Szczegóły seminarium

Data: 28.03.2023

Mirek Giersz (CAMK, Warsaw)

Star Cluster Evolution and BH population

First very briefly I will discuss the fundamental physical processes behind the different phases of star cluster evolution and then I will introduce the MOCCA code. In the next part of the talk, I will discuss the physical processes which shape the population of black holes in the star cluster environment.

Skip to content