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The Cryogenic Dark Matter Search (CDMS) Experiment

The CDMS experiment is searching for WIMP dark matter in our galaxy with novel cryogenic detectors that reject background photons. The experiment has begun first data taking in the summer and fall of 1996 (covering a period that extends beyond the date of this conference). We report on results from 60 g germanium and 100 g silicon detectors, including an assessment of their background rejection performance, their initial measurements of the radioactive background in the cryostat and an estimate of their sensitivity to dark matter.