摘要
锦屏深地核天体物理(JUNA)实验项目将利用中国锦屏深地实验室(CJPL)的良好条件,在天体物理伽莫夫能量窗口开展核天体关键反应^(25)Mg(p,γ)^(26)Al、^(19)F(p,α)^(16)O、^(13)C(α,n)^(16)O和^(12)C(α,γ)^(16)O的直接测量,为理解恒星演化和元素起源提供新的数据。目前,已经在地面上对加速器装置、束流稳定性、靶、探测器以及电子学进行了系统的测试。地面实验内容包括高纯锗探测器效率刻度,^(25)Mg(p,γ)^(26)Al在304 keV的共振强度测量,^(19)F(p,δ)^(16)O的截面测量,聚乙烯作为慢化体的中子探测器的设计、加工和效率刻度,靶的设计和稳定性检测等。JUNA项目整体进展顺利,地面实验已取得一系列关键进展和初步成果。在不远的将来,JUNA项目将有序开展地下实验,完成设定目标,也将促进更广泛的国际合作,助力于天体演化中的若干重大科学问题的解决。
A number of nuclear reactions such as^(25)Mg(p,γ)^(26)Al,^(13)C(α,n)^(16)O,^(12)C(α,β)^(16)O and ^(19 )F(p,α)^(16)O will be measured directly down to the Gamow window energy range in Jinping Underground Nuclear Astrophysics(JUNA)Experiment,taking the advantage of the ultra-low background in China Jinping Unerground Laboratory(CJPL).The measurements can provide updated data for understanding the evolution of stars and the origin of elements.Up to now,tests of accelerator,beam,targets,detectors,and electronics have been performed systematically on the ground.The high-purity germanium detectors efficiency calibration,304 keV resonance strengths measurement in^(25)Mg(p,γ)^(26)Al,^(19) F(p,α)^(16)O cross section measurement,neutron detector design,production and efficiency calibrationas as well as target design and stability test are included as overground experiments.The Whole JUNA project is going smoothly in general.A series of key progresses and primary results have been reached on the ground.Underground experiments in the JUNA project will be carried out in order and reach the prospected goals in the near future.Broader international cooperation will also be promoted,supporting the solution of several major scientific problems in the evolution of cosmogony.
作者
柳卫平
李志宏
何建军
唐晓东
连钢
郭冰
苏俊
李云居
崔保群
孙良亭
武启
安竹
谌阳平
陈治钧
杜先超
符长波
甘林
贺国珠
Alexander Heger
侯素青
黄翰雄
黄宁
江历阳
Shigeru Kubono
李荐民
李阔昂
李涛
Maria Lugaro
罗小兵
马少波
韩治宇
李鑫悦
马田丽
梅东明
南威克
南巍
陈晨
张昊
张龙
曹富强
钱永忠
秦久昌
任杰
谭万鹏
Isao Tanihata
王鹏
王硕
王友宝
许世伟
颜胜权
曾志
于祥庆
岳骞
曾晟
张环宇
张辉
杨丽桃
张立勇
张宁涛
张奇玮
张涛
方晓
张笑鹏
张雪珍
陈云华
祁宁春
吴世勇
郭绪元
周济芳
何胜明
宁金华
岳剑锋
LIU Weiping;LI Zhihong;HE Jianjun;TANG Xiaodong;LIAN Gang;GUO Bing;SU Jun;LI Yunju;CUI Baoqun;SUN Liangting;WU Qi;AN Zhu;CHEN Yangping;CHEN Zhijun;DU Xianchao;FU Changbo;GAN Lin;HE Guozhu;Alexander Heger;HOU Suqing;HUANG Hanxiong;HUANG Ning;JIANG Liyang;Shigeru Kubono;LI Jianmin;LI Kuoang;LI Tao;Maria Lugaro;LUO Xiaobing;MA Shaobo;HAN Zhiyu;LI Xinyue;MA Tianli;MEI Dongming;NAN Weike;NAN Wei;CHEN Chen;ZHANG Hao;ZHANG Long;CAO Fuqiang;QIAN Yongzhong;QIN Jiuchang;REN Jie;TAN Wanpeng;Isao Tanihata;WANG Peng;WANG Shuo;WANG Youbao;XU Shiwei;YAN Shengquan;ZENG Zhi;YU Xiangqing;YUE Qian;ZENG Sheng;ZHANG Huanyu;ZHANG Hui;YANG Litao;ZHANG Liyong;ZHANG Ningtao;ZHANG Qiwei;ZHANG Tao;FANG Xiao;ZHANG Xiaopeng;ZHANG Xuezhen;CHEN Yunhua;QI Ningchun;WU Shiyong;GUO Xuyuan;ZHOU Jifang;HE Shengming;NING Jinhua;YUE Jianfeng(China Institute of Atomic Energy,Beijing 102413,China;School of Nuclear Science and Technology,University of Chinese Academy of Sciences,Beijing 101408,China;Institute of Mordern Physics,Chinese Academy of Sciences,Lanzhou 730000,China;College of Nuclear Science and Technology,Beijing Normal University,Beijing 100875,China;Institute of Nuclear Science and Technology,Sichuan University,Chengdu 610041,China;Department of Engineering Physics,Tsinghua University,Beijing 100084,China;Institue of Modern Physics,Fudan University,Shanghai 200433,China;School of Physics and Astronomy,Monash University,Melbourne 3800,Australia;Institute of Physical and Chemical Research,Saitama Prefecture and Hokkaido 3510198,Japan;Conakry Observatory,Research Centre for Astronomy and Earth Science,Budapest 10111239,Hungary;University of South Dakota,State Ultra Low Background Particle Physics Experiment Centre,South Pakota Vermilion 57069,America;School of Physics and Astronomy,University of Minnesota,Minnesota polis/St.Paul 55455,America;Nuclear Astrophysics Department,University of Notre Dame,Indiana Notre Dame 102413,China;Research Center for Nuclear Physics,Osaka Unibversity,Suita City 5650887167,Japan;School of Space Science and Physics,Shandong University,Weihai 264209,Shandong,China;School of Physics and Astronomy,Shanghai Jiaotong University,Shanghai 200240,China;Sino-French Institute of Nuclear Engineering and Technology,Sun Yat-sen University,Guangzhou 510275,China;Institute of High Energy Physics,Chinese Academy of Sciences,Beijing 100049,China;Yalong River Basin Hydropowper Development Co.,Chengdu 610056,China)
出处
《原子核物理评论》
CAS
CSCD
北大核心
2020年第3期283-290,共8页
Nuclear Physics Review
基金
国家自然科学基金资助项目(11490560,11475265)
国家财政部稳定支持项目(WDJC-2019-13)。
关键词
天体物理
深地实验室
直接测量
伽莫夫能量窗口
astrophysics
underground laboratory
direct measurement
Gamow window energy