Wimp/Neutralino Direct Detection

Details Wimp/Neutralino Direct Detection Wimp/Neutralino Direct Detection

2004-02-02

arxiv.org/abs/astro-ph/0402033v1

Int.J.Mod.Phys. A19 (2004) 1142

Astronomy and Astrophysics

Astrophysics

9 pages, Latex, 12 figures., Review talk presented at the XXIst International Symposium on Lepton and Photon Interactions at H

Scientific paper

10.1142/S0217751X04019056

The most popular candidate for non baryonic dark matter is the neutralino.
More than twenty experiments are dedicated to its direct detection. This review
describes the most competitive and promising experiments with different
detection techniques. The most recent results are presented with some prospects
for the near future.

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