Metal diffusion in smoothed particle hydrodynamics simulations of dwarf galaxies
David John Williamson, Hugo Martel, and Daisuke Kawata

TL;DR
This study uses smoothed particle hydrodynamics simulations to explore how different metal diffusion models affect the chemical evolution and outflows in dwarf galaxies, revealing that diffusion strength influences gas metallicity and outflow efficiency.
Contribution
It systematically compares various metal diffusion models in dwarf galaxy simulations, highlighting their impact on metallicity distributions and outflow properties.
Findings
Stronger diffusion tightens the gas [O/Fe]-[Fe/H] distribution.
Diffusion suppresses low-metallicity star formation.
Metal outflows are strongly affected by diffusion strength.
Abstract
We perform a series of smoothed particle hydrodynamics simulations of isolated dwarf galaxies to compare different metal mixing models. In particular, we examine the role of diffusion in the production of enriched outflows, and in determining the metallicity distributions of gas and stars. We investigate different diffusion strengths, by changing the pre-factor of the diffusion coefficient, by varying how the diffusion coefficient is calculated from the local velocity distribution, and by varying whether the speed of sound is included as a velocity term. Stronger diffusion produces a tighter [O/Fe]-[Fe/H] distribution in the gas, and cuts off the gas metallicity distribution function at lower metallicities. Diffusion suppresses the formation of low-metallicity stars, even with weak diffusion, and also strips metals from enriched outflows. This produces a remarkably tight correlation…
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