计算物理 ›› 1997, Vol. 14 ›› Issue (S1): 545-546.

• 论文 • 上一篇    下一篇

超新星铁星核区对流不稳定的数值模拟

张锁春   

  1. 中国科学院应用数学研究所, 北京 100080
  • 收稿日期:1997-02-28 修回日期:1997-05-12 出版日期:1997-12-25 发布日期:1997-12-25
  • 基金资助:
    国家自然科学基金和国家攀登计划资助项目

NUMERICAL SIMULATION OF CONVECTIVE INSTABILITY IN THE IRON CORE OF SUPERNOVAE

Zhang Suochun   

  1. Institute of Applied Methematics, The Chinese Academy of Sciences, Beijing 100080
  • Received:1997-02-28 Revised:1997-05-12 Online:1997-12-25 Published:1997-12-25

摘要: 通过数值模拟发现,超新星铁星核区中~(0.74~0.91)M区间是十分重要的对流不稳定区域。

关键词: 数值模拟, 铁星核, 对流不稳性

Abstract: The(0.74-0.91)M of the iron core of Supernovae is a very important region of convective instability,which is found through the present numerical simulation.

Key words: numerical simulation, iron core, convective instability

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