This code is to study Primordial Globular Clusters (pGCs) formation in Dark Matter Halos
The original version of this code is in Parkinson et. al. 2008 (https://ui.adsabs.harvard.edu/abs/2008MNRAS.383..557P/abstract)
Here we modify the code with our conditions of DM which can form pGCs, and then get the number of pGCs (*.f90 files).