Summary
Cole Holcomb is a PhD astrophysicist and quantitative modeler with 11 years of research experience applying theoretical and computational methods to plasma physics and nuclear-reactive fluid dynamics. He specializes in multiscale modeling of many-body and stochastic systems, including cosmic ray transport, resonant wave-particle interactions, nonlinear plasma instabilities, and diffusion processes in interstellar and intergalactic media. Comfortable with both kinetic and magnetohydrodynamic frameworks, he brings a blend of analytical rigor and numerical simulation expertise honed through studies of supernovae and stellar explosions. Based in Hoboken, NJ, he pairs a dual background in physics and philosophy from UC Santa Cruz with a Princeton PhD, combining deep technical skill with a habit of questioning assumptions. Colleagues value his ability to translate complex physics into tractable computational experiments and robust data-driven insights.
11 years of coding experience
University of California Santa Cruz
Doctor of Philosophy - PhD, Astrophysics, Doctor of Philosophy - PhD, Astrophysics at Princeton University