by
Klaus Dolag(Universitäs Sternwarte, Muenchen, DE)
→
Europe/Rome
Sala Ovale (Villa Bazzoni)
Sala Ovale
Villa Bazzoni
Description
ABSTRACT:Upcoming astronomical surveys and instruments like Planck, SPT, PanStars,DES, Euclid, LOFAR, eRosita and many more will need a theoretical counterpart in form of simulations which follow the formation of cosmological structures in so far unaccomplished detail, taking into account enough physical processes to allow a self consistent comparison to observations at multiple wavelength and throughout the entire epoch of structure formation. I will report on preliminary results from a recent simulation campaign, where we followed the formation of cosmological structures in so far unaccomplished detail, performing a large set of cosmological, hydrodynamical simulations covering up to Gpc^3 volumes, taking into account enough physical processes (star- formation, chemical enrichment, AGN feedback) to allow a self consistent comparison to observations at multiple wavelength.
