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dc.contributor.authorBeacom, John F.en_US
dc.contributor.authorChen, Shaominen_US
dc.contributor.authorCheng, Jianpingen_US
dc.contributor.authorDoustimotlagh, Sayed N.en_US
dc.contributor.authorGao, Yuanningen_US
dc.contributor.authorGong, Guanghuaen_US
dc.contributor.authorGong, Huien_US
dc.contributor.authorGuo, Leien_US
dc.contributor.authorHan, Ranen_US
dc.contributor.authorHe, Hong-Jianen_US
dc.contributor.authorHuang, Xingtaoen_US
dc.contributor.authorLi, Jianminen_US
dc.contributor.authorLi, Jinen_US
dc.contributor.authorLi, Mohanen_US
dc.contributor.authorLi, Xuegianen_US
dc.contributor.authorLiao, Weien_US
dc.contributor.authorLin, Guey-Linen_US
dc.contributor.authorLiu, Zuoweien_US
dc.contributor.authorMcDonough, Williamen_US
dc.contributor.authorSramek, Ondrejen_US
dc.contributor.authorTang, Jianen_US
dc.contributor.authorWan, Linyanen_US
dc.contributor.authorWang, Yuanqingen_US
dc.contributor.authorWang, Zheen_US
dc.contributor.authorWang, Zongyien_US
dc.contributor.authorWei, Hanyuen_US
dc.contributor.authorXi, Yufeien_US
dc.contributor.authorXu, Yeen_US
dc.contributor.authorXu, Xun-Jieen_US
dc.contributor.authorYang, Zhenweien_US
dc.contributor.authorYao, Chunfaen_US
dc.contributor.authorYeh, Minfangen_US
dc.contributor.authorYue, Qianen_US
dc.contributor.authorZhang, Limingen_US
dc.contributor.authorZhang, Yangen_US
dc.contributor.authorZhao, Zhihongen_US
dc.contributor.authorZheng, Yanghengen_US
dc.contributor.authorZhou, Xiangen_US
dc.contributor.authorZhu, Xiangleien_US
dc.contributor.authorZuber, Kaien_US
dc.date.accessioned2019-04-03T06:35:35Z-
dc.date.available2019-04-03T06:35:35Z-
dc.date.issued2017-02-01en_US
dc.identifier.issn1674-1137en_US
dc.identifier.urihttp://dx.doi.org/10.1088/1674-1137/41/2/023002en_US
dc.identifier.urihttp://hdl.handle.net/11536/144608-
dc.description.abstractThe China Jinping Underground Laboratory (CJPL), which has the lowest cosmic-ray muon flux and the lowest reactor neutrino flux of any laboratory, is ideal to carry out low-energy neutrino experiments. With two detectors and a total fiducial mass of 2000 tons for solar neutrino physics (equivalently, 3000 tons for geo-neutrino and supernova neutrino physics), the Jinping neutrino experiment will have the potential to identify the neutrinos from the CNO fusion cycles of the Sun, to cover the transition phase for the solar neutrino oscillation from vacuum to matter mixing, and to measure the geo-neutrino flux, including the Th/U ratio. These goals can be fulfilled with mature existing techniques. Efforts on increasing the target mass with multi-modular neutrino detectors and on developing the slow liquid scintillator will increase the Jinping discovery potential in the study of solar neutrinos, geo-neutrinos, supernova neutrinos, and dark matter.en_US
dc.language.isoen_USen_US
dc.subjectCJPLen_US
dc.subjectJinping neutrino experimenten_US
dc.subjectsolar neutrinoen_US
dc.subjectgeo-neutrinoen_US
dc.subjectsupernova neutrinoen_US
dc.titlePhysics prospects of the Jinping neutrino experimenten_US
dc.typeArticleen_US
dc.identifier.doi10.1088/1674-1137/41/2/023002en_US
dc.identifier.journalCHINESE PHYSICS Cen_US
dc.citation.volume41en_US
dc.citation.issue2en_US
dc.citation.spage0en_US
dc.citation.epage0en_US
dc.contributor.department物理研究所zh_TW
dc.contributor.departmentInstitute of Physicsen_US
dc.identifier.wosnumberWOS:000396641300002en_US
dc.citation.woscount17en_US
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