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@ARTICLE{An:817755,
author = {An, Fengpeng and An, Guangpeng and An, Qi and Antonelli,
Vito and Baussan, Eric and Beacom, John and Bezrukov, Leonid
and Blyth, Simon and Brugnera, Riccardo and Avanzini,
Margherita Buizza and Busto, Jose and Cabrera, Anatael and
Cai, Hao and Cai, Xiao and Cammi, Antonio and Cao, Guofu and
Cao, Jun and Chang, Yun and Chen, Shaomin and Chen, Shenjian
and Chen, Yixue and Chiesa, Davide and Clemenza,
Massimiliano and Clerbaux, Barbara and Conrad, Janet and
D’Angelo, Davide and Kerret, Hervé De and Deng, Zhi and
Deng, Ziyan and Ding, Yayun and Djurcic, Zelimir and Dornic,
Damien and Dracos, Marcos and Drapier, Olivier and Dusini,
Stefano and Dye, Stephen and Enqvist, Timo and Fan, Donghua
and Fang, Jian and Favart, Laurent and Ford, Richard and
Göger-Neff, Marianne and Gan, Haonan and Garfagnini,
Alberto and Giammarchi, Marco and Gonchar, Maxim and Gong,
Guanghua and Gong, Hui and Gonin, Michel and Grassi, Marco
and Grewing, Christian and Guan, Mengyun and Guarino, Vic
and Guo, Gang and Guo, Wanlei and Guo, Xin-Heng and Hagner,
Caren and Han, Ran and He, Miao and Heng, Yuekun and Hsiung,
Yee and Hu, Jun and Hu, Shouyang and Hu, Tao and Huang,
Hanxiong and Huang, Xingtao and Huo, Lei and Ioannisian, Ara
and Jeitler, Manfred and Ji, Xiangdong and Jiang, Xiaoshan
and Jollet, Cécile and Kang, Li and Karagounis, Michael and
Kazarian, Narine and Krumshteyn, Zinovy and Kruth, Andre and
Kuusiniemi, Pasi and Lachenmaier, Tobias and Leitner, Rupert
and Li, Chao and Li, Jiaxing and Li, Weidong and Li, Weiguo
and Li, Xiaomei and Li, Xiaonan and Li, Yi and Li, Yufeng
and Li, Zhi-Bing and Liang, Hao and Lin, Guey-Lin and Lin,
Tao and Lin, Yen-Hsun and Ling, Jiajie and Lippi, Ivano and
Liu, Dawei and Liu, Hongbang and Liu, Hu and Liu, Jianglai
and Liu, Jianli and Liu, Jinchang and Liu, Qian and Liu,
Shubin and Liu, Shulin and Lombardi, Paolo and Long,
Yongbing and Lu, Haoqi and Lu, Jiashu and Lu, Jingbin and
Lu, Junguang and Lubsandorzhiev, Bayarto and Ludhova, Livia
and Luo, Shu and Lyashuk, Vladimir and Möllenberg, Randolph
and Ma, Xubo and Mantovani, Fabio and Mao, Yajun and Mari,
Stefano M and McDonough, William F and Meng, Guang and
Meregaglia, Anselmo and Meroni, Emanuela and Mezzetto, Mauro
and Miramonti, Lino and Mueller, Thomas and Naumov, Dmitry
and Oberauer, Lothar and Ochoa-Ricoux, Juan Pedro and
Olshevskiy, Alexander and Ortica, Fausto and Paoloni,
Alessandro and Peng, Haiping and Peng, Jen-Chieh and
Previtali, Ezio and Qi, Ming and Qian, Sen and Qian, Xin and
Qian, Yongzhong and Qin, Zhonghua and Raffelt, Georg and
Ranucci, Gioacchino and Ricci, Barbara and Robens, Markus
and Romani, Aldo and Ruan, Xiangdong and Ruan, Xichao and
Salamanna, Giuseppe and Shaevitz, Mike and Sinev, Valery and
Sirignano, Chiara and Sisti, Monica and Smirnov, Oleg and
Soiron, Michael and Stahl, Achim and Stanco, Luca and
Steinmann, Jochen and Sun, Xilei and Sun, Yongjie and
Taichenachev, Dmitriy and Tang, Jian and Tkachev, Igor and
Trzaska, Wladyslaw and Waasen, Stefan van and Volpe,
Cristina and Vorobel, Vit and Votano, Lucia and Wang,
Chung-Hsiang and Wang, Guoli and Wang, Hao and Wang, Meng
and Wang, Ruiguang and Wang, Siguang and Wang, Wei and Wang,
Yi and Wang, Yifang and Wang, Zhe and Wang, Zheng and Wang,
Zhigang and Wang, Zhimin and Wei, Wei and Wen, Liangjian and
Wiebusch, Christopher and Wonsak, Björn and Wu, Qun and
Wulz, Claudia-Elisabeth and Wurm, Michael and Xi, Yufei and
Xia, Dongmei and Xie, Yuguang and Xing, Zhi-zhong and Xu,
Jilei and Yan, Baojun and Yang, Changgen and Yang, Chaowen
and Yang, Guang and Yang, Lei and Yang, Yifan and Yao, Yu
and Yegin, Ugur and Yermia, Frédéric and You, Zhengyun and
Yu, Boxiang and Yu, Chunxu and Yu, Zeyuan and Zavatarelli,
