Convergence of Roberts flow dynamos in Eulerian and Lagrangian codes
physics.comp-ph, astro-ph.CO, astro-ph.GA
Submitted: 2026-10-06
Updated: 2026-10-08
Terminology
Sources
- Sphenix: Smoothed Particle Hydrodynamics for the next generation of galaxy formation simulations
- Revisiting the ABC flow dynamo
- The inverse cascade and nonlinear alpha-effect in simulations of isotropic helical hydromagnetic turbulence
- Magnetic field evolution in simulations with Euler potentials
- The nature of mean-field generation in three classes of optimal dynamos
- Hydromagnetic turbulence in computer simulations
- Resistively controlled primordial magnetic turbulence decay
- Scale dependence of alpha effect and turbulent diffusivity
- Magnetic helicity dissipation and production in an ideal MHD code
- Astrophysical magnetic fields and nonlinear dynamo theory
- Extended theory of the Taylor problem in the plasmoid-unstable regime
- A Co-Scaling Grid for Athena++ II: Magnetohydrodynamics
- Cosmic-void observations reconciled with primordial magnetogenesis
- Memory effects in turbulent transport
- Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation
- Magnetic Prandtl number dependence of plasmoid-mediated reconnection
- A comparison of numerical schemes for driven subsonic MHD turbulence
- Mean-field dynamo action from delayed transport
- SWIFT: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications
- Towards robust simulations of the galactic dynamo: a cross-code comparison between Eulerian and Lagrangian schemes
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