2-D hydro-thermo-mechanical-chemical geodynamic numerical code with a focus on thermodynamic reactions in a two-phase model.
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Updated
Nov 2, 2026 - Julia
2-D hydro-thermo-mechanical-chemical geodynamic numerical code with a focus on thermodynamic reactions in a two-phase model.
UNLV Star & Planet Formation Group
Planet Formation in the Southwest +
Archived C++ simulation of planetesimal motion in a central stellar potential, with stochastic initial conditions and inelastic merger rules.
Figure and source code for the Streaming Instability Code Comparison Project
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