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Concentration, spin and shape of dark matter haloes as a function of the cosmological model:<i>WMAP</i>1, <i>WMAP</i>3 and<i>WMAP</i>5 results
We investigate the effects of changes in the cosmological parameters between the WMAP 1st, 3rd, and 5th year results on the structure of dark matter haloes. We use a set of simulations that cover 5 decades in halo mass ranging from the scales of dwarf galaxies (V_c ~30 km/s) to …