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超新星铁星核区对流不稳定的数值模拟

NUMERICAL SIMULATION OF CONVECTIVE INSTABILITY IN THE IRON CORE OF SUPERNOVAE

    摘要
  • 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。

     

    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.

     

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