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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).

Science Results

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.

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inlist file 1

pre-MS to ZAMS evolution without rotation. ZAMS is reached when logL ~ logLh

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inlist file 2

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.

inlist file 2 - Read More…