Particularly, the slow neutron capture processes (s processes) and the evolution of AGB stars are briefly described.
特别是 ,对慢中子俘获过程 (s 过程 )的机制及相关的AGB星演化图像作了简单介
For selecting nuclides to transform slow neutron into gamma photon effectively, the main decisive aspects are analyzed basing on relative cross section data and a specific model is calculated by using S N method.
为选出能有效地实现慢中子 γ光子转换的核素 ,根据有关截面数据分析了主要的决定因素 ,并结合具体模型用离散纵标法作了计算。
