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I am a theoretical and computational astrophysicist, currently a Postdoctoral Research Associate in the Department of Astronomy at the University of Wisconsin-Madison, working with Nick Stone. In Fall 2026, I will join the Department of Physics at The University of Hong Kong and the Hong Kong Institute for Astronomy and Astrophysics (HKIAA) as an Assistant Professor. Previously, I was a Fellow at the Nevada Center for Astrophysics at UNLV, collaborating with Bing Zhang and Zhaohuan Zhu. I completed my PhD at Stony Brook University under Rosalba Perna.
I work on the fundamental dynamics of few-body gravitational systems in dense astrophysical environments. A particular focus is how stellar and compact-object populations evolve in AGN accretion disks, producing nuclear transients and gravitational-wave sources observable across the electromagnetic and gravitational-wave spectrum. I develop the open-source codes SpaceHub and VegasAfterglow for high-precision few-body integration and gamma-ray burst afterglow modeling.
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Download my CV .
PhD in Physics, 2022
Stony Brook University
MA in Physics, 2017
Stony Brook University
BS in Physics (Theoretical Physics), 2015
University of Science and Technology of China
Our Milky Way’s central black hole, Sagittarius A*, shows a peculiar spin orientation misaligned with the Galactic plane. We proposed that this misalignment is evidence of a past merger with another massive black hole roughly 9 billion years ago. This work provides a new window into the assembly history of supermassive black holes.
Published in Nature Astronomy (2024). Featured in Phys.org and ScienceDaily.
Star-disk coupling in Active Galactic Nuclei fundamentally reshapes nuclear cluster evolution. Objects on retrograde, high-inclination orbits experience eccentricity excitation as their vertical motion is damped. Once flattened, eccentricity is suppressed, leading to prograde, near-circular disk orbits. This process breaks steady-state assumptions and has wide-reaching consequences for tidal disruption events, changing-look AGN, and gravitational wave sources.
Published in MNRAS (2024).
JWST discovered Jupiter-Mass Binary Objects in the Orion Nebula—pairs of planetary-mass objects orbiting each other while floating freely in space. Using N-body simulations, we showed that close stellar flybys can eject two planets that remain gravitationally bound.
JuMBO formation: face-on (left) and edge-on (right) scattering.
Published in Nature Astronomy (2024). Featured in Quanta Magazine and Physics World.
To keep pace with the multi-wavelength data flooding in from gamma-ray bursts, I developed VegasAfterglow — a high-performance framework that pairs C++ speed with Python accessibility. It computes afterglow light curves in milliseconds, fast enough to make full MCMC parameter inference tractable, while capturing rich physics: forward and reverse shocks across relativistic and non-relativistic regimes, synchrotron self-Compton with Klein–Nishina corrections, and structured jets at arbitrary viewing angles.
Published in JHEAp (2026). Open source on GitHub.
I grew up in Chongqing, a city known for its dramatic mountainous terrain and traditional Chinese architecture in southwest China. I enjoy sketching the city’s iconic sites like Hongya Dong, which reflects both its cultural heritage and its striking urban landscape.

I recently revisited this sketch and used Google Gemini to add color and detail:

I picked up skiing during my PhD and quickly got hooked despite an early encounter with ski patrol. What started as a new challenge became a regular pursuit where steady improvement kept me coming back.
I’ve been training toward CSIA Level III certification, drawn to their systematic approach to skill development. Below is a clip from a pre-pandemic ski season with friends. I’m the one in the yellow pants.