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2. New dark matter limits from the Boulby NaI detectors

Author

M.J. van den Putte, N. J. T. Smith, G.J. Davies, J. Li, W. G. Jones, P.F. Smith, T. J. Sumner, T. Ali, P.R. Blake, J. C. Barton, J.J. Quenby, A. Bewick, G. T. J. Arnison, C.H. Lally, J. D. Lewin, G.J. Homer, N. J. C. Spooner, G.J. Alner, and D. Shaul

Subjects
Physics, Nuclear and High Energy Physics, Range (particle radiation), Large Underground Xenon experiment, DAMA/NaI, Weakly interacting massive particles, Dark matter, Detector, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Cryogenic Dark Matter Search, Light dark matter, Atomic and Molecular Physics, and Optics
Abstract

Using pulse shape analysis of data from 173 operating days of our 6.2 kg NaI detector in the energy range 7–10 keV we present new limits on weakly interacting massive particles that may constitute the dark matter. An improvement of a factor >30 has been obtained over Ge for spin-dependent dark matter interactions while limits for coherent interactions are comparable to Ge for masses > 100 GeV.

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