Nuclear Uncertainties of s-Process in Astrophysics  

作　　者：ZHANG You-jin CHEN Yong-shou GUO Jian-you HOU Su-qing LI Zhi-hong SHI Jian-rong 

机构地区：[1]Department of Nuclear Physics [2]Anhui University [3]Institute of Modern Physics,Chinese Academy of sciences [4]National Astronomy and Astrophysics,Chinese Academy of Sciences

出　　处：《Annual Report of China Institute of Atomic Energy》2012年第1期71-71,共1页中国原子能科学研究院年报（英文版）

基　　金：Supported by National Natural Science Foundation of China (11021504, 11175258, 11275068, 11175001)

摘　　要：The heavy elements in the universe are formed during the s- and r-processes mainly in AGB stars and supernovae, respectively. Simulation of s- and r-nucleosynthesis critically depends on the neutron capture and weak decay rates for all nuclei on the reaction chain. The present work analyzes systematically

分 类 号：P14[天文地球—天体物理]