在辐射等离子体中形成冲击波.
F Garcia-Rubio1, V Tranchant2, E C Hansen2
1Laboratory for Laser Energetics, Rochester, New York 14623, USA and Department of Mechanical Engineering, <a href="https://ror.org/022kthw22">University of Rochester</a>, Rochester, New York 14627, USA.
Physical review. E
|July 18, 2024
概括
这项研究调查了辐射介质中的弱冲击,揭示了它们通常会随着时间的推移变得光学厚. 薄溶液是短暂的,与过密层相连,对于冲击演化提供了缩放规律.
科学领域:
- 等离子体物理学的物理学
- 天体物理流体动力学流体动力学
- 计算物理 计算物理
背景情况:
- 辐射冲击结构复杂,涉及交替的光学厚度/薄度区域.
- 传统研究经常使用静止框架,限制了对冲击进化的理解.
- 放射性等离子体中弱冲击形成需要动态分析.
研究的目的:
- 从理论上研究辐射介质中弱冲击的时间演变.
- 为了分析两个具有不同压力的辐射等离子体相互作用时的弱冲击形成.
- 为了推导出光学厚度和薄度解决方案的条件,并提供缩放规律.
主要方法:
- 应用一个减小扰动方法来导出一个汉堡式方程.
- 对扰动变量的分析,包括辐射场.
- 来自FLASH模拟的支持理论发现.
主要成果:
- 一个汉堡式方程控制了弱冲击和辐射的时间演变.
- 在波兹曼数值以下的弱冲击中,光学厚度的溶液是不对称的.
- 光学上薄的溶液是暂时的,并且依赖于压缩材料中的过密层.
结论:
- 基于冲击强度和博尔茨曼数的光学厚度/薄度溶液的衍生条件.
- 确立了弱冲击随着时间的推移倾向于光学厚度的状态.
- 提供了冲击形成时间和宽度的缩放规律,通过模拟验证并对代码基准测试有用.
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