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具有时空轨道角动量的超快脉冲的单帧表征

Single-Frame Characterization of Ultrafast Pulses with Spatiotemporal Orbital Angular Momentum.

作者信息

Gui Guan, Brooks Nathan J, Wang Bin, Kapteyn Henry C, Murnane Margaret M, Liao Chen-Ting

机构信息

JILA and Department of Physics, University of Colorado and NIST, 440 UCB, Boulder, Colorado 80309, United States.

KMLabs Inc., 4775 Walnut Street, Suite 102, Boulder, Colorado 80301, United States.

出版信息

ACS Photonics. 2022 Aug 17;9(8):2802-2808. doi: 10.1021/acsphotonics.2c00626. Epub 2022 Jul 23.

DOI:10.1021/acsphotonics.2c00626
PMID:35996367
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC9389650/
Abstract

Light that carries spatiotemporal orbital angular momentum (ST-OAM) makes possible new types of optical vortices arising from transverse OAM. ST-OAM pulses exhibit novel properties during propagation, transmission, refraction, diffraction, and nonlinear conversion, attracting growing experimental and theoretical interest and studies. However, one major challenge is the lack of a simple and straightforward method for characterizing ultrafast ST-OAM pulses. Using spatially resolved spectral interferometry, we demonstrate a simple, stationary, single-frame method to quantitatively characterize ultrashort light pulses carrying ST-OAM. Using our method, the presence of an ST-OAM pulse, including its main characteristics such as topological charge numbers and OAM helicity, can be identified easily from the unique and unambiguous features directly seen on the raw data-without any need for a full analysis of the data. After processing and reconstructions, other exquisite features, including pulse dispersion and beam divergence, can also be fully characterized. Our fast characterization method allows high-throughput and quick feedback during the generation and optical alignment processes of ST-OAM pulses. It is straightforward to extend our method to single-shot measurement by using a high-speed camera that matches the pulse repetition rate. This new method can help advance the field of spatially and temporally structured light and its applications in advanced metrologies.

摘要

携带时空轨道角动量(ST - OAM)的光使得由横向轨道角动量产生的新型光学涡旋成为可能。ST - OAM脉冲在传播、透射、折射、衍射和非线性转换过程中表现出新颖的特性,吸引了越来越多的实验和理论关注与研究。然而,一个主要挑战是缺乏一种简单直接的方法来表征超快ST - OAM脉冲。利用空间分辨光谱干涉测量法,我们展示了一种简单、静态、单帧的方法来定量表征携带ST - OAM的超短光脉冲。使用我们的方法,可以从原始数据上直接看到的独特且明确的特征中轻松识别出ST - OAM脉冲的存在,包括其拓扑电荷数和轨道角动量螺旋度等主要特征,而无需对数据进行全面分析。经过处理和重建后,其他精细特征,包括脉冲色散和光束发散,也能够得到充分表征。我们的快速表征方法在ST - OAM脉冲的产生和光学对准过程中实现了高通量和快速反馈。通过使用与脉冲重复率匹配的高速相机,将我们的方法扩展到单次测量是很直接的。这种新方法有助于推动时空结构化光领域及其在先进计量学中的应用。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0264/9389650/9dad47887614/ph2c00626_0007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0264/9389650/811f4c4d0c33/ph2c00626_0003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0264/9389650/19e312ab4131/ph2c00626_0004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0264/9389650/aeb5a1610002/ph2c00626_0005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0264/9389650/50cd04239e3c/ph2c00626_0006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0264/9389650/9dad47887614/ph2c00626_0007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0264/9389650/811f4c4d0c33/ph2c00626_0003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0264/9389650/19e312ab4131/ph2c00626_0004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0264/9389650/aeb5a1610002/ph2c00626_0005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0264/9389650/50cd04239e3c/ph2c00626_0006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/0264/9389650/9dad47887614/ph2c00626_0007.jpg

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Spatiotemporal Vortex Pulses: Angular Momenta and Spin-Orbit Interaction.时空涡旋脉冲:角动量与自旋轨道相互作用
Phys Rev Lett. 2021 Jun 18;126(24):243601. doi: 10.1103/PhysRevLett.126.243601.
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