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25 April 2024
 
  » pubmed » pmid10991035

 Article overview



Exclusion limits on the WIMP-nucleon cross section from the cryogenic dark matter search
R Abusaidi ; D S Akerib ; P D Barnes ; D A Bauer ; A Bolozdynya ; P L Brink ; R Bunker ; B Cabrera ; D O Caldwell ; J P Castle ; R M Clarke ; P Colling ; M B Crisler ; A Cummings ; A Da Silva ; A K Davies ; R Dixon ; B L Dougherty ; D Driscoll ; S Eichblatt ; J Emes ; R J Gaitskell ; S R Golwala ; D Hale ; E E Haller ; J Hellmig ; M E Huber ; K D Irwin ; J Jochum ; F P Lipschultz ; A Lu ; V Mandic ; J M Martinis ; S W Nam ; H Nelson ; B Neuhauser ; M J Penn ; T A Perera ; M C Perillo Isaac ; B Pritychenko ; R R Ross ; T Saab ; B Sadoulet ; R W Schnee ; D N Seitz ; P Shestople ; T Shutt ; A Smith ; G W Smith ; A H Sonnenschein ; A L Spadafora ; W Stockwell ; J D Taylor ; S White ; S Yellin ; B A Young ; ;
Date 19 Jun 2000
Journal Phys Rev Lett, 84 (25), 5699-703
AbstractThe Cryogenic Dark Matter Search (CDMS) employs Ge and Si detectors to search for weakly interacting massive particles (WIMPs) via their elastic-scattering interactions with nuclei while discriminating against interactions of background particles. CDMS data, accounting for the neutron background, give limits on the spin-independent WIMP-nucleon elastic-scattering cross section that exclude unexplored parameter space above 10 GeV/c2 WIMP mass and, at >75% C.L., the entire 3sigma allowed region for the WIMP signal reported by the DAMA experiment.
Source PubMed, pmid10991035
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