论文标题

谐振模式耦合近似,用于计算光子晶体平板的光谱。第二部分

Resonant mode coupling approximation for calculation of optical spectra of photonic crystal slabs. Part II

论文作者

Gromyko, Dmitrii A., Dyakov, Sergey A., Tikhodeev, Sergei G., Gippius, Nikolay A.

论文摘要

我们提出进一步开发谐振模式耦合近似,以根据散射矩阵计算堆叠周期性纳米结构的光谱。我们先前表明,鉴于两个子系统的谐振输入和输出向量以及背景散射矩阵,一个可以轻松地计算出包含两个子系统的组合系统。它使我们能够为组合系统编写谐振近似,并为典型计算问题加快计算加快计算。这种方法的主要缺点是,这种近似值中的背景矩阵被认为是恒定的,如果感兴趣的能量范围相对较宽,这并不总是足够的。本文的目的是通过利用更复杂的近似值来解决此问题。特别是,我们表明,对背景矩阵的能量依赖性校正项的考虑显着降低了共振能量的计算误差。在这里,我们首先考虑一个线性近似,尽管它不适合大能范围,但它被用作分段线性近似的基础,这使人们可以保持近似误差可忽略不计,只有几个样品点。此外,背景矩阵的插值允许一个几乎任意的大能量范围应用谐振模式耦合近似。我们还考虑了通过任意矩阵函数对背景矩阵的近似值,并提出了一种在这种情况下推导谐振杆的技术。此处描述的方法可被视为计算光谱堆叠系统的替代方法。

We propose further development of the resonant mode coupling approximation for the calculation of optical spectra of stacked periodic nanostructures in terms of the scattering matrix. We previously showed that given the resonant input and output vectors as well as background scattering matrices of two subsystems, one can easily calculate those for the combined system comprising two subsystems. It allows us to write a resonant approximation for the combined system and speed up calculation significantly for typical calculation problems. The main drawback of this approach is that the background matrix in such approximation was considered constant which is not always sufficient if the energy range of interest is relatively wide. The aim of this article is to solve this problem by utilizing more complicated approximations for the background matrices. In particular, we show that consideration of energy-dependent correction terms for the background matrices remarkably reduces the resonant energies' calculation error. Here we first consider a linear approximation, and although it is not suitable for large energy ranges, it is used as a base for a piecewise-linear approximation which allows one to keep the approximation error negligibly small with only a few sample points. Moreover, interpolation of the background matrices allows one to apply resonant mode coupling approximation in almost arbitrary large energy ranges. We also consider approximation of background matrices by an arbitrary matrix function and propose a technique to derive the resonant poles in this case. The methods described here could be considered as an alternative approach for calculation of optical spectra stacked systems.

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