A new differentiable MHD+self-gravity simulator combines a fifth-order finite-difference WENO scheme with a fourth-order semi-discretely energy-conserving self-gravity module.
A quantitative comparison of numerical methods for the compressible Euler equations: fifth-order WENO and piecewise-linear Godunov
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Per Astronomix ad Astra: High-Order Differentiable (Magneto)hydrodynamics with Energy-Conserving Self-Gravity
A new differentiable MHD+self-gravity simulator combines a fifth-order finite-difference WENO scheme with a fourth-order semi-discretely energy-conserving self-gravity module.