Improved spin-dependent limits from the PICASSO dark matter search experiment

被引:74
作者
Barnabé-Heider, M
Di Marco, M
Doane, P
Genest, MH
Gornea, R
Guénette, R
Leroy, C
Lessard, L
Martin, JP
Wichoski, U
Zacek, V
Clark, K
Krauss, C
Noble, A
Behnke, E
Feighery, W
Levine, I
Muthusi, C
Kanagalingam, S
Noulty, R
机构
[1] Univ Montreal, Dept Phys, Montreal, PQ H3C 3J7, Canada
[2] Queens Univ, Dept Phys, Kingston, ON K7L 3NG, Canada
[3] Indiana Univ, Dept Phys, South Bend, IN 46634 USA
[4] Indiana Univ, Dept Astron, South Bend, IN 46634 USA
[5] Bubble Technol Ind, Chalk River, ON K0J 1J0, Canada
基金
加拿大创新基金会; 加拿大自然科学与工程研究理事会;
关键词
D O I
10.1016/j.physletb.2005.08.021
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:186 / 194
页数:9
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