Experimental Constraints on a Dark Matter Origin for the DAMA Annual Modulation Effect

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ID: 269567
2008
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Abstract
A claim for evidence of dark matter interactions in the DAMA experiment has been recently reinforced. We employ a new type of germanium detector to conclusively rule out a standard isothermal galactic halo of weakly interacting massive particles as the explanation for the annual modulation effect leading to the claim. Bounds are similarly imposed on a suggestion that dark pseudoscalars might lead to the effect. We describe the sensitivity to light dark matter particles achievable with our device, in particular, to next-to-minimal supersymmetric model candidates.
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yocum2008physicalexperimental Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors C. E. Aalseth,Phillip Barbeau,David G. Cerdeño,J. Colaresi,J. I. Collar,P. De Lurgio,G. Drake,J. E. Fast,C. H. Greenberg,Todd Hossbach,J. D. Kephart,Michael Marino,H. S. Miley,John Orrell,D. Reyna,R. G. H. Robertson,R. L. Talaga,O. Tench,T. D. Van Wechel,John Wilkerson,K. M. Yocum;C. E. Aalseth;Phillip Barbeau;David G. Cerdeño;J. Colaresi;J. I. Collar;P. De Lurgio;G. Drake;J. E. Fast;C. H. Greenberg;Todd Hossbach;J. D. Kephart;Michael Marino;H. S. Miley;John Orrell;D. Reyna;R. G. H. Robertson;R. L. Talaga;O. Tench;T. D. Van Wechel;John Wilkerson;K. M. Yocum;
Journal physical review letters
Year 2008
DOI
10.1103/physrevlett.101.251301
URL
https://sciprofiles.com/publication/view/64ffa79367885fc584abefad99fcb71f
Keywords
model dark matter claim dama modulation effect annual modulation effect leading

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