Model-independent Approach of the JUNO 8B Solar Neutrino Program

Author:

Zhao Jie,Yue Baobiao,Lu Haoqi,Li Yufeng,Ling Jiajie,Yu Zeyuan,Abusleme Angel,Adam Thomas,Ahmad Shakeel,Ahmed Rizwan,Aiello Sebastiano,Akram Muhammad,Aleem Abid,Alexandros Tsagkarakis,An Fengpeng,An Qi,Andronico Giuseppe,Anfimov Nikolay,Antonelli Vito,Antoshkina Tatiana,Asavapibhop Burin,Athayde Marcondes de André João Pedro,Auguste Didier,Bai Weidong,Balashov Nikita,Baldini Wander,Barresi Andrea,Basilico Davide,Baussan Eric,Bellato Marco,Bergnoli Antonio,Birkenfeld Thilo,Blin Sylvie,Blum David,Blyth Simon,Bolshakova Anastasia,Bongrand Mathieu,Bordereau Clément,Breton Dominique,Brigatti Augusto,Brugnera Riccardo,Bruno Riccardo,Budano Antonio,Busto Jose,Butorov Ilya,Cabrera Anatael,Caccianiga Barbara,Cai Hao,Cai Xiao,Cai Yanke,Cai Zhiyan,Callegari Riccardo,Cammi Antonio,Campeny Agustin,Cao Chuanya,Cao Guofu,Cao Jun,Caruso Rossella,Cerna Cédric,Chan Chi,Chang Jinfan,Chang Yun,Chen Guoming,Chen Pingping,Chen Po-An,Chen Shaomin,Chen Xurong,Chen Yixue,Chen Yu,Chen Zhiyuan,Chen Zikang,Cheng Jie,Cheng Yaping,Chepurnov Alexander,Chetverikov Alexey,Chiesa Davide,Chimenti Pietro,Chukanov Artem,Claverie Gérard,Clementi Catia,Clerbaux Barbara,Colomer Molla Marta,Conforti Di Lorenzo Selma,Corti Daniele,Dal Corso Flavio,Dalager Olivia,De La Taille Christophe,Deng Zhi,Deng Ziyan,Depnering Wilfried,Diaz Marco,Ding Xuefeng,Ding Yayun,Dirgantara Bayu,Dmitrievsky Sergey,Dohnal Tadeas,Dolzhikov Dmitry,Donchenko Georgy,Dong Jianmeng,Doroshkevich Evgeny,Dracos Marcos,Druillole Frédéric,Du Ran,Du Shuxian,Dusini Stefano,Dvorak Martin,Enqvist Timo,Enzmann Heike,Fabbri Andrea,Fan Donghua,Fan Lei,Fang Jian,Fang Wenxing,Fargetta Marco,Fedoseev Dmitry,Fei Zhengyong,Feng Li-Cheng,Feng Qichun,Ford Richard,Fournier Amélie,Gan Haonan,Gao Feng,Garfagnini Alberto,Gavrikov Arsenii,Giammarchi Marco,Giudice Nunzio,Gonchar Maxim,Gong Guanghua,Gong Hui,Gornushkin Yuri,Göttel Alexandre,Grassi Marco,Gromov Maxim,Gromov Vasily,Gu Minghao,Gu Xiaofei,Gu Yu,Guan Mengyun,Guan Yuduo,Guardone Nunzio,Guo Cong,Guo Jingyuan,Guo Wanlei,Guo Xinheng,Guo Yuhang,Hackspacher Paul,Hagner Caren,Han Ran,Han Yang,He Miao,He Wei,Heinz Tobias,Hellmuth Patrick,Heng Yuekun,Herrera Rafael,Hor YuenKeung,Hou Shaojing,Hsiung Yee,Hu Bei-Zhen,Hu Hang,Hu Jianrun,Hu Jun,Hu Shouyang,Hu Tao,Hu Yuxiang,Hu Zhuojun,Huang Guihong,Huang Hanxiong,Huang Kaixuan,Huang Wenhao,Huang Xin,Huang Xingtao,Huang Yongbo,Hui Jiaqi,Huo Lei,Huo Wenju,Huss Cédric,Hussain Safeer,Ioannisian Ara,Isocrate Roberto,Jelmini Beatrice,Jeria Ignacio,Ji Xiaolu,Jia Huihui,Jia Junji,Jian Siyu,Jiang Di,Jiang Wei,Jiang Xiaoshan,Jing Xiaoping,Jollet Cécile,Kalousis Leonidas,Kampmann Philipp,Kang Li,Karaparambil Rebin,Kazarian Narine,Khatun Amina,Khosonthongkee Khanchai,Korablev