Standing accretion shock instability: Numerical simulations of core-collapse supernova

N. Ohnishi, Wakana Iwakami, K. Kotake, Shoichi Yamada, S. Fujioka, H. Takabe

    Research output: Contribution to journalArticle

    3 Citations (Scopus)

    Abstract

    Standing accretion shock instability (SASI) is one of the candidates to solve the mystery of why we cannot reproduce the explosion with the present core-collapse supernova models. We have studied this phenomenon with including neutrino heating and realistic EOS and found that SASI may enhance neutrino heating. Although g-mode of proto-neutron star may enhance the SASI growth, the simulations just including the pressure perturbation as a mimic of g-mode induced sound wave reveal no significant effect on the shock dynamics. Moreover, we discuss the required conditions toward the possible laboratory experiment of SASI.

    Original languageEnglish
    Article number042018
    JournalJournal of Physics: Conference Series
    Volume112
    Issue numberPart 4
    DOIs
    Publication statusPublished - 2008 Jun 12

    Fingerprint

    supernovae
    shock
    simulation
    neutrinos
    heating
    sound waves
    neutron stars
    explosions
    perturbation

    ASJC Scopus subject areas

    • Physics and Astronomy(all)

    Cite this

    Standing accretion shock instability : Numerical simulations of core-collapse supernova. / Ohnishi, N.; Iwakami, Wakana; Kotake, K.; Yamada, Shoichi; Fujioka, S.; Takabe, H.

    In: Journal of Physics: Conference Series, Vol. 112, No. Part 4, 042018, 12.06.2008.

    Research output: Contribution to journalArticle

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    AU - Yamada, Shoichi

    AU - Fujioka, S.

    AU - Takabe, H.

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