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携带自扭矩或随时间变化的轨道角动量的圆偏振高次谐波光束。

Circularly Polarized High-Harmonic Beams Carrying Self-Torque or Time-Dependent Orbital Angular Momentum.

作者信息

de Las Heras Alba, San Román Julio, Serrano Javier, Plaja Luis, Hernández-García Carlos

机构信息

Grupo de Investigación en Aplicaciones del Láser y Fotónica, Departamento de Física Aplicada, Universidad de Salamanca, E-37008 Salamanca, Spain.

Unidad de Excelencia en Luz y Materia Estructuradas (LUMES), Universidad de Salamanca, Salamanca 37008, Spain.

出版信息

ACS Photonics. 2024 Oct 4;11(10):4365-4373. doi: 10.1021/acsphotonics.4c01320. eCollection 2024 Oct 16.

Abstract

In the rapidly evolving field of structured light, self-torque has been recently defined as an intrinsic property of light beams carrying time-dependent orbital angular momentum. In particular, extreme-ultraviolet (EUV) beams with self-torque, exhibiting a topological charge that continuously varies on the subfemtosecond time scale, are naturally produced in high-order harmonic generation (HHG) when driven by two time-delayed intense infrared vortex beams with different topological charges. Until now, the polarization state of such EUV beams carrying self-torque has been restricted to linear states due to the drastic reduction in the harmonic up-conversion efficiency with increasing the ellipticity of the driving field. In this work, we theoretically demonstrate how to control the polarization state of EUV beams carrying self-torque, from linear to circular. The extremely high sensitivity of HHG to the properties of the driving beam allows us to propose two different driving schemes to circumvent the current limitations to manipulate the polarization state of EUV beams with self-torque. Our advanced numerical simulations are complemented with the derivation of selection rules of angular momentum conservation, which enable precise tunability over the angular momentum properties of the harmonics with self-torque. The resulting high-order harmonic emission, carrying time-dependent orbital angular momentum with a custom polarization state, can expand the applications of ultrafast light-matter interactions, particularly in areas where dichroic or chiral properties are crucial, such as magnetic materials or chiral molecules.

摘要

在快速发展的结构光领域,自扭矩最近被定义为携带随时间变化的轨道角动量的光束的一种固有属性。特别是,具有自扭矩的极紫外(EUV)光束,其拓扑电荷在亚飞秒时间尺度上连续变化,当由两个具有不同拓扑电荷且有时间延迟的强红外涡旋光束驱动时,在高次谐波产生(HHG)过程中自然产生。到目前为止,由于随着驱动场椭圆率的增加,谐波上转换效率急剧降低,此类携带自扭矩的EUV光束的偏振态一直局限于线性状态。在这项工作中,我们从理论上证明了如何将携带自扭矩的EUV光束的偏振态从线性控制为圆形。HHG对驱动光束特性的极高灵敏度使我们能够提出两种不同的驱动方案,以规避当前在操纵携带自扭矩的EUV光束偏振态方面的限制。我们先进的数值模拟辅以角动量守恒选择规则的推导,这使得能够对具有自扭矩的谐波的角动量特性进行精确调谐。由此产生的高次谐波发射,携带具有定制偏振态的随时间变化的轨道角动量,可以扩展超快光与物质相互作用的应用,特别是在二向色性或手性特性至关重要的领域,如磁性材料或手性分子。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/24ec/11487711/a9836efbebd2/ph4c01320_0001.jpg

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