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Minimum entropy production closure of the photo-hydrodynamic equations for radiative heat transfer

机译:光动力学方程的最小熵产生闭包   用于辐射传热

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摘要

In the framework of a two-moment photo-hydrodynamic modelling of radiationtransport, we introduce a concept for the determination of effective radiationtransport coefficients based on the minimization of the local entropyproduction rate of radiation and matter. The method provides the nonequilibriumphoton distribution from which the effective absorption coefficients and thevariable Eddington factor (VEF) can be calculated. The photon distributiondepends on the frequency dependence of the absorption coefficient, in contrastto the distribution obtained by methods based on entropy maximization. Thecalculated mean absorption coefficients are not only correct in the limit ofoptically thick and thin media, but even provide a reasonable interpolation inthe cross-over regime between these limits, notably without introducing any fitparameter. The method is illustrated and discussed for grey matter and for asimple example of non-grey matter with a two-band absorption spectrum. Themethod is also briefly compared with the maximum entropy concept.
机译:在辐射传输的两步光-流体动力学模型的框架内,我们引入了一种基于最小化辐射和物质的局部熵产生率来确定有效辐射传输系数的概念。该方法提供了非平衡光子分布,由此可以计算出有效吸收系数和可变爱丁顿因子(VEF)。与通过基于熵最大化的方法获得的分布相反,光子分布取决于吸收系数的频率依赖性。计算出的平均吸收系数不仅在光学厚介质和薄介质的极限中是正确的,而且甚至可以在这些极限之间的交叉范围内提供合理的插值,特别是无需引入任何拟合参数。图示和讨论了该方法,用于灰质物质和具有两波段吸收光谱的非灰质物质的简单示例。还将该方法与最大熵概念进行了简要比较。

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