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Novel thick-target inverse kinematics method for the astrophysical ^(12)C+^(12)C fusion reaction
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作者 Wei-Ke Nan You-Bao Wang +20 位作者 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 《Nuclear Science and Techniques》 SCIE EI CAS CSCD 2024年第11期237-243,共7页
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.Ho... 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 the-charged-particle coincidence technique to measure the proton andexit channels of ^(24)Mg.Technical details of the ^(23)Na+p thick-target inverse kinematics experiment and analysis are presented herein. 展开更多
关键词 Nuclear astrophysics ^(12)C+^(12)C Thick-target inverse kinematics method -charged particle coincidence
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