Abstract

Essentially non-oscillatory (ENO) and weighted ENO (WENO) methods on equidistant Cartesian grids are widely used to solve partial differential equations with discontinuous solutions. However, stable ENO/WENO methods on unstructured grids are less well studied. We propose a high-order ENO method based on radial basis function (RBF) to solve hyperbolic conservation laws on general two-dimensional grids. The radial basis function reconstruction offers a flexible way to deal with ill-conditioned cell constellations. We introduce a smoothness indicator based on RBFs and a stencil selection algorithm suitable for general meshes. Furthermore, we develop a stable method to evaluate the RBF reconstruction in the finite volume setting which circumvents the stagnation of the error and keeps the condition number of the reconstruction bounded. We conclude with several challenging numerical examples in two dimensions to show the robustness of the method.

Highlights

  • Solving systems of hyperbolic conservation laws with high-order methods continues to attract substantial interest

  • A generalization of the finite volume method is the class of Discontinuous Galerkin (DG) finite element methods [7], for which it is necessary to add limiters to ensure non-oscillatory approximations [22]

  • There exist several approaches that combine radial basis function (RBF) with finite volume methods, e.g. a highorder weighted ENO (WENO) approach based on polyharmonics [1], a high-order WENO approach based on multiquadratics [6], a high-order RBF based CWENO method [21] and an entropy stable RBF based essentially non-oscillatory (ENO) method [20]

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Summary

Introduction

Solving systems of hyperbolic conservation laws with high-order methods continues to attract substantial interest.

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Finite Volume Methods
Standard Interpolation
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Interpolation of Cell-Averages
Stable RBF Evaluation for Fixed Number of Nodes
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Stability Estimate for RBF Coefficients
Stability Estimate for Polynomial Coefficients
Approximation by RBF Interpolation Augmented with Polynomials
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Numerical Examples
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Numerical Results
KPP Rotating Wave
Isentropic Vortex
Riemann Problem
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Shock Vortex Interaction
Double Mach Reflection
Conclusions
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Full Text
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