Pelekanidis Antonios, Zhang Fengling, Eikema Kjeld S E, Witte Stefan
Advanced Research Center for Nanolithography, Science Park 106, 1098 XG Amsterdam, The Netherlands.
Department of Physics and Astronomy, Vrije Universiteit, De Boelelaan 1105, 1081 HV Amsterdam, The Netherlands.
ACS Photonics. 2025 Feb 28;12(3):1638-1649. doi: 10.1021/acsphotonics.4c02516. eCollection 2025 Mar 19.
Light beams carrying orbital angular momentum (OAM) can be generated in the extreme ultraviolet and soft X-ray spectra by means of high harmonic generation (HHG). In HHG, phase properties of the drive laser, such as curvature, aberrations, and topological charge, are upconverted to the harmonic beams and coherently added to the inherent dipole phase. The strong nonlinearity of the HHG process, combined with the rapid phase variations corresponding to large OAM values in these vortex beams, leads to a high sensitivity to small variations in the driving field. However, a study of the generation dynamics via an accurate reconstruction of multiwavelength OAM beams is challenging. Here we show full complex field measurements of multiple individual harmonics of the HHG vortex beams. By using spectrally resolved ptychographic wavefront sensing, we retrieve the high-resolution amplitude and phase profiles for harmonics 23 to 29 in parallel, enabling detailed multiwavelength beam reconstructions. We study the influence of generation conditions and drive laser aberrations on the resulting vortex fields by comparing measured fields to numerical simulations and retrieving the propagation conditions around the focus and the OAM content of the beams. Specifically, we find that the multimodal content of such vortex beams can significantly influence the propagation and field distributions in the focal region. Such a beam propagation analysis allows a prediction of the resulting attosecond pulse trains and associated attosecond light springs that can be generated under realistic driving conditions.
通过高次谐波产生(HHG),可以在极紫外和软X射线光谱中产生携带轨道角动量(OAM)的光束。在高次谐波产生过程中,驱动激光的相位特性,如曲率、像差和拓扑电荷,被上转换到谐波光束中,并相干地加到固有的偶极相位上。高次谐波产生过程的强非线性,再加上这些涡旋光束中与大OAM值相对应的快速相位变化,导致对驱动场的微小变化具有高灵敏度。然而,通过精确重建多波长OAM光束来研究产生动力学具有挑战性。在此,我们展示了高次谐波产生涡旋光束多个单独谐波的完整复场测量结果。通过使用光谱分辨的叠层成像波前传感技术,我们并行检索了第23至29谐波的高分辨率幅度和相位分布,从而实现了详细的多波长光束重建。我们通过将测量场与数值模拟进行比较,并检索焦点周围的传播条件和光束的OAM含量,研究了产生条件和驱动激光像差对所得涡旋场的影响。具体而言,我们发现这种涡旋光束的多模含量会显著影响焦区的传播和场分布。这样的光束传播分析能够预测在实际驱动条件下可能产生的阿秒脉冲序列以及相关的阿秒光弹簧。