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Published byWendy Owens Modified over 9 years ago
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CurrentYufengXin sin 2 2θ 12 4%0.7%0.5% Δm 2 21 3%0.6%0.4% Δm 2 32 3%0.4%0.3% Impacts on neutrinoless beta decay, future unitarity tests of PMNS matrix, test models of neutrino masses and mixing …
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20 kT liquid scintillator detector deep underground Acrylic tank : 34.5m Stainless Steel tank : 37.5m <3% energy resolution @ 1 MeV ~ 80% photon coverage, 700 m rock burden Civil construction 2014-2017 Detector component production 2016-2017 PMT production 2016-2019 Detector installation 2018-2019 Filling and data taking 2020
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Yangjiang NPP Taishan NPP Daya Bay NPP Huizhou NPP Lufeng NPP 53 km Hong Kong Macau Guang Zhou Shen Zhen Zhu Hai 700 m underground 2.5 h drive NPPDaya BayHuizhouLufengYangjiang Taishan StatusOperationalPlanned Under construction Power17.4 GW 18.4 GW
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Additional Physics Topics Supernova neutrinos – Mass of neutrinos through time of flight – Sensitive to both anti-nu_e (IBD) and NC channel – Relic Supernova neutrinos Proton decay (K^+ channel) Geoneutrinos + Solar …
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Calibration of JUNO detector Important to reach 3% @ 1 MeV energy resolution Important to reach sub-1% absolute energy scale Calibrate the PMT timing pulse-shape discrimination ability of JUNO Synergies with DYB/PROSPECT: – Energy model is important to extract neutrino spectrum crucial for JUNO, as no near detector Ideas: positron sources, B12, diffused beta or positron sources, neutron sources, electron/positron pelletrons … Also high performance LS R&D …
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