Numerical simulations of core-collapse supernovae imposing steady shock approximation

Masaru Watanabe; Tatsuya Yamasaki; Hideyuki Suzuki; Shoichi Yamada

doi:10.1088/1742-6596/31/1/030

Numerical simulations of core-collapse supernovae imposing steady shock approximation

Masaru Watanabe^*, Tatsuya Yamasaki, Hideyuki Suzuki, Shoichi Yamada

^*この研究の対応する著者

先進理工学部

研究成果: Article › 査読

抄録

We carried out one-dinensional long-term numerical simulations of core-collapse supernovae imposing steady shock approximation. As a result of a computation, we found core does not explode and shock wave stalls within several hundreds milliseconds from bounce. However, we execute long-term numerical simulation until 3.5 seconds from bounce with short CPU time using Personal Computer.

本文言語	English
ページ（範囲）	155-156
ページ数	2
ジャーナル	Journal of Physics: Conference Series
巻	31
号	1
DOI	https://doi.org/10.1088/1742-6596/31/1/030
出版ステータス	Published - 2006 3月 22

ASJC Scopus subject areas

物理学および天文学（全般）

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10.1088/1742-6596/31/1/030

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Numerical simulations of core-collapse supernovae imposing steady shock approximation

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