WIMP annihilations are required to reproduce the correct dark matter abundance in the Universe. This process can occur in dense regions of our Galaxy such as the Galactic center, dwarf galaxies and other types of sub-haloes. High-energy g-rays are produced in dark matter particle collisions and can
Dark Matter searches with GLAST
β Scribed by E. Nuss
- Publisher
- Elsevier Science
- Year
- 2008
- Tongue
- English
- Weight
- 737 KB
- Volume
- 41
- Category
- Article
- ISSN
- 0273-1177
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π SIMILAR VOLUMES
Different techniques are currently competing in the direct search of Weakly Interacting Massive Particles (WIMP) dark matter, which consists in observing in the laboratory nuclear recoils due to impact of WIMPs from our galactic halo. As an introduction to this Dark Matter session, the experimental
After briefly recalling the evidence which suggests that the dark matter pervading the universe is nonbaryonic, we review the present searches for the best motivated particle candidates: axions, light neutrinos and Weakly Interacting Massive Particles (WIMPs).
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