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The SuperCDMS Experiment
C. N. Bailey
D. O. Caldwell
J. Cooley
M. R. Dragowsky
Daniel S. Akerib
B. Cabrera
M. B. Crisler
P. P. Brusov
P. Cushman
R. J. Gaitskell
S. R. Golwala
P. L. Brink
R. Bunker
L. Duong
L. Baudis
P. Denes
J. Filippini
M. J. Attisha
Daniel A. Bauer
Richard W. Schnee
C. L. Chang
出版
United States. Department of Energy
, 2005
URL
http://books.google.com.hk/books?id=1QX9jwEACAAJ&hl=&source=gbs_api
註釋
Modest improvements in the level and/or discrimination of backgrounds are needed to keep backgrounds negligible during the three phases of SuperCDMS. By developing production designs that require only modest testing, detector production rates may be improved sufficiently to allow an exposure of 500 ton d within a reasonable time and budget. Overall, the improvement estimates described above are conservative. Previous development efforts have shown that some areas prove easier and provide larger factors while others prove more difficult. The conservative estimates together with the broad approach reduce the risk and give us confidence that we will succeed, providing the surest way to probe to WIMP-nucleon cross sections of 10{sup -46} cm{sup 2}.