Limits on the WIMP-nucleon cross-section from the Cryogenic Dark Matter Search

被引：0
|
作者：
Gaitskell, RJ [1 ]
机构：
[1] Univ Coll London, Dept Phys & Astron, London WC1E 6BT, England
来源：
IDENTIFICATION OF DARK MATTER | 2001年
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The Cryogenic Dark Matter Search (CDMS) employs Ge and Si detectors to search for WIMPS via their elastic-scattering interactions with nuclei while discriminating against interactions of background particles. CDMS I data, from the Stanford Underground Facility shallow site, give limits on the spin-independent WIMP-nucleon elastic-scattering cross-section that exclude unexplored parameter space above 10 GeV c(-2) WIMP mass and, at > 75% CL, the entire 3 sigma allowed region for the WIMP signal reported by the DAMA experiment. The move to a deep site at Soudan, Minnesota, should improve the experiment's sensitivity by similar to 100x. "First Dark" for CDMS II will be in 2001.
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页码：349 / 354
页数：6
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