to track explosions of galactic supernovae by detecting neutrinos through coherent elastic neutrino-nucleus scatterings. In this study, a variation of progenitor masses as well as explosion models are assumed to predict the neutrino fluxes and spectra, which result in the number of expected neutrino events ranging from 6.6 to 13.7 at a distance of 10 kpc over a 10-second duration with negligible backgrounds at PandaX-4T. Two specialized triggering alarms for monitoring supernova burst neutrinos are built. The efficiency of detecting supernova explosions at various distances in the Milky Way is estimated. These alarms will be implemented in the real-time supernova monitoring system at PandaX-4T in the near future, providing the astronomical communities with supernova early warnings.
title Detecting Neutrinos from Supernova Bursts in PandaX-4T
topic High Energy Physics - Experiment
Instrumentation and Detectors
url https://arxiv.org/abs/2403.06220