I am a theoretical and computational astrophysicist and an Assistant Professor at the Hong Kong Institute for Astronomy and Astrophysics (HKIAA) and the Department of Physics at The University of Hong Kong. Before joining HKU, I was a Postdoctoral Research Associate in the Department of Astronomy at the University of Wisconsin-Madison, working with Nick Stone, and 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.
Download my CV .
Star-disk coupling reshapes nuclear clusters, with consequences for tidal disruptions, changing-look AGN, and gravitational-wave sources.
Afterglow light curves in milliseconds, fast enough to make full MCMC parameter inference tractable.
EP241113a, an Einstein Probe transient with GRB-like energy but a slow, baryon-loaded jet: the long-sought prototype of a dirty fireball.
Close stellar flybys can eject pairs of planets that remain gravitationally bound, as JWST found in the Orion Nebula.
The misaligned spin of Sagittarius A* as evidence of a merger with another massive black hole about 9 billion years ago.
