The phase-space structure of CDM halos and dark-matter direct detection experiments

Details The phase-space structure of CDM halos and dark-matter direct detection experiments The phase-space structure of CDM halos and dark-matter direct detection experiments

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..17...24h&link_type=abstract

Galaxy Evolution: Theory & Observations (Eds. Vladimir Avila-Reese, Claudio Firmani, Carlos S. Frenk & Christine Allen) Revista

Astronomy and Astrophysics

Astronomy

Dark-Matter

Scientific paper

Here we discuss some results from a high-resolution simulation of the formation of a cluster of galaxies in a Lambda CDM cosmology, which we scale down to a Milky Way size halo. We focus mostly on quantifying how much substructure is left over from the inhomogeneous growth of the halo, and how it may affect the signal in experiments aimed at detecting the dark matter particles directly.

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