Summary
Samuel Dunham is an astrophysics postdoctoral scholar with nine years of research experience, currently at Caltech and based in Ann Arbor, specializing in relativistic magnetohydrodynamics and numerical GRMHD methods. He develops and adapts hydrodynamics codes for general relativity, contributing to simulations of core-collapse supernovae and exploring 14-moment resistive GRMHD theory. His background includes modeling strong gravitational lenses and authoring research in lens mass distributions, reflecting a blend of theoretical, computational, and observational skills. Trained through rigorous programs at Vanderbilt, Fisk, and the University of Michigan, he pairs a strong academic record with hands-on code development for large-scale astrophysical simulations. Notably, he bridges detailed analytic modeling with practical code implementation—turning complex relativistic physics into reproducible simulation tools.
9 years of coding experience
2 years of employment as a software developer
B.S., Astronomy and Astrophysics, 3.72, B.S., Astronomy and Astrophysics, 3.72 at University of Michigan
Associate’s Degree, General Studies in Math and Natural Science, 3.80, Associate’s Degree, General Studies in Math and Natural Science, 3.80 at Washtenaw Community College
M.A., Physics, 4.0, M.A., Physics, 4.0 at Fisk University
Ph.D. (expected), Astronomy and Astrophysics, Ph.D. (expected), Astronomy and Astrophysics at Vanderbilt University
English, Spanish