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Direct Detection of non-baryonic Dark Matter

Published online by Cambridge University Press:  19 May 2006

G.A. Mamon ,
F. Combes ,
C. Deffayet ,
B. Fort  and
C. Goldbach
C. Goldbach*
Affiliation:
Institut d'Astrophysique de Paris, France
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Abstract

Leading candidates for non-baryonic Dark Matter are Weakly Interacting Massive Particles (WIMPs). The principles of WIMP direct detection and different search stategies are introduced. A review of experimental results is presented. The most promising projects for the future are surveyed.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 20: Mass Profiles and Shapes of Cosmological Structures , 2006 , pp. 209 - 216
Copyright
© EAS, EDP Sciences, 2006

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