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Updated: Mar 29, 2026

Magnetically Induced Rotating Rayleigh-Taylor Instability
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急速に回転する核崩壊超新星における大規模なダイナモと磁気流動

Philipp Mösta1,2, Christian D Ott1, David Radice1

  • 1TAPIR, Walter Burke Institute for Theoretical Physics, Mailcode 350-17, California Institute of Technology, Pasadena, California 91125, USA.

Nature
|December 1, 2015
PubMed
まとめ

陽子中性子星の磁気流動的な乱れは強い磁場を作り,超新星とガンマ線爆発を起こすことができます. この研究では 乱流が有秩序な磁場を駆動し マグネタール形成とハイパーノヴァ現象を説明しています

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