Research Projects

Explore my research projects in the field of astronomy and beyond.

Prolific Nitrogen Production and Metallicity Gradient in AGN Accretion Disk

Prolific Nitrogen Production and Metallicity Gradient in AGN Accretion Disk

Nov 2025 - Present
Prof. Douglas N.C. Lin, Dr. Tingtao Zhou, Jiamu Huang

Constructing an idealized diffusion model to show that multiple generation of stars leads to fast N-enrichment with an abundance gradient in the AGN disks. Image credit: ESO/WFI (Optical); MPIfR/ESO/APEX/A.Weiss et al. (Submillimeter); NASA/CXC/CfA/R.Kraft et al. (X-ray).

Migration of High-eccentricity Gas Giants on a Protoplanetary Disk

Migration of High-eccentricity Gas Giants on a Protoplanetary Disk

Jun 2025 - Present
Prof. Shude Mao, Prof. Shigeru Ida, Dr. Yaping Li

Conducting hydrodynamic simulations on gas giant migration on a protoplanetary disk by Athena++. Integrating migration laws from hydro simulations into REBOUNDx framework for effective dynamic simulation on complex planetary systems. Image credit: spacedaily.com.

Launching Mechanism for Freely-Floating Planets from Host Stars with Close-in Planets

Launching Mechanism for Freely-Floating Planets from Host Stars with Close-in Planets

May 2025 - Sep 2025
Prof. Douglas N.C. Lin, Prof. Shigeru Ida, Dr. Xiaochen Zheng, Prof. Shude Mao

Conducted REBOUNDx simulation to test the influence of tides on the production of FFPs from the host stars with cometary companions and close-in planets. Deduced a theoretical model to explain the tide influence on such systems. Image credit: the European Southern Observatory.

Planet Migration in Protoplanetary Disks with Rims

Planet Migration in Protoplanetary Disks with Rims

May 2025 - Nov 2025
Prof. Douglas N.C. Lin, Dr. Yaping Li, Prof. Shude Mao

Conducted simulations on migration of planets on a protoplanetary disk with rim shaped dead zone by Athena++. Theoretically analyzed the migration mechanism as the competition between torques in planet-disk interaction, and further explained the distinct migration behaviors of hot Jupiters and super-Earths. Image credit: Center for Astrophysics | Harvard & Smithsonian.

Comet Shower at the Pliocene-Pleistocene Transition Triggered by a Stellar Fly-by

Comet Shower at the Pliocene-Pleistocene Transition Triggered by a Stellar Fly-by

Sep 2024 - Feb 2025
Prof. Abraham Loeb, Dr. Morgan Macleod

Conducted numerous simulations on Oort cloud and stellar flyby by REBOUND package, revealed and explained the Oort cloud behaviors of a possible comet shower 3 Myr ago during the flyby of star HD7977, analyzed comet duration, intensity, and its impact on the ancient Earth. Collected geographic evidence of craters and comet components, revealing that this comet shower could be the cause of the Pliocene-Pleistocene Transition. Image credit: AAAS | Science.

Stability of the Solar System by Impacts from Free Floating Planets to Stellar Flybys

Stability of the Solar System by Impacts from Free Floating Planets to Stellar Flybys

Oct 2023 - Jun 2024
Prof. Shude Mao

Explored flybys' impact on planetary systems (solar system) by REBOUND, computatively and theoretically revealed the relationship between system collapse probability and intrusion perihelion distance on a large parameter space. Photo: NASA Hubble Telescope. Image credit: solarsystemandgalaxy3.blogspot.com.

HST to JWST Super-Resolution Based on ControlNet

HST to JWST Super-Resolution Based on ControlNet

Feb 2025 - Jun 2025
Prof. Zheng Cai, Fujiang Yu

Using convolution techniques to down-resolve the JWST images to the HST resolution, and validating the database using ControlNet-based machine learning.