My research focuses on the physical and chemical evolution of protoplanetary disks and the origins of planetary materials. Using numerical simulations, I investigate disk instabilities, planet–disk interactions, environmental perturbations, magnetohydrodynamics, and the evolution and transport of solids and volatile species. I aim to connect these physical models with astronomical observations and the meteoritic record to better constrain the processes governing planetary system formation and evolution.
I also develop machine-learning methods for analyzing astronomical observations, including identifying signatures of embedded planets, denoising interferometric data, and detecting anomalous structures and kinematics.