Hydrodynamic Instabilities in Inertial Confinement Fusion

N. Hoffman
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引用次数: 3

Abstract

The focus of the paper is on buoyancy-driven instabilities of the Rayleigh-Taylor type, which are commonly regarded as the most important kind of hydrodynamic instability in inertial-confinement-fusion implosions. The paper is intended to be pedagogical rather than research-oriented, and so is by no means a comprehensive review of work in this field. Rather, it is hoped that the student will find here a foundation on which to build an understanding of current research, and the experienced researcher will find a compilation of useful results. The aim of the paper is to discuss the evolution of a single Rayleigh-Taylor-unstable mode, from its linear phase to its late-stage constant-velocity bubble growth, with a brief consideration of the saturation of linear growth. The influence of other modes in invoked only in the short-range sense (in wavenumber space) of the Haan saturation model. Owing to limitations of space, the treatment of other instabilities such as Richtmyer-Meshkov and Kelvin-Helmholtz is necessarily very brief, and entirely inadequate as an introductory discussion. Likewise, there is no reference to the effect of convergent geometry, to long-range mode coupling, or to shape effects in three-dimensional growth. Furthermore, there is no reference to the large body of experimental research relatedmore » to hydrodynamic instabilities.« less
惯性约束聚变中的流体动力不稳定性
本文的重点是瑞利-泰勒型的浮力驱动不稳定性,这通常被认为是惯性约束聚变内爆中最重要的一种水动力不稳定性。本文旨在以教学为导向,而不是以研究为导向,因此绝不是对该领域工作的全面回顾。相反,我们希望学生在这里找到一个基础,在此基础上建立对当前研究的理解,而有经验的研究人员将找到有用结果的汇编。本文的目的是讨论一个单一的瑞利-泰勒不稳定模态从其线性阶段到其后期等速气泡生长的演变,并简要考虑线性生长的饱和。其他模态的影响仅在Haan饱和模式的短距离意义上(波数空间)被调用。由于篇幅的限制,对其他不稳定性,如richmyer - meshkov和Kelvin-Helmholtz的处理必然非常简短,作为介绍性讨论是完全不够的。同样,也没有提到收敛几何的影响,也没有提到远程模式耦合,也没有提到三维增长中的形状效应。此外,也没有大量与水动力不稳定性有关的实验研究。«少
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