Abstract
Fifteen months of cumulative CoGeNT data are examined for indications of an annual modulation, a predicted signature of weakly interacting massive particle (WIMP) interactions. Presently available data support the presence of a modulated component of unknown origin, with parameters prima facie compatible with a galactic halo composed of light-mass WIMPs. Unoptimized estimators yield a statistical significance for a modulation of ∼2.8σ, limited by the short exposure.
| Original language | English |
|---|---|
| Article number | 141301 |
| Journal | Physical Review Letters |
| Volume | 107 |
| Issue number | 14 |
| DOIs | |
| State | Published - Sep 26 2011 |
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