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Progress of Jinping Underground laboratory for Nuclear Astrophysics(JUNA) 被引量:8
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作者 WeiPing Liu ZhiHong Li +61 位作者 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 《Science China(Physics,Mechanics & Astronomy)》 SCIE EI CAS CSCD 2016年第4期1-7,共7页
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 dire... 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^(25)Mg(p,γ)^(26)Al,^(19)F(p,α)^(16)O,^(13)C(α,n)^(16)O and ^(12)C(α,γ)^(16)O 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. 展开更多
关键词 direct measurement underground laboratory (25)Mg(p γ)(26)Al 19fp α)(16)O (13)C(α n)(16)O and (12)C(α γ)(16)O reactions Gamow window JUNA
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极高温度下^(19)F(p,α)^(16)O与^(19)F(p,γ)^(20)Ne两反应道分支比的计算
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作者 叶子飘 戴长江 《湖南大学学报(自然科学版)》 EI CAS CSCD 北大核心 2004年第3期105-107,共3页
用WKB方法计算在极高温度(非共振情况)下19F(p,α)16O与19F(p,γ)20Ne两反应道分支比.在CNO循环中,这两个核反应反应速度的快慢直接影响着16O和20Ne的含量,进而影响着17F和18F中微子的流量.计算表明,在(2~3)×107K温度范围内其分... 用WKB方法计算在极高温度(非共振情况)下19F(p,α)16O与19F(p,γ)20Ne两反应道分支比.在CNO循环中,这两个核反应反应速度的快慢直接影响着16O和20Ne的含量,进而影响着17F和18F中微子的流量.计算表明,在(2~3)×107K温度范围内其分支比值R约为1.189×103.这表明在CNO循环中,核反应19F(p,γ)20Ne可以忽略. 展开更多
关键词 ^19f α)^16O ^19f γ)^20Ne 分支比R 极高温度 WKB方法
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