Gaseous Dark Matter Detectors
arXiv:0905.3675 · doi:10.1088/1367-2630/11/10/105018
Abstract
Dark Matter detectors with directional sensitivity have the potential of yielding an unambiguous positive observation of WIMPs as well as discriminating between galactic Dark Matter halo models. In this article, we introduce the motivation for directional detectors, discuss the experimental techniques that make directional detection possible, and review the status of the experimental effort in this field.
19 pages, review on gaseous directional dark matter detectors submitted to New Journal of Physics
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Cited by in corpus (14)
- Directional detection as a strategy to discover Galactic Dark Matter
- Inelastic Dark Matter and DAMA/LIBRA: An Experimentum Crucis
- Directional recoil detection
- Search for Dark Matter with CRESST
- Gaseous and dual-phase time projection chambers for imaging rare processes
- Exclusion limits from data of directional Dark Matter detectors
- The median recoil direction as a WIMP directional detection signal
- Data acquisition electronics and reconstruction software for directional detection of Dark Matter with MIMAC
- Magnetic Inelastic Dark Matter: Directional Signals Without a Directional Detector
- Simulations of the 3-Dimensional Velocity Distribution of Halo Weakly Interacting Massive Particles for Directional Dark Matter Detection Experiments
- Particle detection and tracking with DNA
- Probing light WIMPs with directional detection experiments
- Directionality and head-tail recognition in the keV-range with the MIMAC detector by deconvolution of the ionic signal
- Recent Developments in Detector Technology