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Direct Detection of Nonbaryonic Dark Matter

2000/03/29 by L. Baudis, Laura Baudis, Baudis, Laura +3
Physics and Astronomy · #Astrophysics (astro-ph) #Atomic and Subatomic Physics Research #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #Radioactive Decay and Measurement Techniques #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0003434

18 pages, latex, 8 eps figures, requires iopconf1.sty. To appear in Proceedings of Beyond the Desert '99, Second International Conference on Physics beyond the Standard Model, Castle Ringberg, Tegernsee, Germany, 6-12 June 1999

arxiv created 2000/03/29 · openalex publication_date 2000/03/29 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

Weakly Interacting Massive Particles (WIMPs) are leading candidates for the dominant part of the mass density of the Universe. Here we will review direct WIMP detection techniques by giving examples of currently running experiments, and present the status of the most promising future projects.

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