Sandra and Zhan, Liang and Zhang, Chao and Zhang, Hong-Hao
and Zhang, Jiawen and Zhang, Jingbo and Zhang, Qingmin and
Zhang, Yu-Mei and Zhang, Zhenyu and Zhao, Zhenghua and
Zheng, Yangheng and Zhong, Weili and Zhou, Guorong and Zhou,
Jing and Zhou, Li and Zhou, Rong and Zhou, Shun and Zhou,
Wenxiong and Zhou, Xiang and Zhou, Yeling and Zhou, Yufeng
and Zou, Jiaheng},
title = {{N}eutrino physics with {JUNO}},
journal = {Journal of physics / G},
volume = {43},
number = {3},
issn = {1361-6471},
address = {Bristol},
publisher = {IOP Publ.},
reportid = {FZJ-2016-04398},
pages = {030401 -},
year = {2016},
abstract = {The Jiangmen Underground Neutrino Observatory (JUNO), a 20
kton multi-purpose underground liquid scintillator detector,
was proposed with the determination of the neutrino mass
hierarchy (MH) as a primary physics goal. The excellent
energy resolution and the large fiducial volume anticipated
for the JUNO detector offer exciting opportunities for
addressing many important topics in neutrino and
astro-particle physics. In this document, we present the
physics motivations and the anticipated performance of the
JUNO detector for various proposed measurements. Following
an introduction summarizing the current status and open
issues in neutrino physics, we discuss how the detection of
antineutrinos generated by a cluster of nuclear power plants
allows the determination of the neutrino MH at a 3–4σ
significance with six years of running of JUNO. The
measurement of antineutrino spectrum with excellent energy
resolution will also lead to the precise determination of
the neutrino oscillation parameters
${\mathrm{sin}}^{2}{\theta }_{12}$, ${\rm{\Delta
}}{m}_{21}^{2}$, and $| {\rm{\Delta }}{m}_{{ee}}^{2}| $ to
an accuracy of better than 1\%, which will play a crucial
role in the future unitarity test of the MNSP matrix. The
JUNO detector is capable of observing not only antineutrinos
from the power plants, but also neutrinos/antineutrinos from
terrestrial and extra-terrestrial sources, including
supernova burst neutrinos, diffuse supernova neutrino
background, geoneutrinos, atmospheric neutrinos, and solar
neutrinos. As a result of JUNO's large size, excellent
energy resolution, and vertex reconstruction capability,
interesting new data on these topics can be collected. For
example, a neutrino burst from a typical core-collapse
supernova at a distance of 10 kpc would lead to ~5000
inverse-beta-decay events and ~2000 all-flavor
neutrino–proton ES events in JUNO, which are of crucial
importance for understanding the mechanism of supernova
explosion and for exploring novel phenomena such as
collective neutrino oscillations. Detection of neutrinos
from all past core-collapse supernova explosions in the
visible universe with JUNO would further provide valuable
information on the cosmic star-formation rate and the
average core-collapse neutrino energy spectrum.
Antineutrinos originating from the radioactive decay of
uranium and thorium in the Earth can be detected in JUNO
with a rate of ~400 events per year, significantly improving
the statistics of existing geoneutrino event samples.
Atmospheric neutrino events collected in JUNO can provide
independent inputs for determining the MH and the octant of
the ${\theta }_{23}$ mixing angle. Detection of the 7Be and
8B solar neutrino events at JUNO would shed new light on the
solar metallicity problem and examine the transition region
between the vacuum and matter dominated neutrino
oscillations. []},
cin = {IKP-2},
ddc = {530},
cid = {I:(DE-Juel1)IKP-2-20111104},
pnm = {612 - Cosmic Matter in the Laboratory (POF3-612)},
pid = {G:(DE-HGF)POF3-612},
typ = {PUB:(DE-HGF)16},
UT = {WOS:000372064200001},
doi = {10.1088/0954-3899/43/3/030401},
url = {https://juser.fz-juelich.de/record/817755},
}
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