Research Interests

Galaxy-Halo Connection

Galaxies are born and raised in dark matter halos, so they are tightly related to each other. Previous research has established the primary galaxy-halo connection, which is known as the stellar mass-halo mass relation (SHMR), from which we infer the necessity of supernovae feedback and AGN feedback to suppress the conversion from baryon to stars in low-mass and high-mass halos, respectively. Nowadays, people start to pursue the secondary galaxy-halo connection, and I am one of them. The ultimate question in this regard is that

  • To what extent the properties of galaxies are shaped by their dark matter halos?

A brief introduction:

Related projects:

Dark Matter Halo

Dark matter halos are the building blocks of our Universe, and they can be characterized from three perspectives: The temporal dimension: the assembly of dark matter halos as a function of cosmic time, which can be described by halo merger trees. The intra-halo dimension: the spatial and kinematic structures of dark matter halos, such as halo density profile, halo shape, halo spin, and substructures. The inter-halo dimension: the spatial clustering of dark matter halos.

  • Which feature can capture the major diversity of dark matter halos from each perspective?
  • What are the relationships of these features from different perspectives?

A brief introduction:

Related projects:

Connect Structures across Cosmic Time

Galaxies at different redshifts are causally irrelevant but can be statistically linked together. Our strategy is to build the connection between galaxies and cosmic structures, such as dark matter halos and protoclusters, at different redshifts, and connect these structures across cosmic time using cosmological N-body simulations, which is more reliable and convergent than hydrodynamical galaxy formation simulations.

  • How to identify protoclusters from biased high-redshift surveys?
  • How to connect protoclusters at different redshifts?

A brief introduction:

Related projects:

Galaxy Quenching

Galaxy quenching refers to the transition from a active star forming state to the quiescent state for galaxies. Star formation is so important because the integration of the star formation rate is the total stellar mass we can observe in our Universe. Galaxy quenching is so important because it (partially) explains why some galaxies convert their baryons to stars very inefficiently, or why the conversion process stops. Galaxies quench due to multiple reasons, and they can be empirically categorized into two types: internal quenching and external quenching.

  • To what extent the quenching of galaxies is determined by the dark matter halos they live in?
  • What is the causal relation between the galaxy quenching and the morphology transformation?

Related projects: