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Record W4394755235 · doi:10.3847/1538-4357/ad2bfd

Model-independent Approach of the JUNO <sup>8</sup>B Solar Neutrino Program

2024· article· en· W4394755235 on OpenAlexaboutno aff
Bin Yue, Haoqi Lu, Yufeng Li, Jiajie Ling, Zeyuan Yu, Angel Abusleme, Thomas Adam, S. Ahmad, Rizwan Ahmed, S. Aiello, Muhammad Akram, Abid Aleem, Tsagkarakis Alexandros, Fengpeng An, Qi An, Giuseppe Andronico, Н. Анфимов, V. Antonelli, Tatiana Antoshkina, Burin Asavapibhop, J. P. A. M. de André, Didier Auguste, Weidong Bai, Nikita Balashov, W. Baldini, Andrea Barresi, D. Basilico, E. Baussan, Marco Bellato, Antonio Bergnoli, Thilo Birkenfeld, Sylvie Blin, David Blum, S.C. Blyth, Anastasia Bolshakova, M. Bongrand, Clément Bordereau, D. Breton, A. Brigatti, R. Brugnera, Riccardo Bruno, A. Budano, José Busto, Ilya Butorov, J. Busenitz, Barbara Caccianiga, Hao Cai, X. Cai, Yanke Cai, Zhiyan Cai, Riccardo Callegari, Antonio Cammi, Agustín Campeny, Chuanya Cao, Jun Cao, R. Caruso, C. Cerna, Chi Kuen Chan, J. F. Chang, Yun Chang, Guo-Ming Chen, Pingping Chen, Po-An Chen, Shaomin Chen, Xurong Chen, Yixue Chen, Yu Chen, Zhiyuan Chen, Zikang Chen, Jie Cheng, Yaping Cheng, Alexander Chepurnov, Alexey Chetverikov, D. Chiesa, P. Chimenti, A. Chukanov, Gérard Claverie, Catia Clementi, Barbara Clerbaux, Marta Colomer Molla, Selma Conforti Di Lorenzo, Daniele Corti, F. Dal Corso, Olivia Dalager, C. De La Taille, Zhi Deng, Wilfried Depnering, M. A. Díaz, Xuefeng Ding, Yayun Ding, Bayu Dirgantara, Sergey Dmitrievsky, Tadeáš Dohnal, Dmitry Dolzhikov, Georgy Donchenko, J. Dong, E. Doroshkevich, M. Dracos, Frédéric Druillole, Ran Du, Shuxian Du, S. Dusini, Martin Dvořák, T. Enqvist, Heike Enzmann, Andrea Fabbri, Donghua Fan, Lei Fan, J. Fang, Wenxing Fang, Marco Fargetta, Dmitry Fedoseev, Zhengyong Fei, Qichun Feng, R. Ford, Amélie Fournier, Haonan Gan, Feng Gao, A. Garfagnini, Arsenii Gavrikov, Marco Giammarchi, Nunzio Giudice, M. Gonchar, G. Gong, Hui Gong, Y. Gornushkin, Alexandre Göttel, M. Grassi, M. Gromov, Vasily Gromov, M. H. Gu, Xiaofei Gu, Y. T. Gu, Mengyun Guan, Yuduo Guan, Nunzio Guardone, Cong Guo, Jingyuan Guo, Wanlei Guo, Xin‐Heng Guo, Yuhang Guo, Paul Hackspacher, Caren Hagner, Ran Han, Yang Han, Miao He, Wei He, Tobias Heinz, Patrick Hellmuth, Y. K. Heng, R. S. Herrera, YuenKeung Hor, S. Hou, Y. Hsiung, Bei-Zhen Hu, H. Hu, Jianrun Hu, Jun Hu, Shouyang Hu, Tao Hu, Yuxiang Hu, Z. Hu, Guihong Huang, Han‐Xiong Huang, K. X. Huang, Wenhao Huang, X. T. Huang, Xingtao Huang, Yongbo Huang, Jiaqi Hui, Lei Huo, Wenju Huo, Cédric Huss, Safeer Hussain, Ara Ioannisian, R. Isocrate, Beatrice Jelmini, Ignacio Jeria, X. L. Ji, Huihui Jia, Junji Jia, Siyu