We report results from the Cryogenic Dark Matter Search at the Soudan Underground Laboratory (CDMS II) featuring the full complement of 30 detectors. A blind analysis of data taken between October 2006 and July 2007 sets an upper limit on the weakly interacting massive particle (WIMP) nucleon spin-independent cross section of 6.6×10^-44 cm² (4.6×10^-44 cm² when combined with previous CDMS II data) at the 90% confidence level for a WIMP mass of 60 GeV/c². This achieves the best sensitivity for dark matter WIMPs with masses above 44 GeV/c², and significantly restricts the parameter space for some favored supersymmetric models.
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Ahmed et al. (2009) studied this question.
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