About

If forced to define myself, I would say I am a computational and theoretical physicist, with a twist of an applied mathematician, with background in medical physics and electrical engineering. I try to organize my work so that I can dirty my hands with theory, computation and experiments (analysis), if possible. More than anything I consider myself a tool builder, but I like to think that I speak all three languages fluently enough to uniquely bridge many projects, especially considering the fluency in not only methods, but also domain knowledge, like physics, biology, maths, engineering and increasingly machine learning & AI.

I'm currently (for a few more months) a PhD candidate at the University of Rhode Island (advisor: Gaurav Khanna) and I am a Visiting Collaborator at the Princeton Plasma Physics Laboratory, but I live in the New York metropolitan area, where I moved when I started collaboration with the researchers from the Flatiron Institute researchers (co-advisor: Ore Gottlieb).

My doctoral work develops numerical methods for physical systems governed by partial differential equations (PDEs), and pipelines that turn sparse, noisy instrument data into quantitative physical images and maps. Across three projects the unifying thread is the same: building forward models of a physical system and the computational machinery to solve them, or to invert them against real measurements, at scale, on national high-performance computing (HPC) systems, with extensive use of GPU-accelerated codes.

Also: board member of the Polish Astrobiology Society, member of the Event Horizon Telescope Collaboration, and the dog mom of Channi - a miniature dachshund.

Current research

Past research is either published, posted on the blog, never progressed enough to earn it, or was never worth it.

Numerical methods for coupled PDEs in complex geometries

Well-balanced conservative finite-volume method on dynamical spacetimes

Developed a strictly flux-conservative finite-volume framework for the two-way coupled Einstein-Euler system, built on a new first-order hyperbolic formulation of Einstein’s equations and providing its first coupling to matter. Well-balanced to machine precision (Tolman-Oppenheimer-Volkoff equilibria), admissibility and hyperbolicity-preserving; demonstrates long-time neutron-star equilibrium and a controlled collapse to a black hole (Manuscript in preparation).

PDEs: Einsteingeometry ⇔ Eulerrelativistic fluid
Collapse of an unstable neutron star to a black hole
An unstable neutron star collapsing to a black hole: conserved density (left) and lapse (right).

Latest from the blog

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Selected publications

Contact

I'm happy to talk about collaborations, ideas, or just science. Email me at bukowieckan@gmail.com.

New York metropolitan area