Introduction to dark matter experiments
arXiv:1101.5205 · doi:10.1142/9789814327183_0014
Abstract
This is a set of four lectures presented at the Theoretical Advanced Study Institute (TASI-09) in June 2009. I provide an introduction to experiments designed to detect WIMP dark matter directly, focusing on building intuitive understanding of the characteristics of potential WIMP signals and the experimental techniques. After deriving the characteristics of potential signals in direct-detection experiments for standard WIMP models, I summarize the general experimental methods shared by most direct-detection experiments and review the advantages, challenges, and status of such searches (as of late 2009). Experiments are already probing SUSY models, with best limits on the spin-independent coupling below 10^-7 pb.
64 pages, 25 figures, based on lectures at 2009 Theoretical Advanced Study Institute in Elementary Particle Physics (TASI), Boulder, Colorado. This posted version benefits from some editing relative to the version in the published proceedings
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Cited by in corpus (21)
- The Waning of the WIMP? A Review of Models, Searches, and Constraints
- Dark matter direct-detection experiments
- The Waning of the WIMP: Endgame?
- Ring-like features in directional dark matter detection
- Dark Matter Direct Detection of Classical WIMPs
- DAMA vs. the annually modulated muon background
- Measurement of Muon Annual Modulation and Muon-Induced Phosphorescence in NaI(Tl) Crystals with DM-Ice17
- Particle detection at cryogenic temperatures with undoped CsI
- Anapole moment of the lightest neutralino in the cMSSM
- Orbital perturbations due to massive rings
- Sensitivity of alkali halide scintillating calorimeters with particle identification to investigate the DAMA dark matter detection claim
- A Minimal Model of Torsion Mediated Dark Matter
- Baryogenesis and Asymmetric Dark Matter from The Left-Right Mirror Symmetric Model
- The CYGNO experiment, a directional detector for direct Dark Matter searches
- Pandax-4T limits on mass in 3-3-1LHN model
- Analysis of defect formation in semiconductor cryogenic bolometric detectors created by heavy dark matter
- Characterisation of Dark Matter in Direct Detection Experiments: Singlino Versus Higgsino
- A Model of Neutrino Mass, Baryon Asymmetry, and Asymmetric Dark Matter with Dark Sector
- A Left-Right Mirror Symmetric Model: Common Origin of Neutrino Mass, Baryon Asymmetry and Dark Matter
- The Matter-Antimatter Asymmetry and Cold Dark Matter from The Left-Right Mirror Symmetric Model with The Global
- A Model of Asymmetric Hadronic Dark Matter and Leptogenesis