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| 001 | 817755 | ||
| 005 | 20210129224022.0 | ||
| 024 | 7 | _ | |a 10.1088/0954-3899/43/3/030401 |2 doi |
| 024 | 7 | _ | |a 0305-4616 |2 ISSN |
| 024 | 7 | _ | |a 0954-3899 |2 ISSN |
| 024 | 7 | _ | |a 1361-6471 |2 ISSN |
| 024 | 7 | _ | |a 2128/12216 |2 Handle |
| 024 | 7 | _ | |a WOS:000372064200001 |2 WOS |
| 024 | 7 | _ | |a altmetric:4302485 |2 altmetric |
| 037 | _ | _ | |a FZJ-2016-04398 |
| 082 | _ | _ | |a 530 |
| 100 | 1 | _ | |a An, Fengpeng |0 P:(DE-HGF)0 |b 0 |e Corresponding author |
| 245 | _ | _ | |a Neutrino physics with JUNO |
| 260 | _ | _ | |a Bristol |c 2016 |b IOP Publ. |
| 336 | 7 | _ | |a article |2 DRIVER |
| 336 | 7 | _ | |a Output Types/Journal article |2 DataCite |
| 336 | 7 | _ | |a Journal Article |b journal |m journal |0 PUB:(DE-HGF)16 |s 1472714290_15966 |2 PUB:(DE-HGF) |
| 336 | 7 | _ | |a ARTICLE |2 BibTeX |
| 336 | 7 | _ | |a JOURNAL_ARTICLE |2 ORCID |
| 336 | 7 | _ | |a Journal Article |0 0 |2 EndNote |
| 520 | _ | _ | |a 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. [] |
| 536 | _ | _ | |a 612 - Cosmic Matter in the Laboratory (POF3-612) |0 G:(DE-HGF)POF3-612 |c POF3-612 |f POF III |x 0 |
| 588 | _ | _ | |a Dataset connected to CrossRef |
| 700 | 1 | _ | |a An, Guangpeng |b 1 |
| 700 | 1 | _ | |a An, Qi |b 2 |
| 700 | 1 | _ | |a Antonelli, Vito |b 3 |
| 700 | 1 | _ | |a Baussan, Eric |b 4 |
| 700 | 1 | _ | |a Beacom, John |b 5 |
| 700 | 1 | _ | |a Bezrukov, Leonid |b 6 |
| 700 | 1 | _ | |a Blyth, Simon |b 7 |
| 700 | 1 | _ | |a Brugnera, Riccardo |b 8 |
| 700 | 1 | _ | |a Avanzini, Margherita Buizza |b 9 |
| 700 | 1 | _ | |a Busto, Jose |b 10 |
| 700 | 1 | _ | |a Cabrera, Anatael |b 11 |
| 700 | 1 | _ | |a Cai, Hao |b 12 |
| 700 | 1 | _ | |a Cai, Xiao |b 13 |
| 700 | 1 | _ | |a Cammi, Antonio |b 14 |
| 700 | 1 | _ | |a Cao, Guofu |b 15 |
| 700 | 1 | _ | |a Cao, Jun |b 16 |
| 700 | 1 | _ | |a Chang, Yun |b 17 |
| 700 | 1 | _ | |a Chen, Shaomin |b 18 |
| 700 | 1 | _ | |a Chen, Shenjian |b 19 |
| 700 | 1 | _ | |a Chen, Yixue |b 20 |
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| 700 | 1 | _ | |a Kerret, Hervé De |b 26 |
| 700 | 1 | _ | |a Deng, Zhi |b 27 |
| 700 | 1 | _ | |a Deng, Ziyan |b 28 |
| 700 | 1 | _ | |a Ding, Yayun |b 29 |
| 700 | 1 | _ | |a Djurcic, Zelimir |b 30 |
| 700 | 1 | _ | |a Dornic, Damien |b 31 |
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| 700 | 1 | _ | |a Dusini, Stefano |b 34 |
| 700 | 1 | _ | |a Dye, Stephen |b 35 |
| 700 | 1 | _ | |a Enqvist, Timo |b 36 |
| 700 | 1 | _ | |a Fan, Donghua |b 37 |
| 700 | 1 | _ | |a Fang, Jian |b 38 |
| 700 | 1 | _ | |a Favart, Laurent |b 39 |
| 700 | 1 | _ | |a Ford, Richard |b 40 |
| 700 | 1 | _ | |a Göger-Neff, Marianne |b 41 |
| 700 | 1 | _ | |a Gan, Haonan |b 42 |
| 700 | 1 | _ | |a Garfagnini, Alberto |b 43 |
| 700 | 1 | _ | |a Giammarchi, Marco |b 44 |
| 700 | 1 | _ | |a Gonchar, Maxim |b 45 |
| 700 | 1 | _ | |a Gong, Guanghua |b 46 |
| 700 | 1 | _ | |a Gong, Hui |b 47 |
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| 700 | 1 | _ | |a Grassi, Marco |b 49 |
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| 700 | 1 | _ | |a Guo, Wanlei |b 54 |
| 700 | 1 | _ | |a Guo, Xin-Heng |b 55 |
| 700 | 1 | _ | |a Hagner, Caren |b 56 |
| 700 | 1 | _ | |a Han, Ran |b 57 |
| 700 | 1 | _ | |a He, Miao |b 58 |
| 700 | 1 | _ | |a Heng, Yuekun |b 59 |
| 700 | 1 | _ | |a Hsiung, Yee |b 60 |
| 700 | 1 | _ | |a Hu, Jun |b 61 |
| 700 | 1 | _ | |a Hu, Shouyang |b 62 |
| 700 | 1 | _ | |a Hu, Tao |b 63 |
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| 700 | 1 | _ | |a Huang, Xingtao |b 65 |
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| 700 | 1 | _ | |a Ji, Xiangdong |b 69 |
| 700 | 1 | _ | |a Jiang, Xiaoshan |b 70 |
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| 700 | 1 | _ | |a Li, Chao |b 80 |
| 700 | 1 | _ | |a Li, Jiaxing |b 81 |
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| 773 | _ | _ | |a 10.1088/0954-3899/43/3/030401 |g Vol. 43, no. 3, p. 030401 - |0 PERI:(DE-600)1472964-7 |n 3 |p 030401 - |t Journal of physics / G |v 43 |y 2016 |x 1361-6471 |
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