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流体动力学起源的光学克尔时空暗块动力学

Optical Kerr Spatiotemporal Dark-Lump Dynamics of Hydrodynamic Origin.

作者信息

Baronio Fabio, Wabnitz Stefan, Kodama Yuji

机构信息

INO CNR and Dipartimento di Ingegneria dell'Informazione, Università di Brescia, Via Branze 38, 25123 Brescia, Italy.

Department of Mathematics, Ohio State University, Columbus, Ohio 43210, USA.

出版信息

Phys Rev Lett. 2016 Apr 29;116(17):173901. doi: 10.1103/PhysRevLett.116.173901. Epub 2016 Apr 27.

Abstract

There is considerable fundamental and applicative interest in obtaining nondiffractive and nondispersive spatiotemporal localized wave packets propagating in optical cubic nonlinear or Kerr media. Here, we analytically predict the existence of a novel family of spatiotemporal dark lump solitary wave solutions of the (2+1)D nonlinear Schrödinger equation. Dark lumps represent multidimensional holes of light on a continuous wave background. We analytically derive the dark lumps from the hydrodynamic exact soliton solutions of the (2+1)D shallow water Kadomtsev-Petviashvili model, inheriting their complex interaction properties. This finding opens a novel path for the excitation and control of optical spatiotemporal waveforms of hydrodynamic footprint and multidimensional optical extreme wave phenomena.

摘要

在光学立方非线性或克尔介质中获得非衍射和非色散的时空局域波包具有相当大的基础和应用价值。在此,我们通过解析预测了(2 + 1)维非线性薛定谔方程一类新型时空暗块孤波解的存在。暗块表示连续波背景上的多维光洞。我们从(2 + 1)维浅水卡多姆采夫 - 彼得维谢夫利模型的流体动力学精确孤子解中解析推导暗块,继承了它们复杂的相互作用特性。这一发现为激发和控制具有流体动力学特征的光学时空波形以及多维光学极端波现象开辟了一条新途径。

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