Denis,Kouzakov Konstantin,Krasnoperov Alexey,Kutovskiy Nikolay,Kuusiniemi Pasi,Lachenmaier Tobias,Landini Cecilia,Leblanc Sébastien,Lebrin Victor,Lefevre Frederic,Lei Ruiting,Leitner Rupert,Leung Jason,Li Daozheng,Li Demin,Li Fei,Li Fule,Li Gaosong,Li Huiling,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 Yichen,Li Zepeng,Li Zhaohan,Li Zhibing,Li Ziyuan,Li Zonghai,Liang Hao,Liang Hao,Liao Jiajun,Limphirat Ayut,Lin Guey-Lin,Lin Shengxin,Lin Tao,Lippi Ivano,Liu Fang,Liu Haidong,Liu Haotian,Liu Hongbang,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,Lokhov Alexey,Lombardi Paolo,Lombardo Claudio,Loo Kai,Lu Chuan,Lu Jingbin,Lu Junguang,Lu Shuxiang,Lubsandorzhiev Bayarto,Lubsandorzhiev Sultim,Ludhova Livia,Lukanov Arslan,Luo Daibin,Luo Fengjiao,Luo Guang,Luo Shu,Luo Wuming,Luo Xiaojie,Lyashuk Vladimir,Ma Bangzheng,Ma Bing,Ma Qiumei,Ma Si,Ma Xiaoyan,Ma Xubo,Maalmi Jihane,Mai Jingyu,Malyshkin Yury,Mandujano Roberto Carlos,Mantovani Fabio,Manzali Francesco,Mao Xin,Mao Yajun,Mari Stefano M.,Marini Filippo,Martellini Cristina,Martin-Chassard Gisele,Martini Agnese,Mayer Matthias,Mayilyan Davit,Mednieks Ints,Meng Yue,Meregaglia Anselmo,Meroni Emanuela,Meyhöfer David,Mezzetto Mauro,Miller Jonathan,Miramonti Lino,Montini Paolo,Montuschi Michele,Müller Axel,Nastasi Massimiliano,Naumov Dmitry V.,Naumova Elena,Navas-Nicolas Diana,Nemchenok Igor,Nguyen Thi Minh Thuan,Nikolaev Alexey,Ning Feipeng,Ning Zhe,Nunokawa Hiroshi,Oberauer Lothar,Ochoa-Ricoux Juan Pedro,Olshevskiy Alexander,Orestano Domizia,Ortica Fausto,Othegraven Rainer,Paoloni Alessandro,Parmeggiano Sergio,Pei Yatian,Pelliccia Nicomede,Peng Anguo,Peng Haiping,Peng Yu,Peng Zhaoyuan,Perrot Frédéric,Petitjean Pierre-Alexandre,Petrucci Fabrizio,Pilarczyk Oliver,Piñeres Rico Luis Felipe,Popov Artyom,Poussot Pascal,Previtali Ezio,Qi Fazhi,Qi Ming,Qian Sen,Qian Xiaohui,Qian Zhen,Qiao Hao,Qin Zhonghua,Qiu Shoukang,Ranucci Gioacchino,Raper Neill,Re Alessandra,Rebber Henning,Rebii Abdel,Redchuk Mariia,Redchuk Mariia,Ren Bin,Ren Jie,Ricci Barbara,Rifai Mariam,Roche Mathieu,Rodphai Narongkiat,Romani Aldo,Roskovec Bedřich,Ruan Xichao,Rybnikov Arseniy,Sadovsky Andrey,Saggese Paolo,Sanfilippo Simone,Sangka Anut,Sawangwit Utane,Sawatzki Julia,Schever Michaela,Schwab Cédric,Schweizer Konstantin,Selyunin Alexandr,Serafini Andrea,Settanta Giulio,Settimo Mariangela,Shao Zhuang,Sharov Vladislav,Shaydurova Arina,Shi Jingyan,Shi Yanan,Shutov Vitaly,Sidorenkov Andrey,Šimkovic Fedor,Sirignano Chiara,Siripak Jaruchit,Sisti Monica,Slupecki Maciej,Smirnov Mikhail,Smirnov Oleg,Sogo-Bezerra Thiago,Sokolov Sergey,Songwadhana Julanan,Soonthornthum Boonrucksar,Sotnikov Albert,Šrámek Ondřej,Sreethawong Warintorn,Stahl Achim,Stanco Luca,Stankevich Konstantin,Štefánik Dušan,Steiger Hans,Steinmann Jochen,Sterr Tobias,Stock Matthias