Vid Iršič

Univerza v Ljubljani, Fakulteta za matematiko in fiziko

torek, 26. 5. 2009, ob 15h v F6

In the past few years cosmological simulations had rapidly advanced to a point where they became useful and powerful tool to constraint cosmological models. They can be used to study physics on variety of scales, from galaxy collisions to clusters and large-scale structure formation. In this talk I would like to present basic steps to run your own cosmological simulation and what physics can be constrained from the results.