2005/05/13 by U. Schwanke, Schwanke, U.
Physics and Astronomy · #Astrophysics (astro-ph) #Atomic and Subatomic Physics Research #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #Radioactive Decay and Measurement Techniques #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0505290
10 pages, Latex, seven eps figures, one ps figure, uses moriond.sty, to be published in the proceedings of the Moriond Conference "ElectroWeak Interactions and Unified Theories" 2005
arxiv created 2005/05/13 · openalex publication_date 2005/05/13 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
A number of signals involving charged cosmic rays and high-energy photons have been interpreted as being due to annihilating dark matter. This article provides an overview of the experimental evidence and discusses in particular detections of antiprotons and positrons in the cosmic radiation, the diffuse gamma-ray emission between 10 MeV and 100 GeV from the Milky Way, and the 511 keV annihilation radiation and the flux of very high-energy photons (>100 GeV) from the Galactic Centre.