Discretely nonlinearly stable weight-adjusted flux reconstruction high-order method for compressible flows on curvilinear grids

IF 3.8 2区 物理与天体物理 Q2 COMPUTER SCIENCE, INTERDISCIPLINARY APPLICATIONS
Alexander Cicchino , Siva Nadarajah
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引用次数: 0

Abstract

To achieve genuine predictive capability, an algorithm must consistently deliver accurate results over prolonged temporal integration periods, avoiding the unwarranted growth of aliasing errors that compromise the discrete solution. Provable nonlinear stability bounds the discrete approximation and ensures that the discretization does not diverge. Nonlinear stability is accomplished by satisfying a secondary conservation law, namely for compressible flows; the second law of thermodynamics. For high-order methods, discrete nonlinear stability and entropy stability, have been successfully implemented for discontinuous Galerkin (DG) and residual distribution schemes, where the stability proofs depend on properties of L2-norms. In this paper, nonlinearly stable flux reconstruction (NSFR) schemes are developed for three-dimensional compressible flow in curvilinear coordinates. NSFR is derived by merging the energy stable flux reconstruction (ESFR) framework with entropy stable DG schemes. NSFR is demonstrated to use larger time-steps than DG due to the ESFR correction functions, at the cost of larger error levels at design order convergence for equivalent degrees of freedom, while preserving discrete nonlinear stability. NSFR differs from ESFR schemes in the literature since it incorporates the FR correction functions on the volume terms through the use of a modified mass matrix. We also prove that discrete kinetic energy stability cannot be preserved to machine precision for quadrature rules where the surface quadrature is not a subset of the volume quadrature. This result stems from the inverse mapping from the kinetic energy variables to the conservative variables not existing for the kinetic energy projected variables. This paper also presents the NSFR modified mass matrix in a weight-adjusted form. This form reduces the computational cost in curvilinear coordinates because the dense matrix inversion is approximated by a pre-computed projection operator and the inverse of a diagonal matrix on-the-fly and exploits the tensor product basis functions to utilize sum-factorization. The nonlinear stability properties of the scheme are verified on a nonsymmetric curvilinear grid for the inviscid Taylor-Green vortex problem and the correct orders of convergence were obtained on a curvilinear mesh for a manufactured solution. Lastly, we perform a computational cost comparison between conservative DG, overintegrated DG, and our proposed entropy conserving NSFR scheme, and find that our proposed entropy conserving NSFR scheme is computationally competitive with the conservative DG scheme.
曲线网格上可压缩流的离散非线性稳定权重调整通量重构高阶方法
要实现真正的预测能力,算法必须在较长的时间积分周期内持续提供准确的结果,避免不必要的混叠误差增长损害离散解。可证明的非线性稳定性对离散近似进行了约束,并确保离散化不会发生偏离。非线性稳定性是通过满足次要守恒定律来实现的,即对于可压缩流;热力学第二定律。对于高阶方法,离散非线性稳定性和熵稳定性已成功应用于非连续伽勒金(DG)和残差分布方案,其稳定性证明取决于 L2 值的属性。本文针对曲线坐标下的三维可压缩流开发了非线性稳定通量重构(NSFR)方案。NSFR 是通过合并能量稳定通量重构(ESFR)框架和熵稳定 DG 方案而得出的。由于采用了 ESFR 修正函数,NSFR 可以使用比 DG 更大的时间步长,但在保持离散非线性稳定性的同时,等效自由度的设计阶收敛误差水平也会增大。NSFR 与文献中的 ESFR 方案不同,它通过使用修改后的质量矩阵,在体积项上加入了 FR 修正函数。我们还证明,对于曲面正交不是体积正交子集的正交规则,离散动能稳定性无法保持到机器精度。这一结果源于从动能变量到保守变量的反映射不存在于动能投影变量中。本文还以权重调整形式提出了 NSFR 修正质量矩阵。这种形式降低了曲线坐标的计算成本,因为密集矩阵反演是通过预先计算的投影算子和对角矩阵的逆来近似进行的,并利用张量乘积基函数来利用和因式分解。我们在非对称曲线网格上验证了该方案的非线性稳定性,用于解决不粘性泰勒-格林旋涡问题,并在曲线网格上获得了正确的收敛阶数,用于解决人造问题。最后,我们对保守 DG、过积分 DG 和我们提出的熵守恒 NSFR 方案进行了计算成本比较,发现我们提出的熵守恒 NSFR 方案在计算上与保守 DG 方案具有竞争力。
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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来源期刊
Journal of Computational Physics
Journal of Computational Physics 物理-计算机:跨学科应用
CiteScore
7.60
自引率
14.60%
发文量
763
审稿时长
5.8 months
期刊介绍: Journal of Computational Physics thoroughly treats the computational aspects of physical problems, presenting techniques for the numerical solution of mathematical equations arising in all areas of physics. The journal seeks to emphasize methods that cross disciplinary boundaries. The Journal of Computational Physics also publishes short notes of 4 pages or less (including figures, tables, and references but excluding title pages). Letters to the Editor commenting on articles already published in this Journal will also be considered. Neither notes nor letters should have an abstract.
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