Regarding the extension of metaplectic geometrical optics to modeling evanescent waves in ray-tracing codes

IF 2 3区 物理与天体物理 Q3 PHYSICS, FLUIDS & PLASMAS Physics of Plasmas Pub Date : 2024-08-09 DOI:10.1063/5.0221784
N. A. Lopez, R. Højlund, M. G. Senstius
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Abstract

Metaplectic geometrical optics (MGO) is a recently developed ray-tracing framework to accurately compute the wavefield behavior near a caustic (turning point or focal point), where traditional ray-tracing breaks down. However, MGO has thus far been restricted to having real-valued wavevectors. This is disadvantageous because often upon crossing a caustic from the “illuminated” region to the “shadow” region, two real-valued rays coalesce into one complex-valued ray corresponding to the transition from propagating to evanescent behavior. One can distinguish caustics as having either “illuminated shadows” or “proper shadows”—the former corresponds to when the shadow still contains real-valued rays (albeit in a fewer quantity than in the illuminated region), while the latter corresponds to when the shadow contains no real-valued rays. Here, by means of examples, we show how MGO can be used to model both types of shadows. First, for illuminated shadows, we show that MGO can actually be used “as is,” provided a corrected integration scheme is used compared to that proposed in the original references. This is then implemented and demonstrated in a recently developed MGO ray-tracing code. Second, we show that for proper shadows, the MGO formalism can still be used if the symplectic rotation matrix that removes caustics along rays is allowed to be complex-valued. In both cases, strong agreement is seen between the MGO and the exact solution, demonstrating the potential of MGO for improving the predictive capability of ray-tracing codes and laying the foundations for modeling more complicated evanescent phenomena such as tunneling with MGO.
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关于将元折射几何光学扩展到射线追踪代码中的蒸发波建模
元折射几何光学(MGO)是最近开发的一种光线追踪框架,用于精确计算苛点(转折点或焦点)附近的波场行为,而传统的光线追踪会在苛点附近出现故障。然而,到目前为止,MGO 还仅限于实值波向量。这样做的不利之处在于,从 "照明 "区域到 "阴影 "区域,在穿过苛刻区时,两条实值光线往往会凝聚成一条复值光线,从而实现从传播行为到蒸发行为的过渡。我们可以将凹陷区分为 "照明阴影 "或 "适当阴影"--前者对应于阴影中仍包含实值射线(尽管数量少于照明区域),而后者对应于阴影中不包含实值射线。在此,我们将通过实例说明如何使用 MGO 对这两种类型的阴影进行建模。首先,对于照明阴影,我们展示了 MGO 其实可以 "原封不动 "地使用,前提是与原始参考文献中提出的方案相比,我们使用了经过修正的积分方案。随后,我们在最近开发的 MGO 光线跟踪代码中实施并演示了这一方案。其次,我们还展示了对于适当的阴影,如果允许用于消除沿光线产生的凹凸的交点旋转矩阵为复值,那么 MGO 形式主义仍然可以使用。在这两种情况下,MGO 与精确解之间都有很强的一致性,这证明了 MGO 在提高光线跟踪代码预测能力方面的潜力,并为用 MGO 模拟隧道等更复杂的蒸发现象奠定了基础。
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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来源期刊
Physics of Plasmas
Physics of Plasmas 物理-物理:流体与等离子体
CiteScore
4.10
自引率
22.70%
发文量
653
审稿时长
2.5 months
期刊介绍: Physics of Plasmas (PoP), published by AIP Publishing in cooperation with the APS Division of Plasma Physics, is committed to the publication of original research in all areas of experimental and theoretical plasma physics. PoP publishes comprehensive and in-depth review manuscripts covering important areas of study and Special Topics highlighting new and cutting-edge developments in plasma physics. Every year a special issue publishes the invited and review papers from the most recent meeting of the APS Division of Plasma Physics. PoP covers a broad range of important research in this dynamic field, including: -Basic plasma phenomena, waves, instabilities -Nonlinear phenomena, turbulence, transport -Magnetically confined plasmas, heating, confinement -Inertially confined plasmas, high-energy density plasma science, warm dense matter -Ionospheric, solar-system, and astrophysical plasmas -Lasers, particle beams, accelerators, radiation generation -Radiation emission, absorption, and transport -Low-temperature plasmas, plasma applications, plasma sources, sheaths -Dusty plasmas
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