Results from the first stage of a UK Galactic dark matter search using low background sodium iodide detectors

Physics

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Scientific paper

Low-energy background spectra from 1.3 kg and 6.2 kg Nal(TI) crystal scintillators operating in the shielded Boulby underground facility were measured. Upper limits to the scattering interaction rates and cross-sections of Galactic dark matter in the form of Weakly Interacting Massive Particles (WIMPs) are calculated from these data. This work provides an improved limit for spin-dependent interactions for WIMP masses above 10 GeV.

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