Search for an annual modulation in a p-type point contact Germanium dark matter detector

  • C. E. Aalseth
  • , P. S. Barbeau
  • , J. Colaresi
  • , J. I. Collar
  • , J. Diaz Leon
  • , J. E. Fast
  • , N. Fields
  • , T. W. Hossbach
  • , M. E. Keillor
  • , J. D. Kephart
  • , A. Knecht
  • , M. G. Marino
  • , H. S. Miley
  • , M. L. Miller
  • , J. L. Orrell
  • , D. C. Radford
  • , J. F. Wilkerson
  • , K. M. Yocum

    Research output: Contribution to journalArticlepeer-review

    468 Scopus citations

    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 languageEnglish
    Article number141301
    JournalPhysical Review Letters
    Volume107
    Issue number14
    DOIs
    StatePublished - Sep 26 2011

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