The mass power spectrum at sub-galactic scales as a constraint to dark matter properties

Details The mass power spectrum at sub-galactic scales as a constraint to dark matter properties The mass power spectrum at sub-galactic scales as a constraint to dark matter properties

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011rmxac..40...15g&link_type=abstract

XIII Latin American Regional IAU Meeting (Eds. W. J. Henney & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

Dark Matter, Galaxies: Halos

Scientific paper

We explore the possible constraints to the dark matter (DM) mass power spectrum amplitude at sub-galactic scales, with the aim to test the properties of DM particle candidates. We present preliminary results discussing the sensitivity of Solar System dynamics and dSph's wide binaries abundance to the small scale DM distribution. We also discuss possible future avenues.

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