From particles to precision

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Authors: Rubén M. Cabezón, Domingo Garcı́a-Senz, Oliver Avril, Osman Seckin Simsek, Sebastian F. Keller, Axel S. Lechuga, Lucio Mayer, Ralf Stephan Klessen, Florina M. Ciorba
Cited by: 0
References: 35

Abstract

Context . The direct numerical simulation of subsonic turbulence with smoothed particle hydrodynamics (SPH) has traditionally been hampered by zeroth-order (E0) errors, inaccurate gradient evaluations, and excessive numerical dissipation. Aims . We aim to investigate whether a modern SPH formulation can overcome these challenges by comparing its results to those obtained with state-of-the-art non-SPH codes such as AREPO and GIZMO. Methods . We used the SPH-EXA code, a highly scalable, natively GPU-accelerated, state-of-the-art SPH code equipped with an integral-based gradient estimation, advanced artificial viscosity switches with a slope-limited reconstruction, a flexible family of pairing-resistant interpolation kernels, generalized volume elements, and improved handling of density contrasts, which maximizes Lagrangian compatibility. Results . Our results show that SPH-EXA accurately reproduces the Kolmogorov inertial range scaling in the subsonic regime with increasing resolution, closely matching the results of state-of-the-art non-SPH methods. We also identify accurate grad-h terms as critical: a noisy standard implementation can imprint spurious granulation in the density field once dissipation is sufficiently reduced. Conclusions . We demonstrate that, with appropriate methodological advances, SPH can achieve a level of fidelity in modeling subsonic turbulence that rivals the most advanced Eulerian and moving-mesh approaches.

Fields of Study & Subjects

Fluid Dynamics Simulations and Interactions Particle Dynamics in Fluid Flows Computer Graphics and Visualization Techniques

Publication details

Journal / source
Astronomy and Astrophysics
Publisher
EDP Sciences
Volume
710
Pages
A284–A284
Publication date
22 May 2026
Language
EN