Raphael,Strati Virginia,Studenikin Alexander,Su Jun,Sun Shifeng,Sun Xilei,Sun Yongjie,Sun Yongzhao,Sun Zhengyang,Suwonjandee Narumon,Szelezniak Michal,Tang Jian,Tang Qiang,Tang Quan,Tang Xiao,Tietzsch Alexander,Tkachev Igor,Tmej Tomas,Torri Marco Danilo Claudio,Treskov Konstantin,Triossi Andrea,Troni Giancarlo,Trzaska Wladyslaw,Tuve Cristina,Ushakov Nikita,Vedin Vadim,Verde Giuseppe,Vialkov Maxim,Viaud Benoit,Vollbrecht Cornelius Moritz,Volpe Cristina,von Sturm Katharina,Vorobel Vit,Voronin Dmitriy,Votano Lucia,Walker Pablo,Wang Caishen,Wang Chung-Hsiang,Wang En,Wang Guoli,Wang Jian,Wang Jun,Wang Lu,Wang Meifen,Wang Meng,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 Yifang,Wang Yuanqing,Wang Yuman,Wang Zhe,Wang Zheng,Wang Zhimin,Wang Zongyi,Watcharangkool Apimook,Wei Wei,Wei Wei,Wei Wenlu,Wei Yadong,Wen Kaile,Wen Liangjian,Wiebusch Christopher,Wong Steven Chan-Fai,Wonsak Bjoern,Wu Diru,Wu Qun,Wu Zhi,Wurm Michael,Wurtz Jacques,Wysotzki Christian,Xi Yufei,Xia Dongmei,Xiao Xiang,Xie Xiaochuan,Xie Yuguang,Xie Zhangquan,Xin Zhao,Xing Zhizhong,Xu Benda,Xu Cheng,Xu Donglian,Xu Fanrong,Xu Hangkun,Xu Jilei,Xu Jing,Xu Meihang,Xu Yin,Xu Yu,Yan Baojun,Yan Taylor,Yan Wenqi,Yan Xiongbo,Yan Yupeng,Yang Changgen,Yang Chengfeng,Yang Huan,Yang Jie,Yang Lei,Yang Xiaoyu,Yang Yifan,Yang Yifan,Yao Haifeng,Ye Jiaxuan,Ye Mei,Ye Ziping,Yermia Frédéric,Yin Na,You Zhengyun,Yu Boxiang,Yu Chiye,Yu Chunxu,Yu Hongzhao,Yu Miao,Yu Xianghui,Yu Zezhong,Yuan Cenxi,Yuan Chengzhuo,Yuan Ying,Yuan Zhenxiong,Zafar Noman,Zavadskyi Vitalii,Zeng Shan,Zeng Tingxuan,Zeng Yuda,Zhan Liang,Zhang Aiqiang,Zhang Bin,Zhang Binting,Zhang Feiyang,Zhang Guoqing,Zhang Honghao,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 Xueyao,Zhang Yinhong,Zhang Yiyu,Zhang Yongpeng,Zhang Yu,Zhang Yuanyuan,Zhang Yumei,Zhang Zhenyu,Zhang Zhijian,Zhao Fengyi,Zhao Rong,Zhao Runze,Zhao Shujun,Zheng Dongqin,Zheng Hua,Zheng Yangheng,Zhong Weirong,Zhou Jing,Zhou Li,Zhou Nan,Zhou Shun,Zhou Tong,Zhou Xiang,Zhu Jiang,Zhu Jingsen,Zhu Kangfu,Zhu Kejun,Zhu Zhihang,Zhuang Bo,Zhuang Honglin,Zong Liang,Zou Jiaheng

Abstract

Abstract The physics potential of detecting 8B 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 13C nuclei in the liquid scintillator detectors and the expected low background level, 8B solar neutrinos are observable in the CC and NC interactions on 13C 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 8B solar neutrinos. From the sensitivity studies performed in this work, we show that JUNO, with 10 yr of data, can reach the 1σ precision levels of 5%, 8%, and 20% for the 8B neutrino flux, sin 2 θ 12 , and Δ m 21 2 , 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 8B neutrino flux.

Publisher

American Astronomical Society

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