Understanding dark matter with Fermi and the CLUES numerical simulation

Details Understanding dark matter with Fermi and the CLUES numerical simulation Understanding dark matter with Fermi and the CLUES numerical simulation

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1223..119c&link_type=abstract

SCIENCE WITH THE NEW GENERATION OF HIGH ENERGY GAMMA-RAY EXPERIMENTS: Proceedings of the 7th Workshop on Gamma-Ray Physics in th

Physics

Astronomical Telescopes, Gamma-Ray Sources (Astronomical), Dark Matter, Galactic Centre, Baryons, X- And Gamma-Ray Telescopes And Instrumentation, Gamma-Ray, Dark Matter, Galactic Halo, Baryons

Scientific paper

N body numerical simulations of the Universe are a fundamental tool for the study of dark matter. Starting from a large scale simulation, we have performed two resimulations of a Local Group-like region with a higher resolution. In one of them, baryons have been included. This allows us to qualitatively and quantitatively study the effect of baryons in the distribution of dark matter. In this work, we present some results of our analysis of these simulations, which is aimed in particular to determine the effect of baryons on dark matter detectability by the Fermi Gamma Ray Telescope (FGST).

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