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G. Jungman
1996
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D.N. Spergel
2003
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E. A. Baltz & P. Gondolo, JHEP 10, 052 (2004)
2004
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2005
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2006
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2008
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CDMS Collab., in preparation
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Z. Ahmed
Original
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2009
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Z. Ahmed
2009
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2010

CDMS-II to SuperCDMS: WIMP search at a zeptobarn

Bruch, T.

Understand

The Cryogenic Dark Matter search experiment (CDMS) employs low-temperature Ge and Si detectors to detect WIMPs via their elastic scattering of target nuclei.

The last analysis with an germanium exposure of 397.8 kg-days resulted in zero observed candidate events, setting an upper limit on the spin-independent WIMP-nucleon cross-section of 6.6 x 10^{-44} cm^2 (4.6 x 10^{-44} cm^2, when previous CDMS Soudan data is included) for a WIMP mass of 60 GeV.
The improvements in the surface event rejection capability for the current analysis with an germanium exposure about a factor of 2.5 greater than used in the last analysis will be discussed.
To increase the sensitivity beyond the 1 x 10^{-44} cm^2 benchmark new 1 inch thick detectors have been developed.