机构地区:[1]Dept. of Physics, Dept. of Astronomy, and CCAPP, The Ohio State University [2]Department of Engineering Physics,Tsinghua University [3]Science and Technology on Reliability and Environmental Engineering Laboratory,Beijing Institute of Spacecraft Environment Engineering [4]School of Physics, Shandong University [5]School of Physics, Nankai University [6]Institute of Modern Physics, East China University of Science and Technology [7]Institute of Physics, National Chiao-Tung University [8]University of Maryland, College Park [9]Department of Geophysics, Faculty of Mathematics and Physics, Charles University in Prague [10]School of Physics, Sun Yat-Sen University [11]Department of Civil Engineering, Tsinghua University [12]Institute of Hydrogeology and Environmental Geology, Chinese Academy of Geological Sciences [13]Fujian University of Technology [14]Department of Structural Steels, China Iron & Steel Research Institute Group [15]Brookhaven National Laboratory [16]School of Physical Sciences, University of Chinese Academy of Sciences [17]School of Physics and Technology, Wuhan University [18]Institut für Kern- und Teilchenphysik, Technische Universitt Dresden
出 处:《Chinese Physics C》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)
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.
关 键 词:CJPL Jinping neutrino experiment solar neutrino geo-neutrino supernova neutrino
分 类 号:O572.321[理学—粒子物理与原子核物理]
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