Abstract

We report new limits on nuclear scattering events resulting from Galactic dark matter in the form of hypothetical weakly interacting massive particles. By pulse shape analysis of 6 months' underground data from a 6 kg sodium iodide crystal, over the gamma-equivalent energy range 4–25 keV, we achieve a sensitivity to nuclear recoil events a factor 10–40 below the gamma and beta background. Limits obtained for spin-dependent dark matter interactions improve on Ge detectors by a factor 50. Limits for coherent interactions improve marginally on Ge for masses > 50 GeV, with foreseeable improvements offering further gains of 1–2 orders of magnitude.

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