Simulation of thermal conductivity of rare gases by the stochastic method

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Abstract

One of the main successes of the kinetic theory of gases is the explicit calculation of the transport coefficients of rarefied gases. However, the greatest problems arise when calculating the thermal conductivity coefficient, especially for polyatomic gases. Also, when using different potentials, it is necessary to systematically calculate the so-called Ω-integrals, which in itself is a rather difficult task. For this reason, direct numerical molecular modeling of the processes of transfer of rarefied gases, in particular, the calculation of their transfer coefficients, is also relevant. A well-known method for such modeling is the molecular dynamics method. Unfortunately, until now this method is not available for modeling the processes of rarefied gas transfer. Under nor-mal conditions, the simulation cell should contain tens or even hundreds of millions of molecules during calculations. At the same time, the numerical implementation of the molecular dynamics method is accompanied by a systematic appearance of errors, which is the reason for the appearance of dynamic chaos. With this simulation, the true phase trajectories of the system under consideration cannot be obtained. Therefore, naturally, the idea of developing a method for modeling transport processes arises, in which phase trajectories are not calculated based on Newton's laws, but are simulated, and then are used to calculate any observables. In our works, we developed a method of stochastic molecular modeling (STM) of rarefied gas transfer processes, where this idea was implemented. The efficiency of the SMM method was demonstrated by calculating the coefficients of self-diffusion, diffusion, and viscosity of both monoatomic gases and polyatomic gases. At the same time, the possibility of modeling the most complex transfer process – the energy transfer process – has not yet been considered. This work aims to simulate the thermal conductivity coefficient by the SMM method. Both monoatomic (Ar, Kr, Ne, Xe) and polyatomic gases (CH4, O2) were considered.
用随机方法模拟稀有气体的导热性
气体动力学理论的主要成就之一是明确地计算了稀薄气体的输运系数。然而,最大的问题出现在计算导热系数时,特别是对于多原子气体。此外,当使用不同的势时,需要系统地计算所谓的Ω-integrals,这本身就是一项相当困难的任务。因此,稀薄气体传递过程的直接数值分子模拟,特别是其传递系数的计算,也是相关的。这种建模的一种众所周知的方法是分子动力学方法。不幸的是,到目前为止,这种方法还不能用于模拟稀薄气体的传递过程。在正常情况下,模拟细胞在计算时应包含数千万甚至数亿个分子。同时,分子动力学方法的数值实现伴随着系统误差的出现,这是动态混沌出现的原因。这种模拟不能得到系统的真实相轨迹。因此,自然产生了开发一种模拟输运过程的方法的想法,在这种方法中,相位轨迹不是根据牛顿定律计算的,而是模拟的,然后用于计算任何可观测值。在我们的工作中,我们开发了一种稀薄气体传递过程的随机分子建模(STM)方法,并在其中实现了这一想法。通过计算单原子气体和多原子气体的自扩散系数、扩散系数和粘度,证明了SMM方法的有效性。同时,还没有考虑对最复杂的传递过程——能量传递过程——进行建模的可能性。本工作旨在用SMM方法模拟热传导系数。考虑了单原子气体(Ar, Kr, Ne, Xe)和多原子气体(CH4, O2)。
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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