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Spectral interferometric microscopy reveals absorption by individual optical antennas from extinction phase

机译:光谱干涉显微镜显示单个光学天线从消光阶段吸收

摘要

In this thesis, we aim to understand how individual metallic nano-antennas can mediate the interaction of light with matter at optical frequencies. Firstly, we assess optical antennas in a focussed beam configuration and confirm recent theoretical predictions of extremely strong extinction by a dipole in a focussed beam. Our result reveals the practical limitation of focus - position related distortions in the extinction spectra due to the chromatic aberration of our microscopy system. From this insight, we develop a systematic approach to retrieve the longitudinal chromatic focal shift of our high NA microscope objectives using optical antennas. Secondly, we develop a novel spectral interferometric microscope (SIM) to measure over an octave the spectral transmission phase of an optical antenna. With this capability, we show how to extract the contributions of absorption and scattering to the total extinction from the transmission amplitude and phase of an antenna. As examples, we study the condition of critical coupling with gold discs and clarify the mechanism of Fano interference in a multi-particle ‘dimer’ antenna. Here, we were able to observe the residual absorption caused by Fano interference, which has not been observed before in experiments. Thirdly, we study a range of multi-resonant antenna configurations to expose the mechanism of SHG from metallic nano-structures. We show that the radiation phase of our optical antennas plays an important role in boosting SHG efficiency of an optical antenna. Finally, we assess the validity of the Rayleigh – Debye – Gans – Born approximation, which we used to assess the absorption and scattering of optical antennas. This involves direct methods to assess scattering and absorption in antennas. In particular, we investigate ultrashort laser pulse-induced heating of electrons in gold disc antennas.
机译:在本文中,我们旨在了解各个金属纳米天线如何在光频率下介导光与物质的相互作用。首先,我们评估聚焦波束配置中的光学天线,并确认最近的理论预测,即聚焦波束中的偶极子极强地消光。我们的结果揭示了由于我们的显微镜系统的色差导致的消光光谱中与焦点位置相关的畸变的实际局限性。根据这一见解,我们开发了一种系统的方法,可以使用光学天线来获取高NA显微镜物镜的纵向色聚焦偏移。其次,我们开发了一种新型的光谱干涉显微镜(SIM),可以在一个八度的范围内测量光学天线的光谱传输相位。借助此功能,我们将展示如何从天线的传输幅度和相位中提取吸收和散射对整个消光的贡献。作为示例,我们研究了与金盘的临界耦合条件,并阐明了多粒子“二聚体”天线中的Fano干扰机制。在这里,我们能够观察到由Fano干扰引起的残留吸收,这在实验之前还没有观察到。第三,我们研究了一系列多谐振天线配置,以从金属纳米结构中揭示SHG的机理。我们表明,我们的光学天线的辐射相位在提高光学天线的SHG效率方面起着重要作用。最后,我们评估了Rayleigh – Debye – Gans – Born近似的有效性,该近似用来评估光学天线的吸收和散射。这涉及评估天线中散射和吸收的直接方法。特别地,我们研究了金盘天线中超短激光脉冲诱导的电子加热。

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    Gennaro Sylvain Damien;

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  • 年度 2016
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