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作 者:Wei-Ke Nan You-Bao Wang Yao-De Sheng Jun Su Yu-Qiang Zhang Lu-Yang Song Yang-Ping Shen Fu-Qiang Cao Chen Chen Chao Dong Yun-Ju Li Zhi-Hong Li Gang Lian Wei Nan Qiang Wang Na Song Sheng-Quan Yan Seng Zeng Qi-Wen Fan Hao Zhang Ming-Hao Zhu Bing Guo Wei-Ping Liu
机构地区:[1]China Institute of Atomic Energy,P.O.Box 275(10),Beijing 102413,China [2]Key Laboratory of Beam Technology and Material Modification of Ministry of Education,College of Nuclear Science and Technology,Beijing Normal University,Beijing 100875,China [3]Institute of Radiation Technology,Beijing Academy of Science and Technology,Beijing 100875,China [4]School of Physics,Xi’an Jiaotong University,Xi’an 710049,China [5]Department of Physics,Southern University of Science and Technology,Shenzhen 518055,China
出 处:《Nuclear Science and Techniques》2024年第11期237-243,共7页核技术(英文)
基 金:supported by the National Key Research and Development Project (No. 2022YFA1602301);the National Natural Science Foundation of China (Nos. U2267205, 12275361, 12125509, 12222514, 11961141003, and 12005304);the CAST Young Talent Support Plan;the CNNC Science Fund for Talented Young Scholars;the Continuous-Support Basic Scientific Research Project
摘 要:The ^(12)C+^(12)C fusion is one of the most important reactions in modern nuclear astrophysics.The trend and magnitude of the reaction rate within the Gamow window strongly influence various astrophysical processes.However,direct measurement of this reaction is extremely difficult,which makes it necessary to develop indirect methods.In this study,the ^(23)Na+p reaction system was used to study the compound nucleus ^(24)Mg.We employed a thick-target inverse kinematics method combined with theγ-charged-particle coincidence technique to measure the proton andα exit channels of ^(24)Mg.Technical details of the ^(23)Na+p thick-target inverse kinematics experiment and analysis are presented herein.
关 键 词:Nuclear astrophysics ^(12)C+^(12)C Thick-target inverse kinematics method γ-charged particle coincidence
分 类 号:TL61[核科学技术—核技术及应用]
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