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Limits on Spin-Independent Interactions of Weakly Interacting Massive Particles with Nucleons from the Two-Tower Run of the Cryogenic Dark Matter Search

2005/09/09 by CDMS Collaboration, D. S. Akerib, M. J. Attisha +53 · 2 citations
Physics and Astronomy · #Astrophysics #Cosmology #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark matter #Meson #Nuclear physics #Nucleon #Particle physics #Particle physics theoretical and experimental studies #Physics #Recoil #Scalar field dark matter #Spin (aerodynamics) #WIMP #Weakly interacting massive particles #astro-ph #hep-ex #nucl-ex

paper · pdf · doi:10.1103/physrevlett.96.011302

published as Phys.Rev.Lett.96:011302,2006 · 4 pages, 4 figures, submitted to Phys. Rev. Lett

arxiv created 2005/09/09 · openalex publication_date 2006/01/03 · arxiv updated 2012/08/27 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

We report new results from the Cryogenic Dark Matter Search (CDMS II) at the Soudan Underground Laboratory. Two towers, each consisting of six detectors, were operated for 74.5 live days, giving spectrum-weighted exposures of 34 (12) kg d for the Ge (Si) targets after cuts, averaged over recoil energies 10--100 keV for a weakly interacting massive particle (WIMP) mass of 60 GeV/c2. A blind analysis was conducted, incorporating improved techniques for rejecting surface events. No WIMP signal exceeding expected backgrounds was observed. When combined with our previous results from Soudan, the 90% C.L. upper limit on the spin-independent WIMP-nucleon cross section is 1.6\ifmmode×\else\texttimes\fi10^\ensuremath-43 cm2 from Ge and 3\ifmmode×\else\texttimes\fi10^\ensuremath-42 cm2 from Si, for a WIMP mass of 60 GeV/c2. The combined limit from Ge (Si) is a factor of 2.5 (10) lower than our previous results and constrains predictions of supersymmetric models.

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