Esteso Victoria, Carretero-Palacios Sol, Míguez Hernán
Institute of Materials Science of Seville , Consejo Superior de Investigaciones Cientı́ficas (CSIC)-Universidad de Sevilla (US) , Américo Vespucio 49 , 41092 Seville , Spain.
Departamento de Física de Materiales , Universidad Autónoma de Madrid , 28049 Madrid , Spain.
J Phys Chem Lett. 2019 Oct 3;10(19):5856-5860. doi: 10.1021/acs.jpclett.9b02030. Epub 2019 Sep 19.
We theoretically investigate the building of optical resonators based on the levitation properties of thin films subjected to strong repulsive Casimir-Lifshitz forces when immersed in an adequate medium and confronted with a planar substrate. We propose a design in which cavities supporting high Q-factor optical modes at visible frequencies can be achieved by means of combining commonly found materials, such as silicon oxide, polystyrene or gold, with glycerol as a mediating medium. We use the balance between flotation and repulsive Casimir-Lifshitz forces in the system to accurately tune the optical cavity thickness and hence its modes. The effects of other forces, such as electrostatic, that may come into play are also considered. Our results constitute a proof of concept that may open the route to the design of photonic architectures in environments in which dispersion forces play a substantial role and could be of particular relevance for devising novel microfluidic optical resonators.
我们从理论上研究了基于薄膜悬浮特性构建光学谐振器的方法。当薄膜浸入适当介质并与平面衬底相对时,会受到强排斥性卡西米尔 - 利夫希茨力作用。我们提出了一种设计方案,通过将常见材料(如氧化硅、聚苯乙烯或金)与甘油作为中介介质相结合,可以实现支持可见频率高Q因子光学模式的腔体。我们利用系统中浮力与排斥性卡西米尔 - 利夫希茨力之间的平衡来精确调整光学腔厚度及其模式。还考虑了可能起作用的其他力(如静电力)的影响。我们的结果构成了一个概念验证,可能为在色散力起重要作用的环境中设计光子架构开辟道路,并且对于设计新型微流控光学谐振器可能具有特别重要的意义。