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Volumn 327, Issue 5973, 2010, Pages 1619-1621

Dark matter search results from the CDMS il experiment

(60)  Cooley, Jodi i   Ahmed, Z a   Akerib, D S b   Arrenberg, S r   Bailey, C N b   Balakishiyeva, D p   Baudis, L r   Bauer, D A c   Brink, P L j   Bruch, T r   Bunker, R n   Cabrera, B j   Caldwell, D O n   Cushman, P q   Daal, M m   Dejongh, F c   Dragowsky, M R b   Duong, L q   Fallows, S q   Figueroa Feliciano, E e   more..


Author keywords

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Indexed keywords

GERMANIUM;

EID: 77950284298     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1186112     Document Type: Article
Times cited : (717)

References (20)
  • 1
    • 69649107499 scopus 로고    scopus 로고
    • E. Komatsu et al., Astrophys. J. 180, (Suppl), 330 (2009).
    • (2009) Astrophys. J. , vol.180 , Issue.SUPPL. , pp. 330
    • Komatsu, E.1
  • 8
    • 58649118638 scopus 로고    scopus 로고
    • CDMS Collaboration
    • Z. Ahmed et al.; CDMS Collaboration, Phys. Rev. Lett. 102, 011301 (2009).
    • (2009) Phys. Rev. Lett. , vol.102 , pp. 011301
    • Ahmed, Z.1
  • 12
    • 77950213348 scopus 로고    scopus 로고
    • note
    • We calculate the 90% confidence level upper limit based on standard galactic halo assumptions (15) and in the presence of two events at the observed energies. We use the optimum interval method (16) with no background subtraction. A combined limit was also calculated by combining these data with all previous results from Soudan (8), including alt candidates and with efficiency weighted by the exposure of each analysis. The abrupt features in these curves are consequences of threshold crossings at which intervals containing one or more events could enter into the optimum interval computation. An improved estimate of our detector masses was used for the reported exposure calculation and applied retroactively to our previous CDMS II result.
  • 20
    • 77950244270 scopus 로고    scopus 로고
    • note
    • The CDMS collaboration gratefully acknowledges the contributions of numerous engineers and technicians; we would like to especially thank J. Beaty, B. Hines, L. Novak, R. Schmitt, and A. Tomada. This work is supported in part by the National Science Foundation (grants AST-9978911, PHY-0542066, PHY-0503729, PHY-0503629, PHY0503641, PHY-0504224, PHY-0705052, PHY-0801708, PHY-0801712, PHY-0802575, and PHY-0855525), by the Department of Energy (contracts DE-AC03-76SF00098, DE-FG02-91ER40688, DE-FG02-92ER40701, DE-FG0390ER40569, and DE-FG03-91ER40618), by the Swiss National Foundation (SNF grant 20-118119), and by the Natural Sciences and Engineering Research Council of Canada (grant SAPIN 341314-07).


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.