The Detectability of Angular Signatures of Galactic Dark Matter Substructure in the Diffuse Gamma-ray Background

Details The Detectability of Angular Signatures of Galactic Dark Matter Substructure in the Diffuse Gamma-ray Background The Detectability of Angular Signatures of Galactic Dark Matter Substructure in the Diffuse Gamma-ray Background

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008head...10.0205s&link_type=abstract

American Astronomical Society, HEAD meeting #10, #2.05

Astronomy and Astrophysics

Astronomy

Scientific paper

The majority of the gamma-ray emission from Galactic dark matter annihilation is likely to be detected as a contribution to the diffuse gamma-ray background. The Galactic dark matter distribution will induce characteristic anisotropies in the measured diffuse emission which may offer a unique method of extracting the dark matter signal. I will discuss angular features in the Galactic diffuse emission arising from the small-scale clumping of cold dark matter, and the detectability of these signatures with current and upcoming instruments.

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