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

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;
physical review letters 2008 Vol. 101 pp. 251301-
135
yocum2008physicalexperimental

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.

Keywords

model dark matter claim dama modulation effect annual modulation effect leading

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DOI:
10.1103/physrevlett.101.251301
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https://sciprofiles.com/publication/view/64ffa7936...

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