Nonlinear growth of Rayleigh-Taylor instabilities and mixing in SN 1987A

Nonlinear growth of Rayleigh-Taylor instabilities and mixing in SN 1987A
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DOI:
10.1086/185779
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发表时间:
1990-08
期刊:
The Astrophysical Journal
影响因子:
--
通讯作者:
I. Hachisu;T. Matsuda;K. Nomoto;T. Shigeyama
I. Hachisu;T. Matsuda;K. Nomoto;T. Shigeyama
中科院分区:
其他
文献类型:
--
作者:
I. Hachisu;T. Matsuda;K. Nomoto;T. Shigeyama

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利用二维轴对称流体力学程序研究了Rayleigh-Taylor(R-T)不稳定性的起源和发展。在冲击波发生后,观察到了2000 S的蘑菇状结构,并且在H/He界面处开始发展R-T不稳定性。这些结果与Arnett等人的结果有很好的相关性。(1989)数据。研究了SN1987A喷射物中的混合程度以及R-T不稳定性与混合的关系。参考文献36篇。
The origin and development of the Rayleigh-Taylor (R-T) instability is studied using an axisymmetric two-dimensional hydrodynamic code. It is observed that mushroomlike structures appear 2000 s after the blast shock and the R-T instability starts to grow at the H/He interface. These results correlate well with the Arnett et al. (1989) data. The extent of mixing in the ejecta of SN 1987A and the relation between R-T instability and mixing are examined. 36 refs.