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cdms-ii - CDMS Experiment - University of California, Berkeley

cdms-ii - CDMS Experiment - University of California, Berkeley

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Abstract<br />

There is an abundance <strong>of</strong> evidence that the majority <strong>of</strong> the mass <strong>of</strong> the universe<br />

is in the form <strong>of</strong> non-baryonic non-luminous matter that was non-relativistic at the<br />

time when matter began to dominate the energy density. Weakly Interacting Massive<br />

Particles, or WIMPs, are attractive cold dark matter candidates because they would<br />

have a relic abundance today <strong>of</strong> ∼0.1 which is consistent with precision cosmological<br />

measurements. WIMPs are also well motivated theoretically. Many minimal supersymmetric<br />

extensions <strong>of</strong> the Standard Model have WIMPs in the form <strong>of</strong> the lightest<br />

supersymmetric partner, typically taken to be the neutralino.<br />

The <strong>CDMS</strong> II experiment searches for WIMPs via their elastic scattering <strong>of</strong>f <strong>of</strong><br />

nuclei. The experiment uses Ge and Si ZIP detectors, operated at

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