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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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Direct measurement of the resonance strengths and branching ratios of low-energy(p,γ)reactions on Mg isotopes 被引量:1
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作者 Hao Zhang Zhi-Hong Li +13 位作者 Jun Su Yun-Ju Li Chen Chen Long Zhang fu-qiang cao Yang-Ping Shen Wei Nan Wei-KeNan Xin-Yue Li Li-Hua Chen Gang Lian Bao-Qun Cui Bing Guo Wei-Ping Liu 《Chinese Physics C》 SCIE CAS CSCD 2021年第8期132-138,共7页
Proton capture reactions on Mg isotopes are significant in the Mg-Al cycle in stellar H-burning.In particular,the resonance strengths and branching ratios of low-energy resonances in 23Mg(p,γ)26Al reactions determine... Proton capture reactions on Mg isotopes are significant in the Mg-Al cycle in stellar H-burning.In particular,the resonance strengths and branching ratios of low-energy resonances in 23Mg(p,γ)26Al reactions determine the production of which is one of the most important long-lived radioactive nuclei in nuclear astrophysics.In this article,we report our first experiment using the intense proton beam of approximately 2 mA provided by the JUNA accelerator ground laboratory and a new technique that can minimize the composition change of targets under intense beam irradiation.The resonance strengths and branching ratios of E=214,304,and 326 keV resonances in the reactions of 2~4Mg(p,γ)25Al,25Mg(p,γ)26Al,and 26Mg(p,γ)27Al,respectively,were measured with high accuracy.The success of this experiment provides a good calibration for the nuclear astrophysical experiment at the Jinping underground laboratory. 展开更多
关键词 stellar hydrogen burning resonance reactions radiative capture
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