Detecting neutrinos from supernova bursts in PandaX-4T

Binyu Pang; Abdusalam Abdukerim; Zihao Bo; Wei Chen; Xun Chen; Chen Cheng; Zhaokan Cheng; Xiangyi Cui; Yingjie Fan; Deqing Fang; Changbo Fu; Mengting Fu; Lisheng Geng; Karl Giboni; Linhui Gu; Xuyuan Guo; Chencheng Han; Ke Han; Changda He; Jinrong He; Di Huang; Yanlin Huang; Junting Huang; Zhou Huang; Ruquan Hou; Yu Hou; Xiangdong Ji; Yonglin Ju; Chenxiang Li; Jiafu Li; Mingchuan Li; Shuaijie Li; Tao Li; Qing Lin; Qi Jianglaing Liu; Congcong Lu; Xiaoying Lu; Lingyin Luo; Yunyang Luo; Wenbo Ma; Yugang Ma; Yajun Mao; Yue Meng; Xuyang Ning; Ningchun Qi; Zhicheng Qian; Xiangxiang Ren; Nasir Shaheed; Xiaofeng Shang; Xiyuan Shao; Guofang Shen; Lin Si; Wenliang Sun; Andi Tan; Yi Tao; Anqing Wang; Meng Wang; Qiuhong Wang; Shaobo Wang; Siguang Wang; Wei Wang; Xiuli Wang; Zhou Wang; Yuehuan Wei; Mengmeng Wu; Weihao Wu; Jingkai Xia; Mengjiao Xiao; Xiang Xiao; Pengwei Xie; Binbin Yan; Xiyu Yan; Jijun Yang; Yong Yang; Yukun Yao; Chunxu Yu; Ying Yuan; Zhe Yuan; Xinning Zeng; Dan Zhang; Minzhen Zhang; Peng Zhang; Shibo Zhang; Shu Zhang; Tao Zhang; Yang Zhang; Yingxin Zhang; Yuanyuan Zhang; Li Zhao; Qibin Zheng; Jifang Zhou; Ning Zhou; Xiaopeng Zhou; Yong Zhou; Yubo Zhou

doi:10.1088/1674-1137/ad3efe

Detecting neutrinos from supernova bursts in PandaX-4T

Binyu Pang, Abdusalam Abdukerim, Zihao Bo, Wei Chen, Xun Chen, Chen Cheng, Zhaokan Cheng, Xiangyi Cui, Yingjie Fan, Deqing Fang, Changbo Fu, Mengting Fu, Lisheng Geng, Karl Giboni, Linhui Gu, Xuyuan Guo, Chencheng Han, Ke Han, Changda He, Jinrong HeDi Huang, Yanlin Huang, Junting Huang, Zhou Huang, Ruquan Hou, Yu Hou, Xiangdong Ji, Yonglin Ju, Chenxiang Li, Jiafu Li, Mingchuan Li, Shuaijie Li, Tao Li, Qing Lin, Qi Jianglaing Liu, Congcong Lu, Xiaoying Lu, Lingyin Luo, Yunyang Luo, Wenbo Ma, Yugang Ma, Yajun Mao, Yue Meng, Xuyang Ning, Ningchun Qi, Zhicheng Qian, Xiangxiang Ren, Nasir Shaheed, Xiaofeng Shang, Xiyuan Shao, Guofang Shen, Lin Si, Wenliang Sun, Andi Tan, Yi Tao, Anqing Wang, Meng Wang, Qiuhong Wang, Shaobo Wang, Siguang Wang, Wei Wang, Xiuli Wang, Zhou Wang, Yuehuan Wei, Mengmeng Wu, Weihao Wu, Jingkai Xia, Mengjiao Xiao, Xiang Xiao, Pengwei Xie, Binbin Yan, Xiyu Yan, Jijun Yang, Yong Yang, Yukun Yao, Chunxu Yu, Ying Yuan, Zhe Yuan, Xinning Zeng, Dan Zhang, Minzhen Zhang, Peng Zhang, Shibo Zhang, Shu Zhang, Tao Zhang, Yang Zhang, Yingxin Zhang, Yuanyuan Zhang, Li Zhao, Qibin Zheng, Jifang Zhou, Ning Zhou, Xiaopeng Zhou, Yong Zhou, Yubo Zhou

Research output: Contribution to journal › Article › peer-review

3 Scopus citations

Abstract

Neutrinos from core-collapse supernovae are essential for understanding neutrino physics and stellar evolution. Dual-phase xenon dark matter detectors can be used to track explosions of galactic supernovae by detecting neutrinos through coherent elastic neutrino-nucleus scatterings. In this study, a variation of progenitor masses and explosion models are assumed to predict 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-s 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, which will provide supernova early warnings for the astronomical community.

