论文标题
极端拉曼红移:超快多模型非线性时空动力学,脉冲压缩和广泛可调的频率转换
Extreme Raman red shift: ultrafast multimode non-linear space-time dynamics, pulse compression, and broadly tunable frequency conversion
论文作者
论文摘要
如今,在超过1 $ $ $ m的波长下,超短高能脉冲在超快和强场物理学中的多种应用中都需要。迄今为止,对能量的波长可调性的主要答案仍然依赖于光学参数放大(OPA),通常需要多个和复杂的阶段,可能具有不完善的光束质量,并且转化效率有限,将其转化为一个扩增的波。在这项工作中,我们提出了一种完全不同的策略,以实现节能且可扩展的激光频率变速杆。这取决于在充满氮的空心核纤维(HCF)中长长的繁殖距离内刺激的拉曼散射(SRS)提供的连续红移。我们显示了从1030 nm到1730 nm的激光波长的连续可调节性,转化效率高于70%和远光灯质量。高度不对称的光谱拓宽是由HCF高阶模式之间的时空非线性相互作用引起的,可以轻易地用于产生脉冲(〜20 fs),比泵质量(〜200 fs)的脉冲(〜20 fs)明显短,并且脉冲能量可以进一步扩展到米尔小岛的紧张局部。我们设想,这种技术再加上新兴的高功率YB激光技术,有可能回答对近IR中可调节的少数循环源对高能多-TW的需求的不断增长。
Ultrashort high-energy pulses at wavelengths longer than 1 $μ$m are nowadays desired for a vast variety of applications in ultrafast and strong-field physics. To date, the main answer to the wavelength tunability for energetic, broadband pulses still relies on optical parametric amplification (OPA), which often requires multiple and complex stages, may feature imperfect beam quality and has limited conversion efficiency into one of the amplified waves. In this work, we present a completely different strategy to realize an energy-efficient and scalable laser frequency shifter. This relies on the continuous red shift provided by stimulated Raman scattering (SRS) over a long propagation distance in nitrogen-filled hollow core fibers (HCF). We show a continuous tunability of the laser wavelength from 1030 nm up to 1730 nm with conversion efficiency higher than 70% and high beam quality. The highly asymmetric spectral broadening, arising from the spatiotemporal nonlinear interplay between high-order modes of the HCF, can be readily employed to generate pulses (~20 fs) significantly shorter than the pump ones (~200 fs) with high beam quality, and the pulse energy can further be scaled up to tens of millijoules. We envision that this technique, coupled with the emerging high-power Yb laser technology, has the potential to answer the increasing demand for energetic multi-TW few-cycle sources tunable in the near-IR.