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WIMP/NEUTRALINO DIRECT DETECTION

2004/02/02 by M. De Jesus, M. DE JÉSUS
Physics and Astronomy · #Dark Matter and Cosmic Phenomena #Particle physics theoretical and experimental studies #Quantum Chromodynamics and Particle Interactions #astro-ph

paper · pdf · doi:10.1142/s0217751x04019056

published as Int.J.Mod.Phys. A19 (2004) 1142 · 9 pages, Latex, 12 figures., Review talk presented at the XXIst International Symposium on Lepton and Photon Interactions at High Energies, 11-16 August 2003, FNAL, Batavia, Illinois, USA

arxiv created 2004/02/02 · openalex publication_date 2004/03/20 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

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.

Citations