\section{Potential Applications}
This project could lead to the solution to a long-standing problem in stellar astrophysics. A tested, novel implementation for internal angular momentum transport is required to make quantitative predictions about the state of the stellar core before core collapse. The chemically homogeneous channel for the formation of BH-BH binary mergers relies on the amount of internal mixing and angular momentum transport in stellar interiors, so our work may also improve our quantitative understanding of potential aLIGO sources.

