Lehmann G, Spatschek K H, Sewell G
Institut für Theoretische Physik, Heinrich-Heine-Universität Düsseldorf, D-40225 Düsseldorf, Germany.
Phys Rev E Stat Nonlin Soft Matter Phys. 2013 Jun;87(6):063107. doi: 10.1103/PhysRevE.87.063107. Epub 2013 Jun 13.
Raman-seed pulse amplification in a one-dimensional backscattering geometry is investigated with the help of numerical simulations and analytical estimates. The significant dependence of the initial amplification on the pulse form is revisited on the basis of a three-wave interaction as well as a kinetic Vlasov model. It is shown how the short duration of the input seed pulse influences its subsequent behavior, depending on plasma density and pump strength. The evolution during a "start-up period," which has been observed earlier, can be explained analytically. In the nonlinear (pump depletion) regime, the pulse generated in the start-up period will be further amplified and may evolve into a self-similar π-pulse solution. The Vlasov code predicts algebraic growth in time of the seed amplitude, similar to the findings based on self-similar solutions of the three-wave-interaction model. An initially very narrow pulse is shown to grow more slowly than an initially broad one.
借助数值模拟和解析估计,研究了一维背散射几何结构中的拉曼种子脉冲放大。基于三波相互作用以及动力学弗拉索夫模型,重新审视了初始放大对脉冲形式的显著依赖性。结果表明,输入种子脉冲的短持续时间如何根据等离子体密度和泵浦强度影响其后续行为。早期观察到的 “启动期” 内的演化过程可以通过解析方法进行解释。在非线性(泵浦耗尽) regime 中,启动期产生的脉冲将进一步放大,并可能演化为自相似的 π 脉冲解。弗拉索夫代码预测种子振幅随时间呈代数增长,这与基于三波相互作用模型自相似解的研究结果相似。结果表明,初始非常窄的脉冲比初始宽的脉冲增长得更慢。