Jian, Di Jiang, Wei Jiang, Xiaoshan Jiang, Xiaoping Jing, C. Jollet, Leonidas Kalousis, Philipp Kampmann, Kang Li, Rebin Karaparambil, Narine Kazarian, Amina Khatun, Khanchai Khosonthongkee, Denis Korablev, Konstantin Kouzakov, Alexey Krasnoperov, Nikolay Kutovskiy, P. Kuusiniemi, Tobias Lachenmaier, Cecilia Landini, Sébastien Leblanc, Victor Lebrin, F. Lefèvre, Ruiting Lei, R. Leitner, Jason Leung, Daozheng Li, Demin Li, Li Fei, Fule Li, Gaosong Li, Hui-Ling Li, Mengzhao Li, Min Li, Nan Li, Nan Li, Qingjiang Li, Ruhui Li, Rui Li, Shanfeng Li, Tao Li, Teng Li, Weidong Li, Weiguo Li, Xiaomei Li, Xiaonan Li, Xinglong Li, Yi Li, Z. Li, Zhaohan Li, Zhibing Li, Ziyuan Li, Zonghai Li, Hao Liang, Jiajun Liao, A. Limphirat, Guey-Lin Lin, Shengxin Lin, T. Lin, I. Lippi, Fang Liu, Haidong Liu, Haotian Liu, H. Liu, Hongjuan Liu, Hongtao Liu, Hui Liu, Jianglai Liu, Jinchang Liu, Min Liu, Qian Liu, Qin Liu, Runxuan Liu, Shubin Liu, Shulin Liu, Xiaowei Liu, Xiwen Liu, Yan Liu, Yunzhe Liu, Alexey Lokhov, P. Lombardi, Claudio Lombardo, Kai Loo, Chuan Lu, Jingbin Lu, Junguang Lu, Shuxiang Lu, Б. К. Лубсандоржиев, Sultim Lubsandorzhiev, L. Ludhová, Arslan Lukanov, Daibin Luo, Guang Luo, Shu Luo, W. Luo, Xiaojie Luo, Vladimir Lyashuk, Bangzheng Ma, Bing Ma, Qiumei Ma, Si Ma, X. Y. Ma, Xubo Ma, Jihane Maalmi, Jingyu Mai, Yury Malyshkin, Roberto Carlos Mandujano, Fabio Mantovani, Francesco Manzali, Xin Mao, Yajun Mao, Stefano Maria Mari, Filippo Marini, C. Martellini, G. Martin-Chassard, Agnese Martini, Matthias Mayer, Davit Mayilyan, Ints Mednieks, Yue Meng, A. Meregaglia, Emanuela Meroni, David Meyhöfer, M. Mezzetto, J. Miller, L. Miramonti, P. Montini, M. Montuschi, Axel Müller, M. Nastasi, D. Naumov, E. Naumova, D. Navas-Nicolás, I. Nemchenok, Minh Thuan Nguyen Thi, А. Г. Николаев, Feipeng Ning, Zhe Ning, Hiroshi Nunokawa, Lothar Oberauer, J. P. Ochoa‐Ricoux, A. Olshevskiy, Domizia Orestano, F. Ortica, Rainer Othegraven, A. Paoloni, S. Parmeggiano, Yatian Pei, N. Pelliccia, Anguo Peng, Haiping Peng, Yu Peng, Zhaoyuan Peng, F. Perrot, Pierre-Alexandre Petitjean, F. Petrucci, Oliver Pilarczyk, Luis Felipe Piñeres Rico, Artyom Popov, Pascal Poussot, E. Previtali, F. Z. Qi, Ming Qi, S. Qian, Xiaohui Qian, Z. Qian, Hao Qiao, Zhonghua Qin, Shoukang Qiu, G. Ranucci, N. Raper, A. Re, Henning Rebber, Abdel Rebii, M. Redchuk, Bin Ren, Jie Ren, Barbara Ricci, Mariam Rifai, Mathieu Roche, Narongkiat Rodphai, A. Romani, Bedřich Roskovec, Xichao Ruan, Arseniy Rybnikov, Andrey Sadovsky, P. Saggese, S. Sanfilippo, Anut Sangka, Utane Sawangwit, Julia Sawatzki, Michaela Schever, Cédric Schwab, Konstantin Schweizer, Alexandr Selyunin, Andrea Serafini, Giulio Settanta, M. Settimo, Zhuang Shao, Vladislav