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The Directional Dark Matter Detector

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arxiv 1110.3401 v1 pith:RYKYGPWL submitted 2011-10-15 astro-ph.IM

classification astro-ph.IM
keywords darkdetectormatterbackgrounddirectionallow-masssearchessuitable
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abstract

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-$\rm m^3$-scale directional dark matter detector, \dcube. 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.

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  1. Ubiquitous Corotation of Dark Matter Halos: Implications for Direct Detection

    hep-ph 2026-07 conditional novelty 6.0 of 10

    Dark matter in simulated Milky Way analogues preferentially corotates with the baryonic disk, suppressing predicted direct-detection rates for light WIMPs, reducing directional modulation, and producing a 21% astrophy...

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