宽带极端紫外线旋束的生成动力学
Antonios Pelekanidis1,2, Fengling Zhang1,2, Kjeld S E Eikema1,2
1Advanced Research Center for Nanolithography, Science Park 106, 1098 XG Amsterdam, The Netherlands.
概括
研究人员精确测量了由高波生成 (HHG) 产生的多波长轨道角动量 (OAM) 束. 这种先进的技术揭示了驱动激光器的缺陷如何影响OAM光束特性和传播动态.
科学领域:
- 量子光学是一种量子光学.
- 激光物理 激光物理
- 在一秒钟的科学.
背景情况:
- 高波生成 (HHG) 能够产生具有轨道角运动量 (OAM) 的极紫外线和软X射线光束.
- 驱动激光器的相位属性与固有的双极相位一起被打印在HHG光束上.
- HHG的非线性性质和OAM光束的快速相变化会对驾驶场产生高灵敏度.
研究的目的:
- 克服了从HHG.准确重建多波长OAM光束的挑战.
- 为了研究产生条件和驱动激光偏差对束属性的影响.
- 为了使详细的多波长光束重建能够理解OAM生成动态.
主要方法:
- 在HHG束中对单个波 (23-29) 进行全复杂场测量.
- 应用光谱分辨率的图形波面传感用于高分辨率的振幅和相位检索.
- 实验测量与数值模拟进行比较,以分析光束传播和OAM含量.
主要成果:
- 对多个波的高分辨率振幅和相位配置文件并行检索.
- 该研究量化了产生条件和驱动激光偏差对产生的场的影响.
- 结果发现,多模式旋束的含量显著影响着焦点区域的传播和场分布.
结论:
- 精确的多波长重建HHG束是可以实现的.
- 了解光束传播和多模式内容对于控制OAM光束特征至关重要.
- 这种分析有助于在现实的条件下预测和生成每秒脉冲列车和光弹.
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