Progress of Jinping Underground laboratory for Nuclear Astrophysics(JUNA)
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 rele...
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creator | 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 |
description | 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. |
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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. 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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. 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Astronomy</addtitle><date>2016</date><risdate>2016</risdate><issue>4</issue><spage>1</spage><epage>7</epage><pages>1-7</pages><issn>1674-7348</issn><eissn>1869-1927</eissn><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. 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language | eng |
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source | Springer Online Journals Complete; Alma/SFX Local Collection |
subjects | ECR源 地下实验室 强流加速器 核天体物理学 流体静压 演化过程 直接测量 高灵敏度 |
title | Progress of Jinping Underground laboratory for Nuclear Astrophysics(JUNA) |
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