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Progress of Jinping Underground laboratory for Nuclear Astrophysics (JUNA)
Authors:WeiPing Liu  ZhiHong Li  JiangJun He  XiaoDong Tang  Gang Lian  Zhu An  JianJun Chang  Han Chen  QingHao Chen  XiongJun Chen  ZhiJun Chen  BaoQun Cui  XianChao Du  ChangBo Fu  Lin Gan  Bing Guo  GuoZhu He  Alexander Heger  SuQing Hou  HanXiong Huang  Ning Huang  BaoLu Jia  LiYang Jiang  Shigeru Kubono  JianMin Li  KuoAng Li  Tao Li  YunJu Li  Maria Lugaro  XiaoBing Luo  HongYi Ma  ShaoBo Ma  DongMing Mei  YongZhong Qian  JiuChang Qin  Jie Ren  YangPing Shen  Jun Su  LiangTing Sun  WanPeng Tan  Isao Tanihata  Shuo Wang  Peng Wang  YouBao Wang  Qi Wu  ShiWei Xu  ShengQuan Yan  LiTao Yang  Yao Yang  XiangQing Yu  Qian Yue  Sheng Zeng  HuanYu Zhang  Hui Zhang  LiYong Zhang  NingTao Zhang  QiWei Zhang  Tao Zhang  XiaoPeng Zhang  XueZhen Zhang  ZiMing Zhang  Wei Zhao  Zuo Zhao  Chao Zhou  JUNA Collaboration
Abstract:Jinping Underground laboratory for Nuclear Astrophysics (JUNA) will take the advantage of the ultra-low background of CJPL lab and high current accelerator based on an ECR source and a highly sensitive detector to directly study for the first time a number of crucial reactions occurring at their relevant stellar energies during the evolution of hydrostatic stars. In its first phase, JUNA aims at the direct measurements of 25Mg(p,γ)26Al, 19F(p,α)16O, 13C(α,n)16O and 12C(α,γ)16O reactions. The experimental setup, which includes an accelerator system with high stability and high intensity, a detector system, and a shielding material with low background, will be established during the above research. The current progress of JUNA will be given.
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