A review on the discovery reach of Dark Matter directional detection
arXiv:1310.0214 · doi:10.1088/1742-6596/469/1/012013
Abstract
Directional detection of galactic Dark Matter offers a unique opportunity to identify Weakly Interacting Massive Particle (WIMP) events as such. Depending on the unknown WIMP-nucleon cross section, directional detection may be used to : exclude Dark Matter, discover galactic Dark Matter with a high significance or constrain WIMP and halo properties. We review the discovery reach of Dark Matter directional detection.
Proceedings of the 4th international conference on Directional Detection of Dark Matter (CYGNUS 2013), 10-12 June 2013, Toyama, Japan
References in corpus (13)
- Implication of neutrino backgrounds on the reach of next generation dark matter direct detection experiments
- Sinks in the Landscape, Boltzmann Brains, and the Cosmological Constant Problem
- First Dark Matter Search Results from a Surface Run of the 10-L DMTPC Directional Dark Matter Detector
- Optimizing WIMP directional detectors
- Determining the WIMP mass using direct detection experiments
- Markov Chain Monte Carlo analysis to constrain Dark Matter properties with directional detection
- Directional recoil rates for WIMP direct detection
- Exclusion limits from data of directional Dark Matter detectors
- The median recoil direction as a WIMP directional detection signal
- Probing the Local Velocity Distribution of WIMP Dark Matter with Directional Detectors
- Consequences of statistical sense determination for WIMP directional detection
- The Maximum Patch Method for Directional Dark Matter Detection
- Extending the optimum interval method