Recent progress in nuclear astrophysics research and its astrophysical implications at the China Institute of Atomic Energy
Authors: Liu Wei-Ping , Guo Bing , An Zhu , Cui Bao-Qun , Fang Xiao , Fu Chang-Bo , Gao Bin-Shui , He Jian-Jun , Jiang Yu-Chen , Lv Chong , Li Er-Tao , Li Ge-Xing , Li Yun-Ju , Li Zhi-Hong , Lian Gang , Lin Wei-Ping , Liu Yi-Hui , Nan Wei , Nan Wei-Ke , Shen Yang-Ping , Song Na , Su Jun , Sun Liang-Ting , Tang Xiao-Dong , Wang Luo-Huan , Wang Shuo , Wang You-Bao , Wu Di , Xi Xiao-Feng , Yan Sheng-Quan , Zhang Li-Yong 
Published: November 2024

AbstractNuclear astrophysics is a rapidly developing interdisciplinary field of research that has received extensive attention from the scientific community since the mid-twentieth century. Broadly, it uses the laws of extremely small atomic nuclei to explain the evolution of the universe. Owing to the complexity of nucleosynthesis processes and our limited understanding of nuclear physics in astrophysical environments, several critical astrophysical problems remain unsolved. To achieve a better understanding of astrophysics, it is necessary to measure the cross sections of key nuclear reactions with the precision required by astrophysical models. Direct measurement of nuclear reaction cross sections is an important method of investigating how nuclear reactions influence stellar evolution. Given the challenges involved in measuring the extremely low cross sections of nuclear reactions in the Gamow peak and preparing radioactive targets, indirect methods, such as the transfer reaction, coulomb dissociation, and surrogate ratio methods, have been developed over the past several decades. These are powerful tools in the investigation of, for example, neutron-capture (n,$$\gamma$$
γ
) reactions with short-lived radioactive isotopes. However, direct measurement is still preferable, such as in the case of reactions involving light and stable nuclei. As an essential part of stellar evolution, these low-energy stable nuclear reactions have been of particular interest in recent years. To overcome the difficulties in measurements near or deeply within the Gamow window, the combination of an underground laboratory and high-exposure accelerator/detector complex is currently the optimal solution. Therefore, underground experiments have emerged as a new and promising direction of research. In addition, to better simulate the stellar environment in the laboratory, research on nuclear physics under laser-driven plasma conditions has gradually become a frontier hotspot. In recent years, the CIAE team conducted a series of distinctive nuclear astrophysics studies, relying on the Jinping Underground Nuclear Astrophysics platform and accelerators in Earth’s surface laboratories, including the Beijing Radioactive Ion beam Facility, as well as other scientific platforms at home and abroad. This research covered nuclear theories, numerical models, direct measurements, indirect measurements, and other novel approaches, achieving great interdisciplinary research results, with high-level academic publications and significant international impacts. This article reviews the above research and predicts future developments.