Recent progress in nuclear astrophysics research and its astrophysical implications at the China Institute of Atomic Energy
作者:Wei-ping Liu, Bing Guo, Z. An, Bao-Qun Cui, Xiao Fang, Chang-Bo Fu, B. Gao, Jian-Jun He, Yu-Chen Jiang, Chong Lv, Er-Tao Li, Ge-Xing Li, Yun-Ju Li, Zhi-Hong Li, G. Lian, Wei-Ping Lin, Yi-Hui Liu, W. Nan, W. Nan, Yang-Ping Shen, Na Song, Jun Su, Liang-Ting Sun, Xiao-Dong Tang, Luo-Huan Wang, Shuo Wang, You-Bao Wang, Di Wu, Xiao-Feng Xi, Sheng-Quan Yan, Li-Yong Zhang · 发表于:Nuclear Science and Techniques · 年份:2024 · DOI:10.1007/s41365-024-01590-3 · 被引用次数:17
Nuclear 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,γ\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\gamma$$\end{document}) reactions with short-lived radioactive isotopes. However, direct meas...