Journal
PHYSICS LETTERS B
Volume 624, Issue 3-4, Pages 186-194Publisher
ELSEVIER SCIENCE BV
DOI: 10.1016/j.physletb.2005.08.021
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The PICASSO experiment reports an improved limit for the existence of cold dark matter WIMPs interacting via spin-dependent interactions with nuclei. The experiment is installed in the Sudbury Neutrino Observatory at a depth of 2070 m. With superheated C4F10 droplets as the active material, and an exposure of 1.98 +/- 0.19 kg day, no evidence for a WIMP signal was found. For a WIMP mass of 29 GeV/c(2), limits on the spin-dependent cross section on protons of sigma(p) = 1.31 pb and on neutrons of sigma(n) = 21.5 pb have been obtained at 90% C.L. In both cases, some new parameter space in the region of WIMP masses below 20 GeV/c2 has now been ruled out. The results of these measurements are also presented in terms of limits on the effective WIMP-proton and neutron coupling strengths a(p) and a(n). (c) 2005 Elsevier B.V. All rights reserved.
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