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锗纳米天线中的表面等离激元中红外三次谐波产生

Plasmonic mid-infrared third harmonic generation in germanium nanoantennas.

作者信息

Fischer Marco P, Riede Aaron, Gallacher Kevin, Frigerio Jacopo, Pellegrini Giovanni, Ortolani Michele, Paul Douglas J, Isella Giovanni, Leitenstorfer Alfred, Biagioni Paolo, Brida Daniele

机构信息

1Department of Physics and Center for Applied Photonics, University of Konstanz, 78457 Konstanz, Germany.

2School of Engineering, University of Glasgow, Rankine Building, Oakfield Avenue, Glasgow, G12 8LT UK.

出版信息

Light Sci Appl. 2018 Dec 12;7:106. doi: 10.1038/s41377-018-0108-8. eCollection 2018.

Abstract

We demonstrate third harmonic generation in plasmonic antennas consisting of highly doped germanium grown on silicon substrates and designed to be resonant in the mid-infrared frequency range that is inaccessible with conventional nonlinear plasmonic materials. Owing to the near-field enhancement, the result is an ultrafast, subdiffraction, coherent light source with a wavelength tunable between 3 and 5 µm, and ideally overlapping with the fingerprint region of molecular vibrations. To observe the nonlinearity in this challenging spectral window, a high-power femtosecond laser system equipped with parametric frequency conversion in combination with an all-reflective confocal microscope setup is employed. We demonstrate spatially resolved maps of the linear scattering cross section and the nonlinear emission of single isolated antenna structures. A clear third-order power dependence as well as mid-infrared emission spectra prove the nonlinear nature of the light emission. Simulations support the observed resonance length of the double-rod antenna and demonstrate that the field enhancement inside the antenna material is responsible for the nonlinear frequency mixing.

摘要

我们展示了在由生长在硅衬底上的高掺杂锗构成的等离子体天线中产生的三次谐波,该天线设计为在传统非线性等离子体材料无法达到的中红外频率范围内产生共振。由于近场增强,结果是一个超快、亚衍射的相干光源,其波长可在3至5微米之间调谐,并且理想地与分子振动的指纹区域重叠。为了在这个具有挑战性的光谱窗口中观察非线性,我们采用了配备参量频率转换的高功率飞秒激光系统,并结合全反射共焦显微镜设置。我们展示了单个孤立天线结构的线性散射截面和非线性发射的空间分辨图。明显的三阶功率依赖性以及中红外发射光谱证明了光发射的非线性性质。模拟结果支持了双杆天线观察到的共振长度,并表明天线材料内部的场增强是导致非线性频率混合的原因。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/3639/6290006/c5a17b6932b3/41377_2018_108_Fig1_HTML.jpg

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