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

被引:48
作者
Chaitanya, N. Apurv [1 ,2 ]
Jabir, M. V. [1 ]
Banerji, J. [1 ]
Samanta, G. K. [1 ]
机构
[1] Phys Res Lab, Photon Sci Lab, Ahmadabad 380009, Gujarat, India
[2] Indian Inst Technol Gandhinagar, Ahmadabad 382424, Gujarat, India
关键词
PROPAGATION; LIGHT;
D O I
10.1038/srep32464
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
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.
引用
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页数:6
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