基于GPU的大规模模拟计算薄膜动力学

Michael-Angelo Y.-H. Lam , Linda J. Cummings , Lou Kondic
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引用次数: 5

摘要

我们给出了扩散型四阶非线性偏微分方程的大规模模拟结果,这些方程在模拟基底上的薄流体膜动力学时通常会遇到。仿真基于交替方向隐式(ADI)方法,主要计算工作在GPU计算环境中进行。高效和准确的计算允许在三维(3D)的大计算域上进行模拟,并允许长的计算时间。我们将所开发的方法应用于纳米级厚度的流体薄膜的不稳定性这一特殊问题。大规模的模拟最大限度地减少了边界的影响,也允许模拟已发表实验中遇到的大小的域。因此,我们可以以前所未有的详细程度来分析不稳定性的发展。特别关注的是分析不稳定性发展的方式,特别是关于线性不稳定薄膜的去湿的旋节型和成核型之间的差异,以及亚稳薄膜的不稳定性。3D模拟允许考虑之前在2D几何结构中获得的一些最新结果[28]。一些新的结果包括使用傅立叶变换和拓扑不变量(Betti数)来区分旋节和成核类型的不稳定性的结果,精确描述导致卫星液滴形成的复杂过程,以及区分线性不稳定和亚稳状态下演化膜锋的形状。我们还讨论了向列型液晶和聚合物薄膜的模拟和可用实验结果之间的直接比较。
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Computing dynamics of thin films via large scale GPU-based simulations

We present the results of large scale simulations of 4th order nonlinear partial differential equations of diffusion type that are typically encountered when modeling dynamics of thin fluid films on substrates. The simulations are based on the alternate direction implicit (ADI) method, with the main part of the computational work carried out in the GPU computing environment. Efficient and accurate computations allow for simulations on large computational domains in three spatial dimensions (3D) and for long computational times. We apply the methods developed to the particular problem of instabilities of thin fluid films of nanoscale thickness. The large scale of the simulations minimizes the effects of boundaries, and also allows for simulating domains of the size encountered in published experiments. As an outcome, we can analyze the development of instabilities with an unprecedented level of detail. A particular focus is on analyzing the manner in which instability develops, in particular regarding differences between spinodal and nucleation types of dewetting for linearly unstable films, as well as instabilities of metastable films. Simulations in 3D allow for consideration of some recent results that were previously obtained in the 2D geometry [28]. Some of the new results include using Fourier transforms as well as topological invariants (Betti numbers) to distinguish the outcomes of spinodal and nucleation types of instabilities, describing in precise terms the complex processes that lead to the formation of satellite drops, as well as distinguishing the shape of the evolving film front in linearly unstable and metastable regimes. We also discuss direct comparison between simulations and available experimental results for nematic liquid crystal and polymer films.

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来源期刊
Journal of Computational Physics: X
Journal of Computational Physics: X Physics and Astronomy-Physics and Astronomy (miscellaneous)
CiteScore
6.10
自引率
0.00%
发文量
7
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