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通过光子与轨道角动量的非线性相互作用产生空心高斯光束。

Hollow Gaussian beam generation through nonlinear interaction of photons with orbital angular momentum.

机构信息

Photonic Sciences Lab., Physical Research Laboratory, Ahmedabad 380009, Gujarat, India.

Indian Institute of Technology-Gandhinagar, Ahmedabad 382424, Gujarat, India.

出版信息

Sci Rep. 2016 Sep 1;6:32464. doi: 10.1038/srep32464.

Abstract

Hollow Gaussian beams (HGB) are a special class of doughnut shaped beams that do not carry orbital angular momentum (OAM). Such beams have a wide range of applications in many fields including atomic optics, bio-photonics, atmospheric science, and plasma physics. Till date, these beams have been generated using linear optical elements. Here, we show a new way of generating HGBs by three-wave mixing in a nonlinear crystal. Based on nonlinear interaction of photons having OAM and conservation of OAM in nonlinear processes, we experimentally generated ultrafast HGBs of order as high as 6 and power >180 mW at 355 nm. This generic concept can be extended to any wavelength, timescales (continuous-wave and ultrafast) and any orders. We show that the removal of azimuthal phase of vortices does not produce Gaussian beam. We also propose a new and only method to characterize the order of the HGBs.

摘要

空心高斯光束(HGB)是一类特殊的环形光束,不携带轨道角动量(OAM)。这种光束在原子光学、生物光子学、大气科学和等离子体物理等多个领域有广泛的应用。迄今为止,这些光束是通过线性光学元件产生的。在这里,我们展示了一种通过非线性晶体中的三波混频产生 HGB 的新方法。基于具有 OAM 的光子的非线性相互作用和非线性过程中 OAM 的守恒,我们实验产生了高达 6 阶和功率 >180mW 的超快 HGB,波长为 355nm。这个通用概念可以扩展到任何波长、时间尺度(连续波和超快)和任何阶数。我们表明,去除涡旋的角向相位不会产生高斯光束。我们还提出了一种新的、唯一的方法来表征 HGB 的阶数。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/50bd/5007482/50a8b4946f56/srep32464-f1.jpg

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