中国物理B ›› 2007, Vol. 16 ›› Issue (10): 3146-3149.doi: 10.1088/1009-1963/16/10/055

• • 上一篇    

Nuclear statistical equilibrium at core-collapse supernova

刘门全, 张 洁, 罗志全   

  1. Institute of Theoretical Physics, China West Normal University, Nanchong 637002, China
  • 收稿日期:2007-01-13 修回日期:2007-03-30 出版日期:2007-10-08 发布日期:2007-10-08
  • 基金资助:
    Project supported by the National Natural Science Foundation of China (Grant No 10347008).

Nuclear statistical equilibrium at core-collapse supernova

Liu Men-Quan(刘门全), Zhang Jie(张洁), and Luo Zhi-Quan(罗志全)†   

  1. Institute of Theoretical Physics, China West Normal University, Nanchong 637002, China
  • Received:2007-01-13 Revised:2007-03-30 Online:2007-10-08 Published:2007-10-08
  • Supported by:
    Project supported by the National Natural Science Foundation of China (Grant No 10347008).

PDF (PC)

544

赞

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.

关键词: supernova, nucleosynthesis, abundances

Abstract: 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.

Key words: supernova, nucleosynthesis, abundances

中图分类号:  (Nuclear physics aspects of novae, supernovae, and other explosive environments)

  • 26.50.+x
97.60.Bw (Supernovae)