Supersonic turbulence simulations with GPU-based high-order Discontinuous Galerkin hydrodynamics

TL;DR

This paper evaluates the performance of high-order Discontinuous Galerkin hydrodynamics simulations on supersonic turbulence using GPU acceleration, highlighting strengths and limitations in shock-dominated regimes.

Contribution

It demonstrates the applicability of GPU-accelerated high-order DG methods to supersonic turbulence, introducing shock regularization techniques and analyzing their effectiveness across Mach regimes.

Findings

DG performs well at moderate Mach numbers with shock regularization.

Accuracy diminishes in highly supersonic regimes due to shocks.

DG schemes have lower numerical dissipation advantageous in subsonic turbulence.

Abstract

We investigate the numerical performance of a Discontinuous Galerkin (DG) hydrodynamics implementation when applied to the problem of driven, isothermal supersonic turbulence. While the high-order element-based spectral approach of DG is known to efficiently produce accurate results for smooth problems (exponential convergence with expansion order), physical discontinuities in solutions, like shocks, prove challenging and may significantly diminish DG's applicability to practical astrophysical applications. We consider whether DG is able to retain its accuracy and stability for highly supersonic turbulence, characterized by a network of shocks. We find that our new implementation, which regularizes shocks at sub-cell resolution with artificial viscosity, still performs well compared to standard second-order schemes for moderately high Mach number turbulence, provided we also employ an additional projection of the primitive variables onto the polynomial basis to regularize the extrapolated values at cell interfaces. However, the accuracy advantage of DG diminishes significantly in the highly supersonic regime. Nevertheless, in turbulence simulations with a wide dynamic range that start with supersonic Mach numbers and can resolve the sonic point, the low numerical dissipation of DG schemes still proves advantageous in the subsonic regime. Our results thus support the practical applicability of DG schemes for demanding astrophysical problems that involve strong shocks and turbulence, such as star formation in the interstellar medium. We also discuss the substantial computational cost of DG when going to high order, which needs to be weighted against the resulting accuracy gain. For problems containing shocks, this favours the use of comparatively low DG order.