The Cryogenic Dark Matter Search (CDMS) : Present Status and Future

P L Brink,Z Ahmed,D S Akerib,C N Bailey, D Balakishiyeva,D Bauer,J Beaty,R Bunker, B Cabrera,David O Caldwell,J Cooley,E Do Couto E Silva, P Cushman,F Dejongh, M R Dragowsky,L Duong, E Figueroafeliciano,J Filippini,M Fritts, S R Golwala,D R Grant,J Hall, R Henningsyeomans,S A Hertel, A Hojem,D Holmgren,L Hsu,M E Huber,O Kamaev,M Kos, M Kiveni,S W Leman,R Mahapatra,V Mandic, K A Mccarthy,D Moore,N Mirabolfathi,Harry Norman Nelson,L Novak,R W Ogburn,M Pyle,X Qiu,E Ramberg,W Rau,A Reisetter,T Saab, B Sadoulet,J Sander,Randal L Schmitt,R W Schnee, D N Seitz,B Serfass, K M Sundqvist,A Tomada,Gao Wang, P Wikus, S Yellin,Jaehyeok Yoo,B A Young

AIP Conference Proceedings（2009）

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摘要

The CDMS collaboration utilizes Ge detectors for their Weakly Interacting Massive Particle (WIMP) search at the Soudan mine, Minnesota. The final data run of CDMS II is complete and a detector upgrade for SuperCDMS has commenced. A SuperTower of five 1-inch thick Ge crystals has been installed and undergoing commissioning. Its surface-event rejection capability should allow SuperCDMS to continue to run background free for the next proposed phases: 15 kg Ge deployment at Soudan, and up to 150 kg Ge deployment at SNOLAB. Recent detector advances to allow a 1 tonne Ge experiment are also discussed.

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关键词

Dark Matter,Cryogenic detectors

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