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Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
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快速旋转的核心崩超新星中的大规模动力发电机和磁流动
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
概括
质子中子恒星中的磁动能产生强大的磁场,为超新星和马射线爆发提供动力. 这项研究表明流驱动有序的磁场,
科学领域:
- 天体物理学
- 血物理
- 计算科学
背景情况:
- 在高能天体物理系统中,磁动力非常重要.
- 不稳定性可以快速放大磁场,可能形成磁性强度场.
- 磁星形成与巨大的恒星中的磁旋不稳定性和动力发电机作用有关.
研究的目的:
- 调查磁旋不稳定驱动的流是否可以产生大规模的有序磁场.
- 在快速旋转的质子中子星中探索水磁流的作用.
- 确定这些过程是否可以解释Ic-bl型超新星和长马射线爆发的原始物.
主要方法:
- 全球,三维,一般相对论磁动力学模拟.
- 分析能量级联和磁场的排序.
- 与超新星和马射线爆发的观测候选物进行比较.
主要成果:
- 质子中子星中的水磁流会呈现反向的能量级联.
- 一个大规模的,有序的形磁场被产生.
- 产生的电场与双极磁旋驱动的外流一致.
结论:
- 快速旋转的大质量恒星是Ic-bl类超新星和长马射线爆发的可能祖先.
- 证明了磁形成的可行机制.
- 这些发现表明磁星驱动的超光超新星的潜在起源.
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