Directional detection of Dark Matter
arXiv:0811.2764 · doi:10.1142/S0217732309031569
Abstract
Among the many experimental techniques available, those providing directional information have the potential of yielding an unambiguous observation of WIMPs even in the presence of insidious backgrounds. A measurement of the distribution of arrival direction of WIMPs can also discriminate between Galactic Dark Matter halo models. In this article, I will discuss the motivation for directional detectors and review the experimental techniques used by the various experiments. I will then describe one of them, the DMTPC detector, in more detail.
17 pages, 11 postscript figures, mini-review submitted to Modern Physics Letters A (MPLA). Submitted to Modern Physics Letters A (MPLA)
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Cited by in corpus (17)
- Energy Dependence of Direct Detection Cross Section for Asymmetric Mirror Dark Matter
- Inelastic Dark Matter and DAMA/LIBRA: An Experimentum Crucis
- Directional recoil detection
- Can we overcome the neutrino floor at high masses?
- New Experimental Constraints in a New Landscape for Composite Dark Matter
- Direct Dark Matter Detection - A spin 3/2 WIMP candidate
- Disentangling Dark Matter Dynamics with Directional Detection
- Magnetic Inelastic Dark Matter: Directional Signals Without a Directional Detector
- Background Rejection in the DMTPC Dark Matter Search Using Charge Signals
- Background Rejection in the DMTPC Dark Matter Search Using Charge Signals
- On Diurnal and Annual Variations of Directional Detection Rates of Dark Matter
- An Attractive Scenario for Light Dark Matter Direct Detection
- Dark Matter in 3D
- Discretising the velocity distribution for directional dark matter experiments
- Simulations of the 3-Dimensional Velocity Distribution of Halo Weakly Interacting Massive Particles for Directional Dark Matter Detection Experiments
- Numerical Simulations of the Dark Universe: State of the Art and the Next Decade
- Detecting stable massive neutral particles through particle lensing