Prospects for detecting the diffuse supernova neutrino background with JUNO

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

arxiv（2022）

引用 10|浏览38

暂无评分

摘要

We present the detection potential for the diffuse supernova neutrino background (DSNB) at the Jiangmen Underground Neutrino Observatory (JUNO), using the inverse-beta-decay (IBD) detection channel on free protons. We employ the latest information on the DSNB flux predictions, and investigate in detail the background and its reduction for the DSNB search at JUNO. The atmospheric neutrino induced neutral current (NC) background turns out to be the most critical background, whose uncertainty is carefully evaluated from both the spread of model predictions and an envisaged in situ measurement. We also make a careful study on the background suppression with the pulse shape discrimination (PSD) and triple coincidence (TC) cuts. With latest DSNB signal predictions, more realistic background evaluation and PSD efficiency optimization, and additional TC cut, JUNO can reach the significance of 3 sigma for 3 years of data taking, and achieve better than 5 sigma after 10 years for a reference DSNB model. In the pessimistic scenario of non-observation, JUNO would strongly improve the limits and exclude a significant region of the model parameter space.

查看译文

关键词

diffuse supernova neutrino background,juno

AI 理解论文

溯源树

样例

生成溯源树，研究论文发展脉络

Chat Paper

正在生成论文摘要