Dependence of Dust Formation on the Supernova Explosion

We investigate the properties, composition, and dynamics of dust formation growth for a diverse set core-collapse supernovae (CCSNe), varying progenitor mass, explosion energy, engine type. These explosions are evolved with 1-D Lagrangian hydrodynamics code out to several hundred days model ejecta as it expands cools. A multigrain nucleation is applied these results. find that higher energies lead an earlier onset formation, smaller grain sizes, larger silicate abundances. Further, we see nuclear burning during leads enhanced dust. Finally, build composite models from our suite predict efficiency CCSNe production function metallicity.