학술논문
Progress of Jinping Underground laboratory for Nuclear Astrophysics (JUNA)
Document Type
article
Author
Liu WeiPing; Li ZhiHong; He JiangJun; Tang XiaoDong; Lian Gang; An Zhu; Chang JianJun; Chen Han; Chen QingHao; Chen XiongJun; Chen ZhiJun; Cui BaoQun; Du XianChao; Fu ChangBo; Gan Lin; Guo Bing; He GuoZhu; Heger Alexander; Hou SuQing; Huang HanXiong; Huang Ning; Jia BaoLu; Jiang LiYang; Kubono Shigeru; Li JianMin; Li KuoAng; Li Tao; Li YunJu; Lugaro Maria; Luo XiaoBing; Ma HongYi; Ma ShaoBo; Mei DongMing; Qian YongZhong; Qin JiuChang; Ren Jie; Shen YangPing; Su Jun; Sun LiangTing; Tan WanPeng; Tanihata Isao; Wang Shuo; Wang Peng; Wang YouBao; Wu Qi; Xu ShiWei; Yan ShengQuan; Yang LiTao; Yang Yao; Yu XiangQing; Yue Qian; Zeng Sheng; Zhang HuanYu; Zhang Hui; Zhang LiYong; Zhang NingTao; Zhang QiWei; Zhang Tao; Zhang XiaoPeng; Zhang XueZhen; Zhang ZiMing; Zhao Wei; Zhao Zuo; Zhou Chao
Source
EPJ Web of Conferences, Vol 109, p 09001 (2016)
Subject
Language
English
ISSN
2100-014X
Abstract
Jinping Underground lab for Nuclear Astrophysics (JUNA) will take the advantage of the ultralow background in Jinping underground lab, high current accelerator based on an ECR source and highly sensitive detector to study directly a number of crucial reactions to the hydrostatic stellar evolution for the first time at their relevant stellar energies. 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. The experimental setup, which include the accelerator system with high stability and high intensity, the detector system, and the shielding material with low background, will be established during the above research. The current progress of JUNA will be given.