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
Dark matter searches: Technology and backgrounds
β Scribed by Priscilla B. Cushman
- Publisher
- Elsevier Science
- Year
- 2007
- Tongue
- English
- Weight
- 734 KB
- Volume
- 579
- Category
- Article
- ISSN
- 0168-9002
No coin nor oath required. For personal study only.
β¦ Synopsis
The current status of direct dark matter searches is reviewed, with special emphasis on the effect of various backgrounds to the sensitivity attainable by this technology. The current leader in sensitivity is the Cryogenic Dark Matter Search, now operating at the Soudan Underground Laboratory in Minnesota. The next generation of larger and more sensitive detectors will require ever more radiopure materials and access to screening facilities to ensure rapid turn-around in decisions based on material selection and fabrication modification. Recent surveys collected from the DUSEL working groups point to a tripling in screening needs, many of which require an overburden. Low background counting facilities should be established at existing underground sites and integration of their complementary strengths would ensure that new techniques in dark matter, solar neutrino, and neutrinoless double beta decay have the resources they need to build ton-scale detectors.
π SIMILAR VOLUMES
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).
The search for dark matter WIMPs is complementary to direct searches and accelerator searches. The status of present searches and prospects for the future are reviewed.
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