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中文核心期刊

激光聚变烧蚀流体力学不稳定性研究进展

RESEARCH PROGRESS ON HYDRODYNAMIC INSTABILITIES IN LASER FUSION ABLATION

  • 摘要: 激光聚变是实现可控核聚变的重要途径, 而内爆流体力学不稳定性的显著发展, 是性能退化的重要因素以及迈向更高增益的关键瓶颈. 作为内爆主要不稳定界面之一, 本文以烧蚀面扰动演化为切入点, 系统阐述了激光聚变烧蚀流体力学不稳定性的基本理论与最新研究进展. 首先简要介绍了激光聚变内爆物理基本概念以及主要过程. 其次, 介绍了点火对高收缩比、高内爆速度与高压缩的“三高”动力学的需求以及所伴随的流体力学不稳定性风险. 最后, 聚焦烧蚀面扰动增长, 在简要回顾烧蚀Richtmyer-Meshkov不稳定性(RMI)与烧蚀Rayleigh-Taylor不稳定性(RTI)等成熟理论之后, 系统介绍了近期若干新的成果: 一是在辐射驱动早期定位了由烧蚀面形变主导的新阶段; 二是在烧蚀RMI向烧蚀RTI过渡阶段, 实验证实了由稀疏波返回引发的非指数增长(secular增长)过程, 并预测了特定条件下的类似“冻结”现象; 三是针对烧蚀扰动增长后期气泡加速阶段, 给出了有限壳层厚度修正的拟合公式. 上述成果是对烧蚀不稳定性全过程机制机理的深化与完善, 为高增益聚变靶设计提供了理论依据与调控思路.

     

    Abstract: Laser fusion represents a promising approach to achieving controlled nuclear fusion, yet the rapid growth of hydrodynamic instabilities during the implosion remain a primary cause of performance degradation and a critical bottleneck for attaining higher gain. In inertial confinement fusion, the ablation front is among the most unstable interfaces, and its perturbation evolution critically affects target compression and threatens shell integrity. This article systematically reviews the fundamental physics and recent advances in ablative hydrodynamic instabilities, with a particular emphasis on the ablation-front dynamics. The basic concepts and key processes of laser-driven implosions are first outlined, covering the ablation, acceleration, deceleration, and stagnation phases. The stringent ignition requirements—namely, high convergence ratio, high implosion velocity, and high compression—are then described, along with the associated instability risks that arise under such extreme conditions. After briefly revisiting the well-established theories of the ablative Richtmyer-Meshkov instability (RMI) and the ablative Rayleigh-Taylor instability (RTI), we present three major recent advances that integrate theoretical analysis and experimental validation. First, a stage dominated by ablation-front deformation is identified in the early radiation-driven phase, preceding the conventional ablative RMI; this deformation sets the initial conditions for subsequent instability evolution. Second, during the transition from the ablative RMI to the ablative RTI, non-exponential (secular) growth dynamics induced by the return of rarefaction waves are experimentally confirmed, and a wave-number-dependent “freeze” phenomenon is predicted for specific perturbation modes, which may help suppress unwanted growth. Third, a modified fitting formula incorporating finite shell thickness is introduced to improve the accuracy of modeling bubble acceleration in the late nonlinear stage, providing better predictions for actual target designs. Collectively, these findings deepen the mechanistic understanding of ablative instability evolution from linear to deeply nonlinear regimes, and offer both theoretical guidance and practical strategies for optimizing high-gain fusion target performance.

     

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