This area focuses on the structure, origin, and evolution of the universe on the largest scales. Research spans from the early cosmic reionization and the intergalactic medium to galaxy formation and its connection with dark matter halos. Utilizing large-scale numerical simulations and multi-wavelength observations, the team aims to uncover the nature of dark matter and dark energy, and to reveal the complete evolutionary history of the universe from its infancy to the present day.
High-Energy and Time-Domain Astrophysics
This field explores the most violent transient phenomena and extreme physical processes in the cosmos. Research includes active galactic nuclei, black hole accretion, compact object mergers (gravitational waves), and supernova explosions. By integrating multi-messenger observations (electromagnetic waves, gravitational waves) with theoretical modeling, the team seeks to understand the physics behind these high-energy events and their impact on galaxy evolution
Exoplanets and Planet Formation
This area covers the entire journey of planetary systems, from cradle to home. It investigates dust growth, magnetic fields, and planetary formation environments within protoplanetary disks, while also searching for exoplanets and characterizing their atmospheres and orbital properties. Leveraging cutting-edge facilities like ALMA and JWST, the team works to unravel the formation mechanisms and diversity of planetary systems.
This discipline involves direct detection of fundamental cosmic particles through space-based experiments. The team is deeply involved in the Alpha Magnetic Spectrometer (AMS) experiment on the International Space Station, conducting precise measurements of cosmic-ray spectra and composition. This work aims to study the origin and propagation mechanisms of cosmic rays and to search for potential signals of dark matter, exploring high-energy astrophysical processes and new physics at the particle level.
