I am a current PhD student at the Institute of Astronomy within the University of Cambridge, and a student of Churchill College. My research interests include the theory of black hole accretion discs, specifically the production and amplification of magnetic fields via the dynamo process. I study these systems through a mix of theory and simulation using the Adaptive Mesh Refinement (AMR) code Athena++.

In the future I plan to work towards self-consistent models and realistic simulations of AGN which include accretion disks, jets, and coronae — a true “unified theory” of AGN.

You can find a copy of my CV here: Download my CV