On the performances of standard and kinetic energy preserving time-integration methods for incompressible-flow simulations

Marco Artiano, Carlo De Michele, Francesco Capuano, Gennaro Coppola
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Abstract

The effects of kinetic-energy preservation errors due to Runge-Kutta (RK) temporal integrators have been analyzed for the case of large-eddy simulations of incompressible turbulent channel flow. Simulations have been run using the open-source solver Xcompact3D with an implicit spectral vanishing viscosity model and a variety of temporal Runge-Kutta integrators. Explicit pseudo-symplectic schemes, with improved energy preservation properties, have been compared to standard RK methods. The results show a marked decrease in the temporal error for higher-order pseudo-symplectic methods; on the other hand, an analysis of the energy spectra indicates that the dissipation introduced by the commonly used three-stage RK scheme can lead to significant distortion of the energy distribution within the inertial range. A cost-vs-accuracy analysis suggests that pseudo-symplectic schemes could be used to attain results comparable to traditional methods at a reduced computational cost.
关于不可压缩流模拟的标准和动能保存时间积分法的性能
针对不可压缩湍流通道流的大涡模拟,分析了 Runge-Kutta (RK) 时间积分器导致的动能保存误差的影响。模拟使用开源求解器 Xcompact3D 和隐式光谱消失粘度模型以及各种 Runge-Kutta 时间积分器进行。与标准 RK 方法相比,显式伪交映方案具有更好的能量保存特性。结果表明,高阶伪交映方法的时间误差明显减小;另一方面,对能量谱的分析表明,常用的三阶 RK 方案引入的耗散会导致惯性范围内的能量分布发生显著扭曲。成本-精度分析表明,使用伪交错方案可以在降低计算成本的同时获得与传统方法相媲美的结果。
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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