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Effects of Rotation on the Minimum Mass of Primordial Progenitors of Pair-instability Supernovae

Chatzopoulos, E.; Wheeler, J. Craig (2012)

Rotating 80 Msun zero metallicity model (Omega/Omega_crit at ZAMS = 0.5) with mass-loss

This folder contains the inlist and model files used for the full evolution of a rotating and magnetic 80 Msun, zero metallicity star with mass-loss included. The initial ZAMS rotation of the star is taken to be 50% of the critical Keplerian value. This model and other similar models were originally presented in Chatzopoulos & Wheeler (2012).

Rotating 80 Msun zero metallicity model (Omega/Omega_crit at ZAMS = 0.5) with mass-loss - Read More…