Author:
Zhang Hao,Li Zhi-Hong,Su Jun,Li Yun-Ju,Chen Chen,Zhang Long,Cao Fu-Qiang,Shen Yang-Ping,Nan Wei,Nan Wei-Ke,Li Xin-Yue,Chen Li-Hua,Lian Gang,Cui Bao-Qun,Guo Bing,Liu Wei-Ping
Abstract
Abstract
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 25Mg(
)26Al reactions determine the production of 26Al, 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 24Mg(
)25Al, 25Mg(
)26Al, and 26Mg(
)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.
Funder
National Natural Science Foundation of China
Continuous Basic Scientific Research Project
Subject
Astronomy and Astrophysics,Instrumentation,Nuclear and High Energy Physics
Cited by
4 articles.
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