Silicon detector results from the first five-tower run of CDMS II

Autor: Y. Ricci, O. Kamaev, Jeffrey P. Filippini, B. Welliver, G.L. Godfrey, Peter S. Kim, Cristián Martínez, B. Cornell, Martin E. Huber, A. W. Borgland, R. H. Nelson, E. Do Couto E Silva, Steven W. Leman, K. Koch, P. L. Brink, S. Scorza, M. Kiveni, Matt Pyle, T. Hofer, P. Cushman, T. Doughty, David O. Caldwell, D. Balakishiyeva, B. Kara, P. Di Stefano, S. Fallows, Adam Anderson, A. Jastram, A. N. Villano, S. J. Yellin, M. Kos, J. Sander, Tarek Saab, Miguel Daal, Robert A. Moffatt, Sunil Golwala, David G. Cerdeño, J. Hall, S. A. Hertel, Donald J. Holmgren, Kevin A. McCarthy, F. DeJongh, R. Partridge, R. Agnese, S. Arrenberg, P. Nadeau, J. Fox, K. Schneck, Danielle Speller, M. Pepin, R. W. Schnee, N. Mirabolfathi, H. Chagani, L. Hsu, Douglas Wright, R. Mahapatra, Jodi Cooley, J. Zhang, R. Basu Thakur, M. H. Kelsey, K. L. Page, R. H. Harris, J. Yoo, Betty A. Young, L. Esteban, A. Phipps, K. M. Sundqvist, R. Bunker, H. Qiu, T. Bruch, A. Reisetter, W. Rau, D. Brandt, D. A. Bauer, Z. Ahmed, Matthew Fritts, E. Lopez-Asamar, Vuk Mandic, K. Prasad, P. Redl, David Moore, J. J. Yen, B. Shank, B. Serfass, C. H. Crewdson, A. Kennedy, Blas Cabrera, Bernard Sadoulet, Enectali Figueroa-Feliciano
Přispěvatelé: UAM. Departamento de Física Teórica
Rok vydání: 2013
Předmět:
Zdroj: Biblos-e Archivo. Repositorio Institucional de la UAM
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Popis: Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAM
We report results of a search for weakly interacting massive particles (WIMPs) with the Si detectors of the CDMS II experiment. This report describes a blind analysis of the first data taken with CDMS II’s full complement of detectors in 2006–2007; results from this exposure using the Ge detectors have already been presented. We observed no candidate WIMP-scattering events in an exposure of 55.9 kg-days before analysis cuts, with an expected background of ˞1.1 events. The exposure of this analysis is equivalent to 10.3 kg-days over a recoil energy range of 7–100 keV for an ideal Si detector and a WIMP mass of 10 GeV/c2. These data set an upper limit of 1.7 x 10-41 cm2 on the WIMP-nucleon spin-independent cross section of a 10 GeV/c2 WIMP. These data exclude parameter space for spin-independent WIMP-nucleon elastic scattering that is relevant to recent searches for low-mass WIMPs
This work is supported in part by the National Science Foundation (Grants No. AST-9978911, No. NSF-1102795, No. PHY- 0847342, No. PHY-0542066, No. PHY-0503729, No. PHY- 0503629, No. PHY-0503641, No. PHY-0504224, No. PHY-0705052, No. PHY-0801708, No. PHY-0801712, No. PHY-0802575, No. PHY-0847342, No. PHY-0855299, No. PHY-0855525, No. PHY-1151869, and No. PHY- 1205898), by the Department of Energy (Contracts No. DE-AC03-76SF00098, No. DE-FG02-92ER40701, No. DE-FG03-90ER40569, No. DE-FG03-91ER40618, and No. DE-SC0004022), by the Swiss National Foundation (SNF Grant No. 20-118119), by NSERC Canada (Grants No. SAPIN 341314 and No. SAPPJ 386399), and by MULTIDARK CSD2009-00064 and FPA2012-34694. Fermilab is operated by Fermi Research Alliance, LLC under Contract No. De-AC02-07CH11359, while SLAC is operated under Contract No. DE-AC02- 76SF00515 with the U.S. Department of Energy
Databáze: OpenAIRE