\section{Personnel}
Oishi will run the MHD simulations and produce the torque prescription. He will use a series of 1D and 2D simulations to identify areas of parameter space most relevant to post main-sequence stellar interiors, including $\nabla_{\mu}$. Once appropriate parameters are identified, he will run full 3D MHD simulations to construct torque and mixing models from $\nu_T$ and $\mathrm{Sc}$ respectively. Oishi is a founding member of the Dedalus collaboration and has significant experience with MHD turbulence in general and the MRI in particular. 

Cantiello will implement in MESA a 1D diffusion approximation of the  MRI angular momentum transport and chemical mixing results. He will then run stellar evolution models and test the results against, among others, asteroseismic observations. Cantiello is an expert in stellar evolution, asteroseismology, and a member of the  MESA council. 