Sharov, Arina Shaydurova, Jingyan Shi, Yanan Shi, Vitaly Shutov, Andrey Sidorenkov, F. Šimkovic, C. Sirignano, Jaruchit Siripak, M. Sisti, M. Słupecki, Mikhail Smirnov, O. Smirnov, T. J. C. Bezerra, С. В. Соколов, Julanan Songwadhana, Boonrucksar Soonthornthum, A. Sotnikov, Ondřej Šrámek, Warintorn Sreethawong, A. Stahl, L. Stančo, Konstantin Stankevich, Dušan Štefánik, Hans Steiger, Jochen Steinmann, Tobias Sterr, Matthias Raphael Stock, Virginia Strati, Alexander Studenikin, Jun Su, Shifeng Sun, Xilei Sun, Yongjie Sun, Y. K. Sun, Zhengyang Sun, N. Suwonjandee, Michal Szelezniak, J. Tang, Qiang Tang, Quan Tang, X. Tang, Alexander Tietzsch, I. Tkachev, Tomáš Tměj, Marco Danilo Claudio Torri, Konstantin Treskov, Andrea Triossi, Giancarlo Troni, W. H. Trzaska, C. Tuvé, Nikita Ushakov, Vadim Vedin, G. Verde, Maxim Vialkov, Benoit Viaud, Cornelius Moritz Vollbrecht, Cristina Volpe, K. von Sturm, V. Vorobel, Д. Воронин, L. Votano, Pablo Walker, Caishen Wang, Chung-Hsiang Wang, En Wang, Guoli Wang, Jian Wang, Jun Wang, Lu Wang, Meifen Wang, Meng Wang, Ruiguang Wang, Siguang Wang, Wei Wang, Wei Wang, Wenshuai Wang, Xi Wang, Xiangyue Wang, Yangfu Wang, Yaoguang Wang, Yi Wang, Yi Wang, Y. F. Wang, Yuanqing Wang, Yuman Wang, Zhe Wang, Z. Wang, Zhimin Wang, Zongyi Wang, Apimook Watcharangkool, Wei Wei, Wei Wei, Wenlu Wei, Yadong Wei, Kaile Wen, Liangjian Wen, C. H. Wiebusch, Steven Chan-Fai Wong, Bjoern Wonsak, Diru Wu, Qun Wu, Zhi Wu, Jacques Wurtz, Christian Wysotzki, Yufei Xi, Dongmei Xia, Xiang Xiao, Xiaochuan Xie, Yuguang Xie, Zhangquan Xie, Zhi‐zhong Xing, Benda Xu, Cheng Xu, D. L. Xu, Fanrong Xu, Hangkun Xu, Jilei Xu, Jing Xu, M. Xu, Yin Xu, Yu Xu, Baojun Yan, Taylor Yan, Wenqi Yan, Xiongbo Yan, Yupeng Yan, Changgen Yang, Chengfeng Yang, Jie Yang, Lei Yang, Xiaoyu Yang, Y. F. Yang, Yifan Yang, Haifeng Yao, Jiaxuan Ye, Ziping Ye, F. Yermia, Na Yin, Z. You, Boxiang Yu, C. Y. Yu, Chunxu Yu, Hongzhao Yu, Miao Yu, Xianghui Yu, Cenxi Yuan, Ying Yuan, Zhenxiong Yuan, Noman Zafar, Vitalii Zavadskyi, Shan Zeng, Tingxuan Zeng, Yuda Zeng, Liang Zhan, Bin Zhang, Binting Zhang, Feiyang Zhang, Guoqing Zhang, Jialiang Zhang, Jiawen Zhang, Jie Zhang, Jin Zhang, Jingbo Zhang, Jinnan Zhang, Mohan Zhang, Peng Zhang, Qingmin Zhang, Shiqi Zhang, Shu Zhang, Tao Zhang, Xiaomei Zhang, Xin Zhang, Xuantong Zhang, X. Zhang, Yinhong Zhang, Yiyu Zhang, Yongpeng Zhang, Y. Zhang, Yuanyuan Zhang, Yumei Zhang, Zhenyu Zhang, Zhijian Zhang, Fengyi Zhao, Rong Zhao, Runze Zhao, Shujun Zhao, Dongqin Zheng, H. Zheng, Yangheng Zheng, Weirong Zhong, Li Zhou, Nan Zhou, Shun Zhou, Tong Zhou, Xiang Zhou, Jiang Zhu, Jingsen Zhu, Kangfu Zhu, Kejun Zhu, B. A. Zhuang, Honglin Zhuang, Liang Zong, J. H. Zou

