INFALL: A code for calculating the mean initial and final density profiles around a virialized dark matter halo

Details INFALL: A code for calculating the mean initial and final density profiles around a virialized dark matter halo INFALL: A code for calculating the mean initial and final density profiles around a virialized dark matter halo

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ascl.soft07002b&link_type=abstract

Astrophysics Source Code Library, record ascl:1007.002

Astronomy and Astrophysics

Astrophysics

Scientific paper

Infall is a code for calculating the mean initial and final density profiles around a virialized dark matter halo. The initial profile is derived from the statistics of the initial Gaussian random field, accounting for the problem of peaks within peaks using the extended Press-Schechter model. Spherical collapse then yields the typical density and velocity profiles of the gas and dark matter that surrounds the final, virialized halo. In additional to the mean profile, ? profiles are calculated and can be used as an estimate of the scatter.

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