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Active flux methods for hyperbolic conservation laws -- flux vector splitting and bound-preservation: One-dimensional case

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arxiv 2405.02447 v2 pith:OCA6CZO4 submitted 2024-05-03 math.NA cs.NA

classification math.NAcs.NA
keywords methodsfluxpointcellfluxeshigh-ordermethodsplitting
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The active flux (AF) method is a compact high-order finite volume method that evolves cell averages and point values at cell interfaces independently. Within the method of lines framework, the point value can be updated based on Jacobian splitting (JS), incorporating the upwind idea. However, such JS-based AF methods encounter transonic issues for nonlinear problems due to inaccurate upwind direction estimation. This paper proposes to use flux vector splitting for the point value update, offering a natural and uniform remedy to the transonic issue. To improve robustness, this paper also develops bound-preserving (BP) AF methods for one-dimensional hyperbolic conservation laws. Two cases are considered: preservation of the maximum principle for the scalar case, and preservation of positive density and pressure for the compressible Euler equations. The update of the cell average in high-order AF methods is rewritten as a convex combination of using the original high-order fluxes and robust low-order (local Lax-Friedrichs or Rusanov) fluxes, and the desired bounds are enforced by choosing the right amount of low-order fluxes. A similar blending strategy is used for the point value update. Several challenging benchmark tests are conducted to verify the accuracy, BP properties, and shock-capturing ability of the methods.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Bound preserving {P}oint-{A}verage-{M}oment {P}olynomi{A}l-interpreted ({PAMPA}) on polygonal meshes

    math.NA 2025-02 conditional novelty 6.0 of 10

    A new bound-preserving PAMPA scheme for hyperbolic conservation laws on polygonal meshes is presented, with a proof outline and an eigenvalue-based coefficient formula for the Euler equations.

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