MESA inlists and outputs for addition of non-nuclear energy to pair instability supernova progenitors

This archive collects the inlists and outputs for MESA stellar evolution models (MESA v.12778) of high initial mass stars, with zero initial metallicity and the addition of a non-nuclear energy source. Each file is labeled by the initial mass of the star (in solar masses) and the non-nuclear energy added (as a constant specific luminosity in erg/g/sec). The stellar masses we consider here surround the pair instability gap when no non-nuclear energy is added. By adding in non-nuclear energy, we can identify how effects like dark matter heating could impact the pair instability gap.