Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
9860902 | Physics Letters B | 2005 | 9 Pages |
Abstract
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±0.19kgâday, no evidence for a WIMP signal was found. For a WIMP mass of 29 GeV/c2, limits on the spin-dependent cross section on protons of Ïp=1.31pb and on neutrons of Ïn=21.5pb 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 ap and an.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
M. Barnabé-Heider, M. Di Marco, P. Doane, M.-H. Genest, R. Gornea, R. Guénette, C. Leroy, L. Lessard, J.-P. Martin, U. Wichoski, V. Zacek, K. Clark, C. Krauss, A. Noble, E. Behnke, W. Feighery, I. Levine, C. Muthusi, R. Noulty,