Evolution of density profiles of dark matter halos

Astronomy and Astrophysics – Astrophysics

Scientific paper

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2 pages, 1 figure, contribution to the Proceedings of Rencontres Internationales de l'IGRAP, Clustering at High Redshift, Mars

Scientific paper

I apply the modified spherical infall model to test the dependence of the
shape of density profiles of dark matter halos on redshift. The model predicts
that the density profile of a halo of a given mass steepens with time and its
concentration parameter changes like c~1/(1+z_0)^2.

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