Monitoring the evolution of optical coatings during thermal annealing with real-time, in situ spectroscopic ellipsometry

Stefano Colace, Shima Samandari, M. Granata, Alex Amato, M. Caminale, Christophe Michel, G. Gemme, Laurent Pinard, Maurizio Canepa, M. Magnozzi
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Abstract

Thermal annealing plays a key role in optimizing the properties of amorphous optical coatings. In the field of gravitational wave detection (GWD), however, the effects of annealing protocols on the interferometry mirror coatings have been explored primarily by ex post analysis. As a result, the dynamics of the coatings properties during annealing is still poorly known, potentially leading to suboptimal performance. Here, using real-time, in situ spectroscopic ellipsometry (SE) we have tracked the refractive index and thickness of a titania-tantala coating during controlled annealing. We have tested the material and the annealing protocol used in current GWD mirrors. The annealing cycle consisted of a heating ramp from room temperature to 500 °C, followed by a 10-hour plateau at the same temperature and the final cooling ramp. SE measurements have been run continuously during the entire cycle. Significant variations in the thickness and refractive index, which accompany the coating structural relaxation, have been recorded during the heating ramp. These variations start around 200 °C, slightly above the deposition temperature, and show an increased rate in the range 250-350 °C. A smaller, continuous evolution has been observed during the 10-hour high-temperature plateau. The results offer suggestions to modify the current annealing protocol for titania-tantala coatings, for example by increasing the time duration of the high-temperature plateau. They also suggest an increase in the substrate temperature at deposition. The approach presented here paves the way for systematic, real-time investigations to clarify how the annealing parameters shape the properties of optical coatings, and can be leveraged to define and optimize the annealing protocol of new candidate materials for GWD mirrors.
利用实时原位光谱椭偏仪监测热退火过程中光学镀膜的演变情况
热退火在优化非晶态光学镀膜性能方面发挥着关键作用。然而,在引力波探测(GWD)领域,退火协议对干涉镜涂层的影响主要是通过事后分析来探索的。因此,人们对退火过程中涂层性能的动态变化仍然知之甚少,这有可能导致性能不理想。在这里,我们使用实时原位光谱椭偏仪(SE)跟踪了受控退火过程中二氧化钛-钽涂层的折射率和厚度。我们测试了当前 GWD 反射镜使用的材料和退火协议。退火周期包括从室温加热到 500 °C,然后在相同温度下保持 10 小时,最后冷却。SE 测量在整个周期内连续进行。伴随着涂层结构的松弛,在加热斜坡期间记录到厚度和折射率的显著变化。这些变化从 200 °C 左右开始,略高于沉积温度,并在 250-350 °C 范围内呈现上升趋势。在 10 小时的高温高原期间,观察到了较小的连续变化。这些结果为修改当前的二氧化钛-钽涂层退火方案提供了建议,例如延长高温稳定阶段的时间。他们还建议提高沉积时的基底温度。本文介绍的方法为进行系统、实时的研究铺平了道路,以阐明退火参数如何影响光学镀膜的性能,并可用于确定和优化 GWD 镜新候选材料的退火方案。
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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