Changes of the SNAP resonator shape owing to mode energy dissipation

Arcadiy Novikov, Dmitry V. Kudashkin, Ilya D. Vatnik
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Abstract

The whispering gallery mode (WGM) optical microresonators formed on the optical fiber surface appear as a promising ultraprecise and ultralow loss technological platform (known as Surface Nanoscale Axial Photonics, SNAP) to create miniature optical devices including delay lines, signal processors, photonic sensors, optical frequency comb generators, etc. It is important to note that applications involving high intracavity power may face intense cavity heating and hence unwanted radius changes. Here we the heating effects in SNAP cavities both experimentally and numerically and reveal the changes in the mode structure induced by the heating due to whispering gallery mode energy dissipation.
模式能量耗散导致 SNAP 谐振器形状发生变化
在光纤表面形成的耳语画廊模式(WGM)光学微谐振器是一种前景广阔的超精密、超低损耗技术平台(称为表面纳米级轴向光子学,SNAP),可用于制造微型光学设备,包括延迟线、信号处理器、光子传感器、光频率梳发生器等。值得注意的是,涉及高腔内功率的应用可能会面临强烈的腔内加热,从而引起不必要的半径变化。在此,我们通过实验和数值方法研究了 SNAP 腔内的加热效应,并揭示了由于耳语廊模式能量耗散而导致的加热引起的模式结构变化。
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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