English   español  
Por favor, use este identificador para citar o enlazar a este item: http://hdl.handle.net/10261/6861
COMPARTIR / IMPACTO:
Estadísticas
logo share SHARE   Add this article to your Mendeley library MendeleyBASE
Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL
Exportar a otros formatos:
Título

Experimental constraints on a dark matter origin for the DAMA annual modulation effect

AutorAalseth, C. E.; Barbeau, P. S.; Cerdeño, David G. ; Colaresi, J.; Collar, Juan I.; Lurgio, P. de; Drake, G.; Fast, J. E.; Greenberg, C. H.; Hossbach, T. W.; Kephart, J. D.; Marino, M. G.; Miley, H. S.; Orrell, J. L.; Reyna, D.; Robertson, R. G. H.; Talaga, R.; Tench, O.; Wechel, T. D. van; Wilkerson, J. F.; Yocum, K. M.
Palabras claveAstrophysics
High Energy Physics - Experiment
Instrumentation and Detectors
Fecha de publicación31-jul-2008
CitaciónarXiv:0807.0879v4 [astro-ph]
SerieIFT-UAM/CSIC-08-39
FTUAM-08-7
ResumenA 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 (WIMPs) as the explanation for the annual modulation effect leading to the claim. Bounds are similarly imposed on a suggestion that dark pseudoscalars mightlead 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.
Descripción4 pages.-- PACS numbers: 85.30.-z, 95.35.+d, 95.55.Vj, 14.80.Mz.-- Submitted on 5 Jul 2008 (v1), last revised 31 Jul 2008 (this version, v4): v4 introduces recent results from arXiv:0807.3279 and arXiv:0807.2926. Sensitivity to pseudoscalars is revised in light of the first. Discussion on the subject added.
URIhttp://hdl.handle.net/10261/6861
Aparece en las colecciones: (IFT) Artículos
Ficheros en este ítem:
Fichero Descripción Tamaño Formato  
0807.0879v4.pdf4,32 MBAdobe PDFVista previa
Visualizar/Abrir
Mostrar el registro completo
 


NOTA: Los ítems de Digital.CSIC están protegidos por copyright, con todos los derechos reservados, a menos que se indique lo contrario.