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快速的中微子风味转换可以帮助和阻碍中微子驱动的爆炸
Jakob Ehring1,2,3, Sajad Abbar1, Hans-Thomas Janka2
1Max-Planck-Institut für Physik (Werner-Heisenberg-Institut), Föhringer Ring 6, D-80805 München, Germany.
Physical review letters
|August 25, 2023
概括
快速中微子风味转换 (FFC) 模拟显示对核心崩超新星的混合效应. 在低质量恒星中,FFC有助于爆炸,但在高质量恒星中,它阻碍了爆炸.
科学领域:
- 天体物理学 天体物理学
- 核物理 核物理 核物理
- 计算科学 计算科学
背景情况:
- 核心崩超新星 (SNe) 对宇宙元素分布至关重要.
- 中微子风味转换是一种影响SN爆炸的拟议机制.
- 之前的模拟缺乏快速中微子风味转换 (FFC) 的详细处理.
研究的目的:
- 调查FFC对核心崩超新星动态的影响.
- 探索FFC如何影响不同原始质量的SN爆炸结果.
- 介绍第一个包含FFC反的3D模拟.
主要方法:
- 核心崩超新星的轴对称模拟.
- 假设即时的风味平衡,对FFC的图形处理.
- 对于FFC的空间领域的系统变化.
主要成果:
- 在低质量 (9-12 M) 的祖先中,FFC促进了SN爆炸.
- FFC延迟或减弱了更大质量的原始体 (大约20M) 的爆炸.
- FFC的空间范围显著影响爆炸结果.
结论:
- 在核心崩的超新星中,FFC起着复杂的作用.
- FFC的影响取决于原始体质量.
- 需要进一步的研究来完善 SN 模拟中的 FFC 模型.
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