Simulating the Formation of Structure in the Universe

Mike Boylan-Kolchin (MPA) - Aug 27, 2009 at 12:10 pm

Numerical simulations of structure formation have become essential tools for studying cosmology and galaxy formation. I will describe some of the newest, highest resolution cosmological simulations and discuss how they are influencing our understanding of the formation and evolution of dark matter halos. I will also focus on the Milky Way as a testing ground for models of cosmology and galaxy formation. The wealth of available and forthcoming observational data will provide strong constraints on both luminous and dark matter in the Galaxy. I will discuss how combining this data with the latest generation of numerical simulations is advancing our knowledge of how galaxies form.

The seminar will be held in 544 Campbell Hall.

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