Runs SWIFT with different Dark Matter halo profiles initialisations using the ICICLE code in python.
Returns snapshots, plot options over time for:
- Angular momentum
- Kinetic & Potential energies
- Density profiles
- Overdensity radii
- Spatial distribution
Usage goals: Investigate the influence of baryonic mass ejections on the galactic DM halo.
In specific: The DM mass loss fraction due to the change in the overdensity radii.