The effects of asymmetric dark matter on stellar evolution - I. Spin-dependent scattering
We model energy transport resulting from scattering events between nucleons and spin-dependent asymmetric dark matter
Publications
Predicting Orbital Properties Of High Velocity Stars Near The Galactic Center
We develop a 5-component Milky Way-like potential and model the orbits of high velocity stars disrupted via the Hills mechanism.
Raen, T. J. et al. 2015, Undergraduate Research Journal, Volume 1, University of Utah