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Weakly Interacting Massive Particles (WIMPs), are a leading candidate for thedark matter that is observed to constitute ~25% of the total mass-energydensity of the Universe. The direct detection of relic WIMPs (those producedduring the early moments of the Universe's expansion) is at the forefront ofactive research areas in particle astrophysics with a numerous internationalexperimental collaborations pursuing this goal. This paper presents an overviewof the theoretical and practical considerations common to the design andoperation of direct detection experiments, as well as their unique features andcapabilities.

An Introduction to Dark Matter Direct Detection Searches & Techniques