Simulating star formation.
I started with a simple spherical-collapse model for a school physics prize. Afterwards, I explored the Shu and Larson–Penston solutions independently.
Read the approach
First study: evolved collapsing spherical shells with a homologous velocity assumption; calculated shell radii, inferred densities and approximated temperatures from an ideal-gas model.
Independent continuation: investigated Shu inside-out collapse and Larson–Penston self-similar solutions, including infall behaviour, accretion rate and central mass growth.
I checked the outputs against the assumptions and tried to spot results that didn’t make physical sense.