Original language	English (US)
Article number	073002
Journal	Chinese Physics C
Volume	48
Issue number	7
DOIs	https://doi.org/10.1088/1674-1137/ad3efe
State	Published - Jul 2024
Externally published	Yes

All Science Journal Classification (ASJC) codes

Nuclear and High Energy Physics
Instrumentation
Astronomy and Astrophysics

Keywords

core-collapse supernovae
liquid xenon detectors
neutrinos
supernova early warnings

Access to Document

10.1088/1674-1137/ad3efe

Cite this

@article{bde64480302740479246fd0018f9576c,

title = "Detecting neutrinos from supernova bursts in PandaX-4T",

abstract = "Neutrinos from core-collapse supernovae are essential for understanding neutrino physics and stellar evolution. Dual-phase xenon dark matter detectors can be used to track explosions of galactic supernovae by detecting neutrinos through coherent elastic neutrino-nucleus scatterings. In this study, a variation of progenitor masses and explosion models are assumed to predict 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-s 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, which will provide supernova early warnings for the astronomical community.",

keywords = "core-collapse supernovae, liquid xenon detectors, neutrinos, supernova early warnings",

author = "Binyu Pang and Abdusalam Abdukerim and Zihao Bo and Wei Chen and Xun Chen and Chen Cheng and Zhaokan Cheng and Xiangyi Cui and Yingjie Fan and Deqing Fang and Changbo Fu and Mengting Fu and Lisheng Geng and Karl Giboni and Linhui Gu and Xuyuan Guo and Chencheng Han and Ke Han and Changda He and Jinrong He and Di Huang and Yanlin Huang and Junting Huang and Zhou Huang and Ruquan Hou and Yu Hou and Xiangdong Ji and Yonglin Ju and Chenxiang Li and Jiafu Li and Mingchuan Li and Shuaijie Li and Tao Li and Qing Lin and Liu, {Qi Jianglaing} and Congcong Lu and Xiaoying Lu and Lingyin Luo and Yunyang Luo and Wenbo Ma and Yugang Ma and Yajun Mao and Yue Meng and Xuyang Ning and Ningchun Qi and Zhicheng Qian and Xiangxiang Ren and Nasir Shaheed and Xiaofeng Shang and Xiyuan Shao and Guofang Shen and Lin Si and Wenliang Sun and Andi Tan and Yi Tao and Anqing Wang and Meng Wang and Qiuhong Wang and Shaobo Wang and Siguang Wang and Wei Wang and Xiuli Wang and Zhou Wang and Yuehuan Wei and Mengmeng Wu and Weihao Wu and Jingkai Xia and Mengjiao Xiao and Xiang Xiao and Pengwei Xie and Binbin Yan and Xiyu Yan and Jijun Yang and Yong Yang and Yukun Yao and Chunxu Yu and Ying Yuan and Zhe Yuan and Xinning Zeng and Dan Zhang and Minzhen Zhang and Peng Zhang and Shibo Zhang and Shu Zhang and Tao Zhang and Yang Zhang and Yingxin Zhang and Yuanyuan Zhang and Li Zhao and Qibin Zheng and Jifang Zhou and Ning Zhou and Xiaopeng Zhou and Yong Zhou and Yubo Zhou",

note = "Publisher Copyright: {\textcopyright} 2024 Chinese Physical Society and the Institute of High Energy Physics of the Chinese Academy of Sciences and the Institute of Modern Physics of the Chinese Academy of Sciences and IOP Publishing Ltd.",

year = "2024",

month = jul,

doi = "10.1088/1674-1137/ad3efe",

language = "English (US)",

volume = "48",

journal = "Chinese Physics C",

issn = "1674-1137",

publisher = "IOP Publishing Ltd.",

number = "7",

}

Pang, B, Abdukerim, A, Bo, Z, Chen, W, Chen, X, Cheng, C, Cheng, Z, Cui, X, Fan, Y, Fang, D, Fu, C, Fu, M, Geng, L, Giboni, K, Gu, L, Guo, X, Han, C, Han, K, He, C, He, J, Huang, D, Huang, Y, Huang, J, Huang, Z, Hou, R, Hou, Y, Ji, X, Ju, Y, Li, C, Li, J, Li, M, Li, S, Li, T, Lin, Q, Liu, QJ, Lu, C, Lu, X, Luo, L, Luo, Y, Ma, W, Ma, Y, Mao, Y, Meng, Y, Ning, X, Qi, N, Qian, Z, Ren, X, Shaheed, N, Shang, X, Shao, X, Shen, G, Si, L, Sun, W, Tan, A, Tao, Y, Wang, A, Wang, M, Wang, Q, Wang, S, Wang, S, Wang, W, Wang, X, Wang, Z, Wei, Y, Wu, M, Wu, W, Xia, J, Xiao, M, Xiao, X, Xie, P, Yan, B, Yan, X, Yang, J, Yang, Y, Yao, Y, Yu, C, Yuan, Y, Yuan, Z, Zeng, X, Zhang, D, Zhang, M, Zhang, P, Zhang, S, Zhang, S, Zhang, T, Zhang, Y, Zhang, Y, Zhang, Y, Zhao, L, Zheng, Q, Zhou, J, Zhou, N, Zhou, X, Zhou, Y & Zhou, Y 2024, 'Detecting neutrinos from supernova bursts in PandaX-4T', Chinese Physics C, vol. 48, no. 7, 073002. https://doi.org/10.1088/1674-1137/ad3efe

