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arXiv 1602.08464nlin.PS
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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 Spatio-Temporal Dark-Lump Dynamics of Hydrodynamic Origin

F. Baronio, S. Wabnitz, Y. Kodama

摘要:

在光学立方非线性或克尔介质中获得非衍射、非色散的时空局域波包具有重要的理论意义和应用价值。在这里,我们解析地预测了(2+1)维非线性薛定谔方程的一族时空暗块孤波解的存在性。黑色的块状物代表连续波背景上的多维光洞。我们从(2+1)维浅水Kadomtsev-Petviashvili模型的流体动力学精确孤子解中解析地导出了暗块,继承了它们复杂的相互作用性质.这一发现为激发和控制流体动力足迹的光学多维极端波现象开辟了一条新的途径。

英文摘要:

There is considerable fundamental and applicative interest in obtaining non-diffractive and non-dispersive spatio-temporal localized wave packets propagating in optical cubic nonlinear or Kerr media. Here, we analytically predict the existence of a novel family of spatio-temporal dark lump solitary wave solutions of the (2+1)D nonlinear Schrödinger equation. Dark lumps represent multi-dimensional 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 multidimensional extreme wave phenomena of hydrodynamic footprint.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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