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首页> 外文期刊>Journal of Quantitative Spectroscopy & Radiative Transfer >Minimum entropy production closure of the photo-hydrodynamic equations for radiative heat transfer
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Minimum entropy production closure of the photo-hydrodynamic equations for radiative heat transfer

机译:辐射传热的光流体动力学方程的最小熵产生闭合

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摘要

In the framework of a two-moment photo-hydrodynamic modelling of radiation transport, we introduce a concept for the determination of effective radiation transport coefficients based on the minimization of the local entropy production rate of radiation and (generally nongrey) matter. The method provides the nonequilibrium photon distribution from which the effective (variable) absorption coefficients and the variable Eddington factor (VEF) can be calculated. For a single band model, the photon distribution depends explicitly on the frequency dependence of the absorption coefficient. Without introducing artificial fit parameters, multi-group or multi-band concepts, our approach reproduces the exact results in both limits of optically thick (Rosseland mean) and optically thin (Planck mean) media, in contrast to the maximum entropy method. Also the results for general nonequilibrium radiation between the limits of diffusive and ballistic photons are reasonable. We conjecture that the reason for the success of our approach lies in the linearity of the underlying Boltzmann equation of the photon gas. The method is illustrated and discussed for grey matter and for a simple example of nongrey matter with a two-band absorption spectrum. The method 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中,我们引入了一个概念,该方法基于最小化辐射和(通常是非灰色的)物质的局部熵产生率来确定有效的辐射传输系数。该方法提供了非平衡光子分布,由此可以计算出有效(可变)吸收系数和可变爱丁顿因子(VEF)。对于单频带模型,光子分布明确取决于吸收系数的频率依赖性。与最大熵方法相比,在不引入人工拟合参数,多组或多频带概念的情况下,我们的方法可以在光学上较厚(Rosseland均值)和光学上较稀薄(普朗克均值)的极限值中再现精确的结果。对于一般的非平衡辐射,在扩散光子和弹道光子的极限之间的结果也是合理的。我们推测,该方法成功的原因在于光子气体的基本Boltzmann方程的线性。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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