Sum-frequency generation with modified anomalous vortex beams

IF 3.3 Q3 Physics and Astronomy
Results in Optics Pub Date : 2026-03-01 Epub Date: 2026-07-20 DOI:10.1016/j.rio.2026.101086
Bikash K. Das, Camilo Granados, Wenlong Gao, Stephan Fritzsche
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引用次数: 0

Abstract

Light beams carrying orbital angular momentum (OAM) provide an additional degree of freedom to control and manipulate light-matter interactions across different energy regimes. Precise control over the beam and dark-core sizes, while maintaining a high value of the topological charge (TC) is crucial for their applications in optical tweezing, optical communication, and microscopy. While perfect optical vortices were engineered to feature TC-independent intensity distribution, their generation method typically involves bulky experimental setup. Furthermore, their detection is non-trivial, as they are not propagation eigenmodes and thus do not maintain their perfect vortex structure during propagation. A more sophisticated beam configuration is the modified anomalous vortex (MAV) beam — a novel class of anomalous vortex beam engineered with controlled self-focusing characteristics. MAV beams are typically characterized by their TC, beam order, and a so-called modification parameter. For extremely high beam order and a unity modification parameter, the beam and dark-core sizes of MAV beams remain nearly independent of the TC. Despite such novel beam properties, their role in driving nonlinear optical phenomena remains largely untested. In this work, we investigate the sum-frequency generation driven by MAV beams. For this nonlinear process, we derive an analytical expression for the complex field amplitude of the sum-frequency beam at the waist plane. Furthermore, we study the evolution of the generated sum-frequency beam in free-space. We thoroughly discuss the underlying OAM selection rule, and analyze how different parameters of the input MAV beams, such as their TC, beam order, modification parameter, and wavelength affect the sum-frequency beam. Moreover, we compare both the power of the sum-frequency beam generated by fundamental MAV, traditional AV, and Laguerre–Gaussian vortex beams, as well as the corresponding conversion efficiency of the process.
修正反常涡旋光束的和频产生
携带轨道角动量(OAM)的光束提供了额外的自由度来控制和操纵不同能量状态下的光-物质相互作用。精确控制光束和暗芯尺寸,同时保持高的拓扑电荷(TC)值对于它们在光镊,光通信和显微镜中的应用至关重要。虽然完美的光学旋涡被设计成具有与tc无关的强度分布,但它们的产生方法通常需要庞大的实验装置。此外,它们的检测是非平凡的,因为它们不是传播本征模,因此在传播过程中不会保持完美的涡结构。一种更复杂的光束结构是改进的反常涡旋(MAV)光束,这是一种具有可控自聚焦特性的新型反常涡旋光束。MAV波束的典型特征是它们的TC、波束顺序和所谓的修正参数。对于极高的光束阶数和统一的修正参数,MAV光束的光束和暗核大小几乎与TC无关。尽管有这些新颖的光束特性,但它们在驱动非线性光学现象中的作用在很大程度上仍未经测试。在这项工作中,我们研究了由MAV波束驱动的和频产生。对于这一非线性过程,我们导出了和频波束在腰平面的复场幅值的解析表达式。此外,我们还研究了所产生的和频波束在自由空间中的演化。我们深入讨论了基本的OAM选择规则,并分析了输入MAV波束的不同参数,如其TC、波束阶数、修改参数和波长对和频波束的影响。此外,我们还比较了基本MAV、传统AV和拉盖尔-高斯涡旋光束产生的和频光束功率,以及相应过程的转换效率。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Results in Optics
Results in Optics Physics and Astronomy-Atomic and Molecular Physics, and Optics
CiteScore
2.50
自引率
0.00%
发文量
115
审稿时长
71 days
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