The Structure of Our Galaxy's Dark Matter Halo

Details The Structure of Our Galaxy's Dark Matter Halo The Structure of Our Galaxy's Dark Matter Halo

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aps..ses.fd006d&link_type=abstract

American Physical Society, 72nd Annual Meeting of the Southeastern Section of the APS, November 10-12, 2005, abstract #FD.006

Physics

Scientific paper

Incomplete thermalization of the galactic halo leads to cold flows of dark matter particles, with peaks in their velocity distribution. I discuss the expected properties of these flows under the current concordance cosmology and their impact on dark matter detection, focussing on the recent search result from the Axion Dark Matter eXperiment (ADMX) collaboration.

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