Rotating 80 Msun zero metallicity model (Omega/Omega_crit at ZAMS = 0.5) with mass-loss
Minimum masses of zero metallicity Pulsational Pair-Instability and full-fledged Pair-Instability SN progenitors with the effects of rotation and magnetic fields included in the evolution. Effects of the inclusion of mass-loss.
MESA version 3647 was used.
pre-MS to ZAMS evolution without rotation. ZAMS is reached when logL ~ logLh
Evolution from ZAMS to "pre-SN". In this work, as "pre-SN" we consider the case when a significant part of the star's core enters the dynamically unstable Gamma<4/3 pair-formation region at which point the models were mapped to a hydrodynamics code in the original work.