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Physics prospects of the Jinping neutrino experiment

Physics prospects of the Jinping neutrino experiment
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摘要 The 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. The 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.
出处 《Chinese Physics C》 SCIE CAS CSCD 2017年第2期9-32,共24页 中国物理C(英文版)
基金 Supported by the National Natural Science Foundation of China(11235006,11475093,11135009,11375065,11505301,and11620101004) the Tsinghua University Initiative Scientific Research Program(20121088035,20131089288,and 20151080432) the Key Laboratory of Particle&Radiation Imaging(Tsinghua University) the CAS Center for Excellence in Particle Physics(CCEPP) U.S.National Science Foundation Grant PHY-1404311(Beacom) U.S.Department of Energy under contract DE-AC02-98CH10886(Yeh)
关键词 中微子通量 实验物理 太阳中微子 超新星中微子 中微子探测器 地下实验室 中微子实验 展望 CJPL Jinping neutrino experiment solar neutrino geo-neutrino supernova neutrino
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  • 1安丰鹏,A.B.Balantekin,H.R.Band,M.Bishai,S.Blyth,曹德文,曹国富,曹俊,岑吴镕,陳日朗,常劲帆,張立楚,张昀,陈和生,陈泉佑,陈少敏,陈义学,陈羽,程佳樺,程捷,程雅苹,成兆侃,J.J.Cherwinka,朱明中,A.Chukanov,J.P.Cummings,J.de Arcos,邓子艳,丁雪峰,丁雅韵,M.V.Diwan,M.Dolgareva,J.Dove,D.A.Dwyer,W.R.Edwards,R.Gill,M.Gonchar,龚光华,宫辉,M.Grassi,顾文强,关梦云,郭磊,郭如盼,郭新恒,郭子溢,R.W.Hackenburg,韩然,S.Hans,何苗,K.M.Heeger,衡月昆,A.Higuera,Y.K.Hor,熊怡,胡貝禎,胡涛,胡维,黄恩泉,黄翰雄,黄性涛,P.Huber,霍文驹,G.Hussain,D.E.Jaffe,P.Jaffke,任國綸,S.Jetter,季向盼,季筱璐,焦健斌,R.A.Johnson,D.Jones,J.Joshi,康丽,S.H.Kettell,S.Kohn,M.Kramer,關健强,郭文伟,郭天能,T.J.Langford,K.Lau,L.Lebanowski,J.Lee,李曉菁,雷瑞庭,R.Leitner,李超,李登杰,李飞,李高嵩,李秋菊,黎山峰,S.C.Li,李卫东,李小男,李玉峰,李志兵,梁昊,林政儒,林贵林,林盛鑫,林士凱,林禹丞,凌家杰,J.M.Link,L.Littenberg,B.R.Littlejohn,刘大为,刘江来,刘金昌,C.W.Loh,陆昌国,路浩奇,陆稼书,陆锦标,吕志鹏,马秋梅,马晓妍,马续波,马宇倩,Y.Malyshkin,D.A.Martinez Caicedo,K.T.McDonald,R.D.McKeown,I.Mitchell,M.Mooney,Y.Nakajima,J.Napolitano,D.Naumov,E.Naumova,倪浩然,宁哲,J.P.Ochoa-Ricoux,A.Olshevskiy,潘孝儒,J.Park,S.Patton,V.Pec,彭仁杰,L.Pinsky,潘振声,齐法制,祁鸣,钱鑫,N.Raper,任杰,R.Rosero,B.Roskovec,阮锡超,H.Steiner,孙功星,孙吉良,唐炜,D.Taychenachev,K.TVeskov,K.V.Tsang,C.E.Tull,N.Viaux,B.Viren,V.Vorobei,王正祥,王萌,王乃彦,王瑞光,王为,王玺,王贻芳,王喆,王铮,王志民,魏瀚宇,温良剑,K.Whisnant,C.G.White,L.Whitehead,T.Wise,黄显诺,黄振辉,E.Worcester,吳珈豪,吴群,吴文杰,夏冬梅,夏经凯,邢志忠,徐建一,徐吉磊,徐晔,薛涛,杨长根,杨海波,杨雷,阳马生,杨梦婷,叶梅,Z.Ye,叶铭芳,杨炳麟,于泽源,曾珊,占亮,张超,张宏浩,张家文,张清民,张玄同,张一鸣,张一心,张玉美,张志坚,张智勇,张子平,赵洁,赵庆旺,赵豫斌,钟玮丽,周莉,N.Zhou,庄红林,邹佳恒.Improved measurement of the reactor antineutrino flux and spectrum at Daya Bay[J].Chinese Physics C,2017,41(1):11-46.
  • 2王江红.日本建造世界最大的中微子探测器[J].高能物理参考资料,1993(6):19-20.
  • 3杨大卫.太阳中微子通量的估算[J].现代物理知识,1998,10(4):34-35.
  • 4奇云.冰立方——深藏南极冰下的中微子探测器[J].科学24小时,2011(9):53-55.
  • 5张一纯,陈晓苏,何苗,黄性涛,王萌,李卫东,张子平.Mixing MC events in a reactor neutrino experiment[J].Chinese Physics C,2013,37(1):86-90.
  • 6黄明阳,郭新恒,杨炳麟.Detection of supernova neutrinos at spallation neutron sources[J].Chinese Physics C,2016,40(7):15-21.
  • 7郭新恒,黄明阳,杨炳麟.Supernova neutrino detection on earth[J].Chinese Physics C,2010,34(2):257-261.
  • 8CHEN XiaoHui,LUO XiaoLan,HENG YueKun,WANG LingShu,TANG Xiao,MA XiaoYan,ZHUANG HongLin,BAND Henry R.,CHERWINKA Jeff J.,XIAO Qiang,HEEGER Karsten M..Leakage tests of the stainless steel vessels of the antineutrino detectors in the Daya Bay reactor neutrino experiment[J].Science China(Technological Sciences),2013,56(1):148-151. 被引量:2
  • 9高凌云.南极中微子探测器竣工[J].现代物理知识,2011(1):29-29.
  • 10徐晶,黄明阳,胡立军,郭新恒,杨炳麟.Detection of Supernova Neutrinos on the Earth for Large θ_(13)[J].Communications in Theoretical Physics,2014,61(2):226-234.

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