光子晶体光纤中拉曼诱导孤子与色散波在超连续谱产生后期的相互作用管理

R. Driben, F. Mitschke, N. Zhavoronkov
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引用次数: 0

摘要

我们通过实验和数值研究了不同输入峰功率的负预啁啾脉冲在PCF中的动力学特性,并由此产生了光谱展宽和超连续谱。经过几厘米的初始压缩阶段,输入脉冲对应于一个高阶孤子,裂变成多个基本孤子[2],同时发射非孤子辐射[3]。这些孤子的光谱通过拉曼诱发频移[4](RIF)向更长的波长移动,在光谱的红边产生光谱展宽。我们证明了强孤子发出的辐射可以被拖尾孤子吸收,改变它们的路径。这可以导致额外的孤子准弹性或准塑性碰撞,并在产生的超连续统的某些频谱区域增强功率,或者更有趣的是,在产生新的频率分量时。孤子与色散波的相互作用过程对可控的输入脉冲参数极为敏感。例如,初始啁啾参数的微小变化可以导致孤子之间的碰撞模式从准弹性到准塑性的变化。图1展示了一个在C = - 1.16时的塑性碰撞的例子,碰撞孤子合并成一个巨大的孤子波,并以大群速度传播。在此过程中产生了一个较强的光谱带,将SC光谱扩展到1500 nm以上。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Management of interactions between Raman induced solitons and dispersive waves in photonic crystal fibers at the advanced stage of supercontinuum generation
We have studied experimentally [1] and numerically the dynamics of negatively prechirped pulses with different input peak powers in PCF with resultant spectral broadening and supercontinuum generation. After the initial compression stage of a few cm, the input pulse, as it corresponds to a high order soliton, undergoes fission into multiple fundamental solitons [2] accompanied by emission of non-soliton radiation [3]. Spectra of these solitons are shifted toward longer wavelengths by Raman induced frequency shift [4] (RIF) producing spectral broadening at the red edge of the spectrum. We show that the radiation emitted by stonger solitons can be absorbed by trailing solitons, altering their path. This can lead to additional soliton quasi-elastic or quasi-plastic collisions and to an enhancement of the power in certain spectral regions of the generated supercontinuum or, even more interestingly, in the generation of new frequency components. The process of interaction of solitons with dispersive waves is extremely sensitive to manageable input pulse parameters. For example small variations in initial chirp parameter can result in variations of the collision mode between solitons from a quasi-elastic to a quasi-plastic [5]. Fig.1 demonstrates an example of a plastic collision at C = −1.16 when the colliding solitons combine into one giant solitary wave which keeps propagating at large group velocity. In the process a strong spectral band is generated, which extends the SC spectrum beyond 1500 nm.
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