TY - JOUR

T1 - Detecting neutrinos from supernova bursts in PandaX-4T

AU - Pang, Binyu

AU - Abdukerim, Abdusalam

AU - Bo, Zihao

AU - Chen, Wei

AU - Chen, Xun

AU - Cheng, Chen

AU - Cheng, Zhaokan

AU - Cui, Xiangyi

AU - Fan, Yingjie

AU - Fang, Deqing

AU - Fu, Changbo

AU - Fu, Mengting

AU - Geng, Lisheng

AU - Giboni, Karl

AU - Gu, Linhui

AU - Guo, Xuyuan

AU - Han, Chencheng

AU - Han, Ke

AU - He, Changda

AU - He, Jinrong

AU - Huang, Di

AU - Huang, Yanlin

AU - Huang, Junting

AU - Huang, Zhou

AU - Hou, Ruquan

AU - Hou, Yu

AU - Ji, Xiangdong

AU - Ju, Yonglin

AU - Li, Chenxiang

AU - Li, Jiafu

AU - Li, Mingchuan

AU - Li, Shuaijie

AU - Li, Tao

AU - Lin, Qing

AU - Liu, Qi Jianglaing

AU - Lu, Congcong

AU - Lu, Xiaoying

AU - Luo, Lingyin

AU - Luo, Yunyang

AU - Ma, Wenbo

AU - Ma, Yugang

AU - Mao, Yajun

AU - Meng, Yue

AU - Ning, Xuyang

AU - Qi, Ningchun

AU - Qian, Zhicheng

AU - Ren, Xiangxiang

AU - Shaheed, Nasir

AU - Shang, Xiaofeng

AU - Shao, Xiyuan

AU - Shen, Guofang

AU - Si, Lin

AU - Sun, Wenliang

AU - Tan, Andi

AU - Tao, Yi

AU - Wang, Anqing

AU - Wang, Meng

AU - Wang, Qiuhong

AU - Wang, Shaobo

AU - Wang, Siguang

AU - Wang, Wei

AU - Wang, Xiuli

AU - Wang, Zhou

AU - Wei, Yuehuan

AU - Wu, Mengmeng

AU - Wu, Weihao

AU - Xia, Jingkai

AU - Xiao, Mengjiao

AU - Xiao, Xiang

AU - Xie, Pengwei

AU - Yan, Binbin

AU - Yan, Xiyu

AU - Yang, Jijun

AU - Yang, Yong

AU - Yao, Yukun

AU - Yu, Chunxu

AU - Yuan, Ying

AU - Yuan, Zhe

AU - Zeng, Xinning

AU - Zhang, Dan

AU - Zhang, Minzhen

AU - Zhang, Peng

AU - Zhang, Shibo

AU - Zhang, Shu

AU - Zhang, Tao

AU - Zhang, Yang

AU - Zhang, Yingxin

AU - Zhang, Yuanyuan

AU - Zhao, Li

AU - Zheng, Qibin

AU - Zhou, Jifang

AU - Zhou, Ning

AU - Zhou, Xiaopeng

AU - Zhou, Yong

AU - Zhou, Yubo

N1 - Publisher Copyright: © 2024 Chinese Physical Society and the Institute of High Energy Physics of the Chinese Academy of Sciences and the Institute of Modern Physics of the Chinese Academy of Sciences and IOP Publishing Ltd.

PY - 2024/7

Y1 - 2024/7

N2 - Neutrinos from core-collapse supernovae are essential for understanding neutrino physics and stellar evolution. Dual-phase xenon dark matter detectors can be used to track explosions of galactic supernovae by detecting neutrinos through coherent elastic neutrino-nucleus scatterings. In this study, a variation of progenitor masses and explosion models are assumed to predict 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-s 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, which will provide supernova early warnings for the astronomical community.

AB - Neutrinos from core-collapse supernovae are essential for understanding neutrino physics and stellar evolution. Dual-phase xenon dark matter detectors can be used to track explosions of galactic supernovae by detecting neutrinos through coherent elastic neutrino-nucleus scatterings. In this study, a variation of progenitor masses and explosion models are assumed to predict 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-s 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, which will provide supernova early warnings for the astronomical community.

KW - core-collapse supernovae

KW - liquid xenon detectors

KW - neutrinos

KW - supernova early warnings

UR - http://www.scopus.com/inward/record.url?scp=85196153754&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85196153754&partnerID=8YFLogxK

U2 - 10.1088/1674-1137/ad3efe

DO - 10.1088/1674-1137/ad3efe

M3 - Article

AN - SCOPUS:85196153754

SN - 1674-1137

VL - 48

JO - Chinese Physics C

JF - Chinese Physics C

IS - 7

M1 - 073002

ER -

Detecting neutrinos from supernova bursts in PandaX-4T

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All Science Journal Classification (ASJC) codes

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