Chi-Ting Chiang, C.N. Yang Institute for Theoretical Physics at Stony Brook University, "Simulating structure formation in different environments and the applications"
KICP seminar: Apr 20 @ 12PM, ERC 401
The observables of the large-scale structure such as galaxy number density generally depends on the density environment (of a few hundred Mpc). The dependence can traditionally be studied by performing gigantic cosmological N-body simulations and measuring the observables in different density environments.