Investigate the large-scale structure properties and evolutions through cosmological hydro-simulations. Detail the connections between dark matter component with the luminous matters.
When hydro-dynamical simulations meet semi-analytical models.
With this project, I am seeking to push forward the boundary of hydro-dynamical simulations by making suggestions to observations.
See the project/workshop webpage for details.
This project includes three main comparison projects: the nIFTy clusters, the nIFTy galaxies and the nIFTy observations.
The project webpage is at here (http://gax.shao.ac.cn/ELUCID)
Numerical simulations is a powerful tool to distinguish these alternative cosmology models from each other and from LCDM.