ZEPLIN-II limits on WIMP-nucelon interactions

G J Alner,R Preece,E J Daw,R J Walker, Cesar Augusto Tiburcio Silva,P Majewski, V N Lebedenko, S M Paling,F L H Wolfs,F Sergiampietri, A Murphy,J Pinto Da Cunha,S J S Plank,V N Solovov,T Durkin,B Edwards,V Kudryavtsev,M I Lopes,R Luscher,R J Cashmore,D R Tovey,T J Sumner,V Chepel,D Muna,J J Quenby,A Bewick,J T White, J F Dawson,W Ooi,Margaret Robinson,P F Smith,Colin R Thorne,K Mavrokoridis,F Neves, D Cline,A Lindote,T B Lawson,Jun Gao,C Ghag,P K Lightfoot, G G Nicklin,D Davidge,N J T Smith,A S Howard,H Chagani,Mukta C Joshi,J D Lewin,H M Araujo,Hua Wang,W G Jones,M Carson,B Camanzi,T Gamble,B P Morgan,N J C Spooner,C Bungau,I Liubarsky,J C Davies,J E Mcmillan,Eirini Tziaferi

AIP Conference Proceedings（2009）

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摘要

ZEPLIN II is a two-phase xenon detector designed to detect dark matter in the form of Weakly Interacting Massive Particles (WIMPs). Following the first 31-day underground run in Boulby Mine, UK, the collaboration published dark matter limits in January 2007; the first such limits using two-phase xenon technology. We outline the key detector design, performance and results here.

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关键词

cosmology,dark matter,radiation detectors

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