完整後設資料紀錄
DC 欄位語言
dc.contributor.authorAn, Fengpengen_US
dc.contributor.authorAn, Guangpengen_US
dc.contributor.authorAn, Qien_US
dc.contributor.authorAntonelli, Vitoen_US
dc.contributor.authorBaussan, Ericen_US
dc.contributor.authorBeacom, Johnen_US
dc.contributor.authorBezrukov, Leoniden_US
dc.contributor.authorBlyth, Simonen_US
dc.contributor.authorBrugnera, Riccardoen_US
dc.contributor.authorAvanzini, Margherita Buizzaen_US
dc.contributor.authorBusto, Joseen_US
dc.contributor.authorCabrera, Anataelen_US
dc.contributor.authorCai, Haoen_US
dc.contributor.authorCai, Xiaoen_US
dc.contributor.authorCammi, Antonioen_US
dc.contributor.authorCao, Guofuen_US
dc.contributor.authorCao, Junen_US
dc.contributor.authorChang, Yunen_US
dc.contributor.authorChen, Shaominen_US
dc.contributor.authorChen, Shenjianen_US
dc.contributor.authorChen, Yixueen_US
dc.contributor.authorChiesa, Davideen_US
dc.contributor.authorClemenza, Massimilianoen_US
dc.contributor.authorClerbaux, Barbaraen_US
dc.contributor.authorConrad, Janeten_US
dc.contributor.authorD\'Angelo, Davideen_US
dc.contributor.authorDe Kerret, Herveen_US
dc.contributor.authorDeng, Zhien_US
dc.contributor.authorDeng, Ziyanen_US
dc.contributor.authorDing, Yayunen_US
dc.contributor.authorDjurcic, Zelimiren_US
dc.contributor.authorDornic, Damienen_US
dc.contributor.authorDracos, Marcosen_US
dc.contributor.authorDrapier, Olivieren_US
dc.contributor.authorDusini, Stefanoen_US
dc.contributor.authorDye, Stephenen_US
dc.contributor.authorEnqvist, Timoen_US
dc.contributor.authorFan, Donghuaen_US
dc.contributor.authorFang, Jianen_US
dc.contributor.authorFavart, Laurenten_US
dc.contributor.authorFord, Richarden_US
dc.contributor.authorGoeger-Neff, Marianneen_US
dc.contributor.authorGan, Haonanen_US
dc.contributor.authorGarfagnini, Albertoen_US
dc.contributor.authorGiammarchi, Marcoen_US
dc.contributor.authorGonchar, Maximen_US
dc.contributor.authorGong, Guanghuaen_US
dc.contributor.authorGong, Huien_US
dc.contributor.authorGonin, Michelen_US
dc.contributor.authorGrassi, Marcoen_US
dc.contributor.authorGrewing, Christianen_US
dc.contributor.authorGuan, Mengyunen_US
dc.contributor.authorGuarino, Vicen_US
dc.contributor.authorGuo, Gangen_US
dc.contributor.authorGuo, Wanleien_US
dc.contributor.authorGuo, Xin-Hengen_US
dc.contributor.authorHagner, Carenen_US
dc.contributor.authorHan, Ranen_US
dc.contributor.authorHe, Miaoen_US
dc.contributor.authorHeng, Yuekunen_US
dc.contributor.authorHsiung, Yeeen_US
dc.contributor.authorHu, Junen_US
dc.contributor.authorHu, Shouyangen_US
dc.contributor.authorHu, Taoen_US
dc.contributor.authorHuang, Hanxiongen_US
dc.contributor.authorHuang, Xingtaoen_US
dc.contributor.authorHuo, Leien_US
dc.contributor.authorIoannisian, Araen_US
dc.contributor.authorJeitler, Manfreden_US
dc.contributor.authorJi, Xiangdongen_US
dc.contributor.authorJiang, Xiaoshanen_US
dc.contributor.authorJollet, Cecileen_US
dc.contributor.authorKang, Lien_US
dc.contributor.authorKaragounis, Michaelen_US
dc.contributor.authorKazarian, Narineen_US
dc.contributor.authorKrumshteyn, Zinovyen_US
dc.contributor.authorKruth, Andreen_US
dc.contributor.authorKuusiniemi, Pasien_US
dc.contributor.authorLachenmaier, Tobiasen_US
dc.contributor.authorLeitner, Ruperten_US
dc.contributor.authorLi, Chaoen_US
dc.contributor.authorLi, Jiaxingen_US
dc.contributor.authorLi, Weidongen_US
dc.contributor.authorLi, Weiguoen_US
dc.contributor.authorLi, Xiaomeien_US
dc.contributor.authorLi, Xiaonanen_US
dc.contributor.authorLi, Yien_US
dc.contributor.authorLi, Yufengen_US
dc.contributor.authorLi, Zhi-Bingen_US
dc.contributor.authorLiang, Haoen_US
dc.contributor.authorLin, Guey-Linen_US
dc.contributor.authorLin, Taoen_US
dc.contributor.authorLin, Yen-Hsunen_US
dc.contributor.authorLing, Jiajieen_US
dc.contributor.authorLippi, Ivanoen_US
dc.contributor.authorLiu, Daweien_US
dc.contributor.authorLiu, Hongbangen_US
dc.contributor.authorLiu, Huen_US
