Issue |
EAS Publications Series
Volume 53, 2012
CYGNUS 2011: Third International Conference on Directional Detection of Dark Matter
|
|
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Page(s) | 43 - 50 | |
DOI | https://doi.org/10.1051/eas/1253006 | |
Published online | 15 February 2012 |
F. Mayet and D. Santos (eds)
EAS Publications Series, 53 (2012) 43-50
The Directional Dark Matter Detector (D3)
1
University of Hawaii, 2505 Correa Road, Honolulu, HI
96822,
USA
2
Lawrence Berkeley National Laboratory,
1 Cyclotron Road,
Berkeley, CA
94720,
USA
Gas-filled Time Projection Chambers (TPCs) with Gas Electron Multipliers (GEMs) and pixels appear suitable for direction-sensitive WIMP dark matter searches. We present the background and motivation for our work on this technology, past and ongoing prototype work, and a development path towards an affordable, 1-m3-scale directional dark matter detector, D3. Such a detector may be particularly suitable for low-mass WIMP searches, and perhaps sufficiently sensitive to clearly determine whether the signals seen by DAMA, CoGeNT, and CRESST-II are due to low-mass WIMPs or background.
© EAS, EDP Sciences 2012