Bibliographic record

VenueThe Astrophysical Journal · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicNeutrino Physics Research
Canadian institutionsnot available
FundersInstitut National de Physique Nucléaire et de Physique des ParticulesRussian Science FoundationLomonosov Moscow State UniversityMinistero degli Affari Esteri e della Cooperazione InternazionaleMinistry of Education, IndiaJoint Institute for Nuclear ResearchChulalongkorn UniversityFonds De La Recherche Scientifique - FNRSChinese Academy of SciencesIstituto Nazionale di Fisica NucleareDeutsche ForschungsgemeinschaftNational Natural Science Foundation of ChinaCAS Center for Excellence in Particle PhysicsWuyi UniversityFonds Wetenschappelijk OnderzoekInstitut Català de Nanociència i NanotecnologiaSuranaree University of TechnologyAgencia Nacional de Investigación y DesarrolloUniverzita Karlova v PrazeShanghai Jiao Tong UniversityNational Science Foundation
KeywordsPhysicsNeutrinoAlgorithmNuclear physicsComputer science

Abstract

fetched live from OpenAlex

Abstract The physics potential of detecting 8 B solar neutrinos will be exploited at the Jiangmen Underground Neutrino Observatory (JUNO), in a model-independent manner by using three distinct channels of the charged current (CC), neutral current (NC), and elastic scattering (ES) interactions. Due to the largest-ever mass of 13 C nuclei in the liquid scintillator detectors and the expected low background level, 8 B solar neutrinos are observable in the CC and NC interactions on 13 C for the first time. By virtue of optimized event selections and muon veto strategies, backgrounds from the accidental coincidence, muon-induced isotopes, and external backgrounds can be greatly suppressed. Excellent signal-to-background ratios can be achieved in the CC, NC, and ES channels to guarantee the observation of the 8 B solar neutrinos. From the sensitivity studies performed in this work, we show that JUNO, with 10 yr of data, can reach the 1 σ precision levels of 5%, 8%, and 20% for the 8 B neutrino flux, <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:msup> <mml:mrow> <mml:mi>sin</mml:mi> </mml:mrow> <mml:mrow> <mml:mn>2</mml:mn> </mml:mrow> </mml:msup> <mml:msub> <mml:mrow> <mml:mi>θ</mml:mi> </mml:mrow> <mml:mrow> <mml:mn>12</mml:mn> </mml:mrow> </mml:msub> </mml:math> , and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mi mathvariant="normal">Δ</mml:mi> <mml:msubsup> <mml:mrow> <mml:mi>m</mml:mi> </mml:mrow> <mml:mrow> <mml:mn>21</mml:mn> </mml:mrow> <mml:mrow> <mml:mn>2</mml:mn> </mml:mrow> </mml:msubsup> </mml:math> , respectively. Probing the details of both solar physics and neutrino physics would be unique and helpful. In addition, when combined with the Sudbury Neutrino Observatory measurement, the world's best precision of 3% is expected for the measurement of the 8 B neutrino flux.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.683
Threshold uncertainty score0.850

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0000.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0010.000
Research integrity0.0000.002
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.023
GPT teacher head0.286
Teacher spread0.263 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designSimulation or modeling
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations12
Published2024
Admission routes1
Has abstractyes

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