中国物理B ›› 2007, Vol. 16 ›› Issue (10): 3146-3149.doi: 10.1088/1009-1963/16/10/055
• • 上一篇
刘门全, 张 洁, 罗志全
Liu Men-Quan(刘门全), Zhang Jie(张洁), and Luo Zhi-Quan(罗志全)†
摘要: A new improved nuclear partition function is employed to calculate the nuclear statistical equilibrium (NSE) in core-collapse supernova environment. The results show that the change of nucleus abundance is slight even though the temperature is higher than 10$^{11}$\,K when shock propagates, which indicates that the effect of the nuclear partition function is not so important as shown in the previous calculations, but it can also be considered in detailed simulation if it is sensitive to weak interaction rates in core-collapse supernova.
中图分类号: (Nuclear physics aspects of novae, supernovae, and other explosive environments)