密度波动多尺度分析临界六氟化硫的输运性质

A. Oprisan, Dereck Morgado, David Dorf, Seth Zoppelt, S. Oprisan, I. Hahn, Y. Garrabos, C. Lecoutre-Chabot, D. Beysens
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引用次数: 0

摘要

在临界点附近的密度波动具有广泛的大小范围,仅受封闭容器边界的限制。如果我们把临界点附近的波动图像分解成不相交的空间尺度,就像把白光分解成窄带单色波一样,那它会是什么样子呢?每个空间尺度的标度规律是什么?在每个空间尺度上波动的松弛时间与原始图像中波动的动力学是如何相关的?纯流体在临界点附近的波动会导致不同的相分离模式,从而显著影响材料的性能。由于纯流体在临界温度附近的可压缩性发散,临界相在地球上的重量下坍塌。它限制了波动的空间范围和持续时间。在微重力条件下,浮力和对流受到抑制,在更接近临界点的地方观测临界状态的时间更长。局部密度波动引起光强度波动(所谓的“临界乳光”),我们使用国际空间站(ISS)上DECLIC (Dispositif pour l’etude de la Croissance et des Liquides criticals)设施的ALI (Alice-Like Instrumentation insert)对微重力临界点附近的六氟化硫(SF6)样品进行了记录。在距离临界温度200 μK以内的短时间内(记录时间约为173 s),我们确定了不同大小波动的有效扩散系数。对于经过临界温度的热淬火后立即在临界点附近记录的瞬态和非平稳数据,我们使用二维经验模式分解(BEMD)技术从原始图像中分离出各种大小的波动。采用基于傅立叶的动态差分显微镜(DDM)方法对正交和平稳的内禀模态函数(IMF)图像进行分析,提取波动相关时间。我们发现单个幂律指数代表每个IMF的结构因素。此外,每个中间散射函数(ISF)由波动的唯一松弛时间常数确定。我们发现波动的相关时间随着IMF的排序而增加,这表明小规模波动的相关时间最短。在BEMD框架内,可以从受瞬态现象影响的短数据集估计热物理性质。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Transport Properties of Critical Sulfur Hexafluoride From Multiscale Analysis of Density Fluctuations
Density fluctuations near critical points have a wide range of sizes limited only by the boundaries of the enclosing container. How would a fluctuating image near the critical point look if we could break it into disjoint spatial scales, like decomposing white light into narrow-band, monochromatic waves? What are the scaling laws governing each spatial scale? How are the relaxation times of fluctuations at each spatial scale related to the dynamics of fluctuations in the original image? Fluctuations near the critical point of pure fluids lead to different phase separation patterns, which significantly influence the materials’ properties. Due to the diverging compressibility of pure fluids near the critical temperature, the critical phase collapses under its weight on Earth. It limits both the spatial extent of fluctuations and their duration. In microgravity, the buoyancy and convection are suppressed, and the critical state can be observed much closer to the critical point for a more extended period. Local density fluctuations induce light intensity fluctuations (the so-called “critical opalescence”), which we recorded for a sulfur hexafluoride (SF6) sample near the critical point in microgravity using the ALI (Alice-Like Instrumentation insert) of the DECLIC (Dispositif pour l’Etude de la Croissance et des Liquides Critiques) facility on the International Space Station (ISS). From the short (approximately 173 s total recording) data set very near, within 200 μK from the critical temperature, we determined the effective diffusion coefficient for fluctuations of different sizes. For transient and non-stationary data recorded very near the critical point immediately after a thermal quench that steps through critical temperature, we separated fluctuations of various sizes from the original images using the Bidimensional Empirical Mode Decomposition (BEMD) technique. Orthogonal and stationary Intrinsic Mode Function (IMF) images were analyzed using the Fourier-based Dynamic Differential Microscopy (DDM) method to extract the correlation time of fluctuations. We found that a single power-law exponent represented each IMF’s structure factor. Additionally, each Intermediate Scattering Function (ISF) was determined by fluctuations’ unique relaxation time constant. We found that the correlation time of fluctuations increases with IMF’s order, which indicates that small-size fluctuations have the shortest correlation time. Estimating thermophysical properties from short data sets affected by transient phenomena is possible within the BEMD framework.
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