Numerical simulations of core-collapse supernovae imposing steady shock approximation

Masaru Watanabe, Tatsuya Yamasaki, Hideyuki Suzuki, Shoichi Yamada

    研究成果: Article

    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.

    元の言語English
    ページ(範囲)155-156
    ページ数2
    ジャーナルJournal of Physics: Conference Series
    31
    発行部数1
    DOI
    出版物ステータスPublished - 2006 3 22

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    supernovae
    shock
    personal computers
    approximation
    shock waves
    simulation

    ASJC Scopus subject areas

    • Physics and Astronomy(all)

    これを引用

    Numerical simulations of core-collapse supernovae imposing steady shock approximation. / Watanabe, Masaru; Yamasaki, Tatsuya; Suzuki, Hideyuki; Yamada, Shoichi.

    :: Journal of Physics: Conference Series, 巻 31, 番号 1, 22.03.2006, p. 155-156.

    研究成果: Article

    Watanabe, Masaru ; Yamasaki, Tatsuya ; Suzuki, Hideyuki ; Yamada, Shoichi. / Numerical simulations of core-collapse supernovae imposing steady shock approximation. :: Journal of Physics: Conference Series. 2006 ; 巻 31, 番号 1. pp. 155-156.
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