Directional detection of galactic Dark Matter
F. Mayet (1), J. Billard (1), G. Bernard (1), G. Bosson (1), O., Bourrion (1), C. Grignon (1), O. Guillaudin (1), C. Koumeir (1), J.P. Richer, (1), D. Santos (1), P. Colas (2), E. Ferer (2), I. Giomataris (2), A. Allaoua, (3), L. Lebreton (3) ((1) LPSC Grenoble, (2) CEA Saclay
TL;DR
This paper discusses advancements in gaseous detectors for directional detection of galactic Dark Matter, aiming to distinguish genuine WIMP signals from background noise.
Contribution
It presents technical progress and recent phenomenological studies that enable the design of competitive directional Dark Matter detection experiments.
Findings
Progress in gaseous detector technology.
Feasibility of directional detection for Dark Matter.
Enhanced discrimination between WIMP signals and background.
Abstract
Directional detection of galactic Dark Matter is a promising search strategy for discriminating geniune WIMP events from background ones. We present technical progress on gaseous detectors as well as recent phenomenological studies, allowing the design and construction of competitive experiments.
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · CCD and CMOS Imaging Sensors · Spectroscopy and Laser Applications