dc.contributor.authorLiu, Jianglaien_US
dc.contributor.authorLiu, Jianlien_US
dc.contributor.authorLiu, Jinchangen_US
dc.contributor.authorLiu, Qianen_US
dc.contributor.authorLiu, Shubinen_US
dc.contributor.authorLiu, Shulinen_US
dc.contributor.authorLombardi, Paoloen_US
dc.contributor.authorLong, Yongbingen_US
dc.contributor.authorLu, Haoqien_US
dc.contributor.authorLu, Jiashuen_US
dc.contributor.authorLu, Jingbinen_US
dc.contributor.authorLu, Junguangen_US
dc.contributor.authorLubsandorzhiev, Bayartoen_US
dc.contributor.authorLudhova, Liviaen_US
dc.contributor.authorLuo, Shuen_US
dc.contributor.authorLyashuk, Vladimiren_US
dc.contributor.authorMoellenberg, Randolphen_US
dc.contributor.authorMa, Xuboen_US
dc.contributor.authorMantovani, Fabioen_US
dc.contributor.authorMao, Yajunen_US
dc.contributor.authorMari, Stefano M.en_US
dc.contributor.authorMcDonough, William F.en_US
dc.contributor.authorMeng, Guangen_US
dc.contributor.authorMeregaglia, Anselmoen_US
dc.contributor.authorMeroni, Emanuelaen_US
dc.contributor.authorMezzetto, Mauroen_US
dc.contributor.authorMiramonti, Linoen_US
dc.contributor.authorMueller, Thomasen_US
dc.contributor.authorNaumov, Dmitryen_US
dc.contributor.authorOberauer, Lotharen_US
dc.contributor.authorOchoa-Ricoux, Juan Pedroen_US
dc.contributor.authorOlshevskiy, Alexanderen_US
dc.contributor.authorOrtica, Faustoen_US
dc.contributor.authorPaoloni, Alessandroen_US
dc.contributor.authorPeng, Haipingen_US
dc.contributor.authorPeng, Jen-Chiehen_US
dc.contributor.authorPrevitali, Ezioen_US
dc.contributor.authorQi, Mingen_US
dc.contributor.authorQian, Senen_US
dc.contributor.authorQian, Xinen_US
dc.contributor.authorQian, Yongzhongen_US
dc.contributor.authorQin, Zhonghuaen_US
dc.contributor.authorRaffelt, Georgen_US
dc.contributor.authorRanucci, Gioacchinoen_US
dc.contributor.authorRicci, Barbaraen_US
dc.contributor.authorRobens, Markusen_US
dc.contributor.authorRomani, Aldoen_US
dc.contributor.authorRuan, Xiangdongen_US
dc.contributor.authorRuan, Xichaoen_US
dc.contributor.authorSalamanna, Giuseppeen_US
dc.contributor.authorShaevitz, Mikeen_US
dc.contributor.authorSinev, Valeryen_US
dc.contributor.authorSirignano, Chiaraen_US
dc.contributor.authorSisti, Monicaen_US
dc.contributor.authorSmirnov, Olegen_US
dc.contributor.authorSoiron, Michaelen_US
dc.contributor.authorStahl, Achimen_US
dc.contributor.authorStanco, Lucaen_US
dc.contributor.authorSteinmann, Jochenen_US
dc.contributor.authorSun, Xileien_US
dc.contributor.authorSun, Yongjieen_US
dc.contributor.authorTaichenachev, Dmitriyen_US
dc.contributor.authorTang, Jianen_US
dc.contributor.authorTkachev, Igoren_US
dc.contributor.authorTrzaska, Wladyslawen_US
dc.contributor.authorVan Waasen, Stefanen_US
dc.contributor.authorVolpe, Cristinaen_US
dc.contributor.authorVorobel, Viten_US
dc.contributor.authorVotano, Luciaen_US
dc.contributor.authorWang, Chung-Hsiangen_US
dc.contributor.authorWang, Guolien_US
dc.contributor.authorWang, Haoen_US
dc.contributor.authorWang, Mengen_US
dc.contributor.authorWang, Ruiguangen_US
dc.contributor.authorWang, Siguangen_US
dc.contributor.authorWang, Weien_US
dc.contributor.authorWang, Yien_US
dc.contributor.authorWang, Yien_US
dc.contributor.authorWang, Yifangen_US
dc.contributor.authorWang, Zheen_US
dc.contributor.authorWang, Zhengen_US
dc.contributor.authorWang, Zhigangen_US
dc.contributor.authorWang, Zhiminen_US
dc.contributor.authorWei, Weien_US
dc.contributor.authorWen, Liangjianen_US
dc.contributor.authorWiebusch, Christopheren_US
dc.contributor.authorWonsak, Bjoernen_US
dc.contributor.authorWu, Qunen_US
dc.contributor.authorWulz, Claudia-Elisabethen_US
dc.contributor.authorWurm, Michaelen_US
dc.contributor.authorXi, Yufeien_US
dc.contributor.authorXia, Dongmeien_US
dc.contributor.authorXie, Yuguangen_US
dc.contributor.authorXing, Zhi-Zhongen_US
dc.contributor.authorXu, Jileien_US
dc.contributor.authorYan, Baojunen_US
dc.contributor.authorYang, Changgenen_US
dc.contributor.authorYang, Chaowenen_US
