Convectively Driven Three Dimensional Turbulence in Massive Star Envelopes: I. A 1D Implementation of Diffusive Radiative Transport

William Schultz, Lars Bildsten, Yan-Fei Jiang

Massive ($M>30$M${}_{\odot }$) stars exhibit luminosities that are near the Eddington-limit for electron scattering causing the increase in opacity associated with iron at $T\appro…