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Hauptverfasser: Owens, Nicholas, Wadsley, James, Wissing, Robert, Keller, Ben
Format: Preprint
Veröffentlicht: 2026
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Online-Zugang:https://arxiv.org/abs/2604.21983
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author Owens, Nicholas
Wadsley, James
Wissing, Robert
Keller, Ben
author_facet Owens, Nicholas
Wadsley, James
Wissing, Robert
Keller, Ben
contents In this paper, we introduce the first implementation of magnetic field-aligned hyperbolic diffusion for standard smoothed particle (magneto-)hydrodynamics (SPH), and its linear-exact gradient extension (LESPH). Hyperbolic diffusion differs from traditional parabolic methods by incorporating the physical characteristic speed of diffusing particles and is computationally faster. This work extends it to encompass field-aligned diffusion, linear-exact gradients, and linear reconstruction to limit dissipation. Several standard test problems are presented: a diffusing slab, diffusion around a ring, a Gaussian pulse, and the magneto-thermal instability (MTI). The MTI only grows for for LESPH with reconstruction, and not for SPH. Both LESPH and SPH remain stable while fully aligning diffusion to magnetic fields. LESPH is more accurate and converges faster in the L1 error norm. SPH and LESPH both see improvements when using when also using linear reconstruction. These methods apply to other diffusive transport such as cosmic rays, viscosity, or magnetic resistivity.
format Preprint
id arxiv_https___arxiv_org_abs_2604_21983
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Fast, Stable, and Physical: Hyperbolic, Magnetic Field-Aligned Diffusion in SPH
Owens, Nicholas
Wadsley, James
Wissing, Robert
Keller, Ben
Instrumentation and Methods for Astrophysics
In this paper, we introduce the first implementation of magnetic field-aligned hyperbolic diffusion for standard smoothed particle (magneto-)hydrodynamics (SPH), and its linear-exact gradient extension (LESPH). Hyperbolic diffusion differs from traditional parabolic methods by incorporating the physical characteristic speed of diffusing particles and is computationally faster. This work extends it to encompass field-aligned diffusion, linear-exact gradients, and linear reconstruction to limit dissipation. Several standard test problems are presented: a diffusing slab, diffusion around a ring, a Gaussian pulse, and the magneto-thermal instability (MTI). The MTI only grows for for LESPH with reconstruction, and not for SPH. Both LESPH and SPH remain stable while fully aligning diffusion to magnetic fields. LESPH is more accurate and converges faster in the L1 error norm. SPH and LESPH both see improvements when using when also using linear reconstruction. These methods apply to other diffusive transport such as cosmic rays, viscosity, or magnetic resistivity.
title Fast, Stable, and Physical: Hyperbolic, Magnetic Field-Aligned Diffusion in SPH
topic Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2604.21983