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Backscattering and Nonparaxiality Arrest Collapse of Damped Nonlinear Waves

机译:阻尼非线性波的反向散射和非傍轴捕获崩溃

摘要

The critical nonlinear Schrodinger equation (NLS) models the propagation of intense laser light in Kerr media. This equation is derived from the more comprehensive nonlinear Helmholtz equation (NLH) by employing the paraxial approximation and neglecting the backscattered waves. It is known that if the input power of the laser beam (i.e., L(sub 2) norm of the initial solution) is sufficiently high, then the NLS model predicts that the beam will self-focus to a point (i.e.. collapse) at a finite propagation distance. Mathematically, this behavior corresponds to the formation of a singularity in the solution of the NLS. A key question which has been open for many years is whether the solution to the NLH, i.e., the 'parent' equation, may nonetheless exist and remain regular everywhere, in particular for those initial conditions (input powers) that lead to blowup in the NLS. In the current study, we address this question by introducing linear damping into both models and subsequently comparing the numerical solutions of the damped NLH (boundary-value problem) with the corresponding solutions of the damped NLS (initial-value problem). Linear damping is introduced in much the same way as done when analyzing the classical constant-coefficient Helmholtz equation using the limiting absorption principle. Numerically, we have found that it provides a very efficient tool for controlling the solutions of both the NLH and NHS. In particular, we have been able to identify initial conditions for which the NLS solution does become singular. whereas the NLH solution still remains regular everywhere. We believe that our finding of a larger domain of existence for the NLH than that for the NLS is accounted for by precisely those mechanisms, that have been neglected when deriving the NLS from the NLH, i.e., nonparaxiality and backscattering.
机译:临界非线性Schrodinger方程(NLS)可模拟强激光在Kerr介质中的传播。通过使用近轴近似并忽略反向散射波,可以从更全面的非线性亥姆霍兹方程(NLH)中得出该方程。众所周知,如果激光束的输入功率(即初始解的L(sub 2)范数)足够高,则NLS模型将预测该光束将自动聚焦到一个点(即崩溃)。在有限的传播距离在数学上,此行为对应于NLS解中奇点的形成。多年来一直悬而未决的关键问题是,NLH的解(即“父母”方程)是否可能仍然存在并且在各地都保持规则,特别是对于那些导致爆炸的初始条件(输入功率)而言。 NLS。在当前的研究中,我们通过将线性阻尼引入两个模型并随后将阻尼NLH(边值问题)的数值解与阻尼NLS(初始值问题)的相应解进行比较来解决这个问题。线性阻尼的引入方法与使用极限吸收原理分析经典常数系数亥姆霍兹方程时所采用的方法几乎相同。从数值上看,我们发现它为控制NLH和NHS的解决方案提供了非常有效的工具。特别是,我们已经能够确定NLS解决方案确实变得单一的初始条件。而NLH解决方案在任何地方仍然保持常规。我们认为,我们发现NLH的存在域比NLS的存在域更大的原因恰好是那些从NLH导出NLS时被忽略的机制,即非近轴性和反向散射。

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