Recent Progress on the Directional Dark Matter Detector (D$^{3})$
ORAL
Abstract
We present recent progress towards a direction-sensitive WIMP dark matter search based on gas-filled Time Projection Chambers (TPCs) where the drift charge is amplified with Gas Electron Multipliers (GEMs) and detected with pixel electronics. The advantage of this approach is that nuclear recoils can be reconstructed in three dimensions with low energy threshold and low noise, at room temperature. We present performance measurements of small prototypes and a development path towards an affordable, m$^{3}$-scale Directional Dark Matter Detector; D$^{3}$. 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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Authors
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Sven Vahsen
University of Hawaii
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Kamaluoawaiku Beamer
University of Hawaii
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Michael Hedges
University of Hawaii
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Igal Jaegle
University of Hawaii
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Marc Rosen
University of Hawaii
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Steven Ross
University of Hawaii
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Ilsoo Seong
University of Hawaii
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Thomas Thorpe
University of Hawaii
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Jared Yamaoka
University of Hawaii, University of Hawaii at Manoa