Gamma-ray detection of particle dark matter

Details Gamma-ray detection of particle dark matter Gamma-ray detection of particle dark matter

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..587..479b&link_type=abstract

GAMMA 2001: Gamma-Ray Astrophysics 2001. AIP Conference Proceedings, Volume 587, pp. 479-483 (2001).

Astronomy and Astrophysics

Astrophysics

Dark Matter, Galactic Halo, Gamma-Ray, Observation And Data Reduction Techniques, Computer Modeling And Simulation

Scientific paper

Recent results from N-body simulations of structure formation indicate that galactic dark matter halos may have a clumpy structure, with the density profiles of halos and subhalos showing steep cusps near the center. These features imply that the detection of particle dark matter through gamma-rays from annihilations in the Galactic halo, or from the integrated effects of smaller subhalos out to moderate readshifts, may be a promising method to detect supersymmetric dark matter. .

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