Models for Type Ia Supernovae

被引：0

作者：

Woosley, SE ^{[1
]}

机构：

[1] Univ Calif Santa Cruz, Dept Astron & Astrophys, Santa Cruz, CA 95064 USA

来源：

NUCLEAR PHYSICS A | 2001年 / 688卷 / 1-2期

关键词：

D O I：

暂无

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

Even assuming a Chandrasekhar Mass white dwarf as the common starting point for Type la supernova explosions, there remain many uncertainties in the theoretical outcome. Here particular attention is paid to the ignition conditions, which may be largely responsible for the observed diversity in observations. The advantages of and physical uncertainties of models based upon pure deflagration and delayed detonation are discussed with the conclusion that the former is more easily achieved.

引用

页码：9C / 16C

页数：8

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