Modeling dust dynamics in OpenGadget3 -- I. SPH implementation of the One-Fluid model
Giovanni Tedeschi-Prades, Til Birnstiel, Klaus Dolag, Barbara Ercolano, Mark Hutchison

TL;DR
This paper implements and tests an improved One-Fluid SPH model for dust-gas dynamics in astrophysics within OpenGadget3, enhancing stability, accuracy, and applicability across various complex flow scenarios.
Contribution
The study introduces specific improvements to the One-Fluid model in OpenGadget3, including time-dependent viscosity, conductivity, and a new dust diffusion treatment, validated through comprehensive benchmarks.
Findings
Model passes all benchmark tests successfully.
Enhanced diffusion term improves handling of high dust-to-gas ratios.
Model remains stable and accurate in complex astrophysical flows.
Abstract
Dust dynamics plays a critical role in astrophysical processes and has been modeled in hydrodynamical simulations using various approaches. Among particle-based methods like Smoothed Particle Hydrodynamics (SPH), the One-Fluid model has proven to be highly effective for simulating gas-dust mixtures. This study presents the implementation of the One-Fluid model in OpenGadget3, introducing improvements to the original formulation. These enhancements include time-dependent artificial viscosity and conductivity, as well as a novel treatment of dust diffusion using a pressure-like term. The improved model is tested using a suite of dust dynamics benchmark problems: DUSTYBOX, DUSTYWAVE, and DUSTYSHOCK, with the latter extended to multidimensional scenarios, as well as a dusty Sedov-Taylor blast wave. Additional tests include simulations of Cold Keplerian Disks, dusty protoplanetary disks, and…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Particle Dynamics in Fluid Flows · Astro and Planetary Science