dc.contributor.authorYang, Guangen_US
dc.contributor.authorYang, Leien_US
dc.contributor.authorYang, Yifanen_US
dc.contributor.authorYao, Yuen_US
dc.contributor.authorYegin, Uguren_US
dc.contributor.authorYermia, Fredericen_US
dc.contributor.authorYou, Zhengyunen_US
dc.contributor.authorYu, Boxiangen_US
dc.contributor.authorYu, Chunxuen_US
dc.contributor.authorYu, Zeyuanen_US
dc.contributor.authorZavatarelli, Sandraen_US
dc.contributor.authorZhan, Liangen_US
dc.contributor.authorZhang, Chaoen_US
dc.contributor.authorZhang, Hong-Haoen_US
dc.contributor.authorZhang, Jiawenen_US
dc.contributor.authorZhang, Jingboen_US
dc.contributor.authorZhang, Qingminen_US
dc.contributor.authorZhang, Yu-Meien_US
dc.contributor.authorZhang, Zhenyuen_US
dc.contributor.authorZhao, Zhenghuaen_US
dc.contributor.authorZheng, Yanghengen_US
dc.contributor.authorZhong, Weilien_US
dc.contributor.authorZhou, Guorongen_US
dc.contributor.authorZhou, Jingen_US
dc.contributor.authorZhou, Lien_US
dc.contributor.authorZhou, Rongen_US
dc.contributor.authorZhou, Shunen_US
dc.contributor.authorZhou, Wenxiongen_US
dc.contributor.authorZhou, Xiangen_US
dc.contributor.authorZhou, Yelingen_US
dc.contributor.authorZhou, Yufengen_US
dc.contributor.authorZou, Jiahengen_US
dc.date.accessioned2017-04-21T06:56:07Z-
dc.date.available2017-04-21T06:56:07Z-
dc.date.issued2016-03en_US
dc.identifier.issn0954-3899en_US
dc.identifier.urihttp://dx.doi.org/10.1088/0954-3899/43/3/030401en_US
dc.identifier.urihttp://hdl.handle.net/11536/133518-
dc.description.abstractThe Jiangmen Underground Neutrino Observatory (JUNO), a 20 kton multipurpose 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 3-4 sigma 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 sin(2) theta(12), Delta m(21)(2), and vertical bar Delta m(ee)(2)vertical bar 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 similar to 5000 inverse-beta-decay events and similar to 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 similar to 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 Be-7 and B-8 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. Regarding light sterile neutrino topics, sterile neutrinos with 10-(5) eV(2) < Delta m(41)(2) < 10(-2) and a sufficiently large mixing angle theta(14) could be identified through a precise measurement of the reactor antineutrino energy spectrum. Meanwhile, JUNO can also provide us excellent opportunities to test the eV-scale sterile neutrino hypothesis, using either the radioactive neutrino sources or a cyclotron-produced neutrino beam. The JUNO detector is also sensitive to several other beyondthe-standard-model physics. Examples include the search for proton decay via the p -> K++ <(v)over bar> decay channel, search for neutrinos resulting from dark-matter annihilation in the Sun, search for violation of Lorentz invariance via the sidereal modulation of the reactor neutrino event rate, and search for the effects of non-standard interactions. The proposed construction of the JUNO detector will provide a unique facility to address many outstanding crucial questions in particle and astrophysics in a timely and cost-effective fashion. It holds the great potential for further advancing our quest to understanding the fundamental properties of neutrinos, one of the building blocks of our Universe.en_US
dc.language.isoen_USen_US
dc.subjectreactor neutrino experimentsen_US
dc.subjectlarge scintillator detectorsen_US
dc.subjectneutrino physicsen_US
dc.subjectneutrino astronomyen_US
dc.titleNeutrino physics with JUNOen_US
dc.identifier.doi10.1088/0954-3899/43/3/030401en_US
dc.identifier.journalJOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICSen_US
dc.citation.volume43en_US
dc.citation.issue3en_US
dc.contributor.department物理研究所zh_TW
dc.contributor.departmentInstitute of Physicsen_US
dc.identifier.wosnumberWOS:000372064200001en_US
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