Magnetically assisted explosions of weakly magnetized stars

Hidetomo Sawai, Shoichi Yamada

    研究成果: Article

    抜粋

    We carried out high resolution simulations of weakly-magnetized core-collapse supernovae in two-dimensional axisymmetry in order to see the influence of the magnetic field and rotation on the explosion. We found that the magnetic field amplified by magnetorotational instability (MRI) has a great positive impact on the explosion by enhancing the neutrino heating, provided that the progenitor has large angular momentum close to the highest value found in stellar evolution calculations. We also found that even for progenitors neither involving strong magnetic flux nor large angular momentum, the magnetic field is greatly amplified by the convection aand rotation, and this leads to the boost of the explosion again by enhancing the neutrino heating.

    元の言語English
    ページ(範囲)125-130
    ページ数6
    ジャーナルProceedings of the International Astronomical Union
    12
    発行部数S331
    DOI
    出版物ステータスPublished - 2017 2 1

    ASJC Scopus subject areas

    • Astronomy and Astrophysics

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