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.

Authors

  • Sven Vahsen

    University of Hawaii

  • Kamaluoawaiku Beamer

    University of Hawaii

  • Michael Hedges

    University of Hawaii

  • Igal Jaegle

    University of Hawaii

  • Marc Rosen

    University of Hawaii

  • Steven Ross

    University of Hawaii

  • Ilsoo Seong

    University of Hawaii

  • Thomas Thorpe

    University of Hawaii

  • Jared Yamaoka

    University of Hawaii, University of Hawaii at Manoa