Exclusion Limits on the WIMP-Nucleon Cross-Section from the First Run of hte Cryogenic Dark Matter in the Soudan Underground Lab.
Akerib, D. S. ; Armel Funkhouser, M. S. ; Attisha, M. J. ; Bailey, C. N. ; Baudin, L. ; Bauer, D. A. ; Brink, P. L. ; Bunker, R. ; Cabrera, B. ; Caldwell, D. O.
The Cryogenic Dark Matter Search (CDMS-II) employs low-temperature Ge and Si detectors to seek Weakly Interacting Massive Particles (WIMPs) via their elastic scattering interactions with nuclei. Simultaneous measurements of both ionization and phonon energy provide discrimination against interactions of background particles. For recoil energies above 10 keV, events due to background photons are rejected with > 99.99% efficiency. Electromagnetic events very near the detector surface can mimic nuclear recoils because of reduced charge collection, but these surface events are rejected with > 96% efficiency by using additional information from the phonon pulse shape. Efficient use of active and passive shielding, combined with the the 2090 m.w.e. overburden at the experimental site in the Soudan mine, makes the background from neutrons negligible for this first exposure. All cuts are determined in a blind manner from in situ calibrations with external radioactive sources without any prior knowledge of the event distribution in the signal region.