Numerical simulations of core-collapse supernovae imposing steady shock approximation

Masaru Watanabe, Tatsuya Yamasaki, Hideyuki Suzuki, Shoichi Yamada

    Research output: Contribution to journalArticle

    Abstract

    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.

    Original languageEnglish
    Pages (from-to)155-156
    Number of pages2
    JournalJournal of Physics: Conference Series
    Volume31
    Issue number1
    DOIs
    Publication statusPublished - 2006 Mar 22

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    supernovae
    shock
    personal computers
    approximation
    shock waves
    simulation

    ASJC Scopus subject areas

    • Physics and Astronomy(all)

    Cite this

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

    In: Journal of Physics: Conference Series, Vol. 31, No. 1, 22.03.2006, p. 155-156.

    Research output: Contribution to journalArticle

    Watanabe, Masaru ; Yamasaki, Tatsuya ; Suzuki, Hideyuki ; Yamada, Shoichi. / Numerical simulations of core-collapse supernovae imposing steady shock approximation. In: Journal of Physics: Conference Series. 2006 ; Vol. 31, No. 1. pp. 155-156.
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