Wigner measures of electromagnetic waves in heterogeneous bianisotropic media

IF 2.1 3区 物理与天体物理 Q2 ACOUSTICS Wave Motion Pub Date : 2024-02-08 DOI:10.1016/j.wavemoti.2024.103296
Jean-Luc Akian, Éric Savin
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Abstract

We study the propagation of high-frequency electromagnetic waves in randomly heterogeneous bianisotropic media with dissipative properties. For that purpose we consider randomly fluctuating optical responses of such media with correlation lengths comparable to the typical wavelength of the waves. Although the fluctuations are weak, they induce multiple scattering over long propagation times and/or distances such that the waves end up traveling in many different directions with mixed polarizations. We derive the dispersion and evolution properties of the Wigner measure of the electromagnetic fields, which describes their angularly-resolved energy density in this propagation regime. The analysis starts from Maxwell’s equations with general constitutive equations. We first ignore the random fluctuations of the optical response and obtain uncoupled transport equations for the components of the Wigner measure on the different propagation modes (polarizations). Then we use a multi-scale expansion of the Wigner measure to obtain the radiative transfer equations satisfied by these components when the fluctuations are no longer ignored. The radiative transfer equations are coupled through their collisional parts, which account for the scattering of waves by the random fluctuations and their possible changes in polarization. The collisional kernels describing these processes depend on the power and cross-power spectral densities of the fluctuations at the wavelength scale. The overall derivation is based on the interpretation of Wigner transforms and Wigner measures in terms of semiclassical pseudo-differential operators in their standard quantization.

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异质双向各向异性介质中电磁波的维格纳量度
我们研究了高频电磁波在具有耗散特性的随机异质各向同性介质中的传播。为此,我们考虑了这种介质的随机波动光学响应,其相关长度与波的典型波长相当。虽然波动很微弱,但它们会在较长的传播时间和/或距离上引起多重散射,从而使波最终以混合极化的方式沿多个不同方向传播。我们推导了电磁场的维格纳量度的色散和演化特性,它描述了这种传播机制下的角分辨能量密度。分析从带有一般构成方程的麦克斯韦方程开始。我们首先忽略光学响应的随机波动,得到不同传播模式(极化)上 Wigner 测量分量的非耦合传输方程。然后,当波动不再被忽略时,我们使用 Wigner 测量的多尺度扩展来获得这些分量所满足的辐射传递方程。辐射传递方程通过碰撞部分耦合,碰撞部分考虑了随机波动对波的散射及其可能的极化变化。描述这些过程的碰撞核取决于波长尺度上波动的功率和交叉功率谱密度。整体推导是基于对标准量子化半经典伪微分算子的维格纳变换和维格纳度量的解释。
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来源期刊
Wave Motion
Wave Motion 物理-力学
CiteScore
4.10
自引率
8.30%
发文量
118
审稿时长
3 months
期刊介绍: Wave Motion is devoted to the cross fertilization of ideas, and to stimulating interaction between workers in various research areas in which wave propagation phenomena play a dominant role. The description and analysis of wave propagation phenomena provides a unifying thread connecting diverse areas of engineering and the physical sciences such as acoustics, optics, geophysics, seismology, electromagnetic theory, solid and fluid mechanics. The journal publishes papers on analytical, numerical and experimental methods. Papers that address fundamentally new topics in wave phenomena or develop wave propagation methods for solving direct and inverse problems are of interest to the journal.
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