Phys. Rev. Lett. 101, 251301 (2008) [4 pages]Experimental Constraints on a Dark Matter Origin for the DAMA Annual Modulation EffectSee Also: Erratum
See accompanying Physics Synopsis 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. © 2008 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevLett.101.251301
DOI:
10.1103/PhysRevLett.101.251301
PACS:
95.35.+d, 14.80.Mz, 29.40.Wk, 95.55.Vj
See AlsoErratum: C. E. Aalseth, P. S. Barbeau, D. G. Cerdeno, J. Colaresi, J. I. Collar, P. de Lurgio, G. Drake, J. E. Fast, C. H. Greenberg, T. W. Hossbach, J. D. Kephart, M. G. Marino, H. S. Miley, J. L. Orrell, D. Reyna, R. G. Robertson, R. L. Talaga, O. Tench, T. D. Van Wechel, J. F. Wilkerson, and K. M. Yocum, Erratum: Experimental Constraints on a Dark Matter Origin for the DAMA Annual Modulation Effect [Phys. Rev. Lett. 101, 251301 (2008)], Phys. Rev. Lett. 102, 109903 (2009). |
