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

被引:125
作者
Aalseth, C. E. [3 ]
Barbeau, P. S. [1 ,2 ]
Cerdeno, D. G. [4 ,5 ]
Colaresi, J. [6 ]
Collar, J. I. [1 ,2 ]
de Lurgio, P. [7 ]
Drake, G. [7 ]
Fast, J. E. [3 ]
Greenberg, C. H. [1 ,2 ]
Hossbach, T. W. [3 ]
Kephart, J. D. [3 ]
Marino, M. G. [9 ,10 ]
Miley, H. S. [3 ]
Orrell, J. L. [3 ]
Reyna, D. [8 ]
Robertson, R. G. H. [9 ,10 ]
Talaga, R. L. [7 ]
Tench, O. [6 ]
Van Wechel, T. D. [9 ,10 ]
Wilkerson, J. F. [9 ,10 ]
Yocum, K. M. [6 ]
机构
[1] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA
[2] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA
[3] Pacific NW Natl Lab, Richland, WA 99352 USA
[4] Univ Autonoma Madrid, Dept Fis Teor C 11, E-28049 Madrid, Spain
[5] Univ Autonoma Madrid, CSIC, UAM, Inst Fis Teor, E-28049 Madrid, Spain
[6] CANBERRA Ind, Meriden, CT 06450 USA
[7] Argonne Natl Lab, Argonne, IL 60439 USA
[8] Sandia Natl Labs, Livermore, CA 94550 USA
[9] Univ Washington, Ctr Expt Nucl Phys & Astrophys, Seattle, WA 98195 USA
[10] Univ Washington, Dept Phys, Seattle, WA 98195 USA
关键词
D O I
10.1103/PhysRevLett.101.251301
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
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.
引用
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页数:4
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