Published February 16, 2006
| Version public
Book Section - Chapter
The SuperCDMS Experiment
Creators
- Schnee, R. W.1
- Akerib, D. S.1
- Attisha, M. J.2
- Bailey, C. N.1
- Baudis, L.3
- Bauer, D. A.4
- Brink, P. L.5
- Brusov, P. P.1
- Bunker, R.6
- Cabrera, B.5
- Caldwell, D. O.6
- Chang, C. L.5
- Cooley, J.5
- Crisler, M. B.4
- Cushman, P.7
- Denes, P.8
- Dragowsky, M. R.1
- Duong, L.7
- Filippini, J.9
- Gaitskell, R. J.2
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Golwala, S. R.10
- Grant, D. R.1
- Hennings-Yeomans, R.1
- Holmgren, D.4
- Huber, M. E.11
- Irwin, K.12
- Lu, A.8
- Mahapatra, R.6
- Meunier, P.9
- Mirabolfathi, N.9
- Nelson, H.6
- Ogburn, R. W.5
- Ramberg, E.4
- Reisetter, A.7
- Saab, T.3
- Sadoulet, B.9, 8
- Sander, J.6
- Seitz, D. N.9
- Serfass, B.9
- Sundqvist, K. M.9
- Thompson, J-P. F.2
- Yellin, S.6
- Yoo, J.4
- Young, B. A.13
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1.
Case Western Reserve University
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2.
Brown University
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3.
University of Florida
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4.
Fermilab
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5.
Stanford University
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6.
University of California, Santa Barbara
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7.
University of Minnesota
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8.
Lawrence Berkeley National Laboratory
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9.
University of California, Berkeley
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10.
California Institute of Technology
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11.
University of Colorado Denver
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12.
National Institute of Standards and Technology
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13.
Santa Clara University
Contributors
Abstract
Nonluminous, nonbaryonic, weakly interacting massive particles (WIMPs) [1, 2] may constitute most of the matter in the universe [3]. WIMPs are expected to be in a roughly isothermal Galactic halo. They would interact elastically with nuclei, generating a recoil energy of a few tens of keV, at a rate ≾1 event kg⁻¹ d⁻¹ [2, 4, 5].
Additional Information
© 2006 Springer-Verlag Berlin Heidelberg.Additional details
Identifiers
- Eprint ID
- 101967
- DOI
- 10.1007/3-540-26373-x_20
- Resolver ID
- CaltechAUTHORS:20200318-101419532
Related works
- Describes
- 10.1007/3-540-26373-x_20 (DOI)
Dates
- Created
-
2020-03-18Created from EPrint's datestamp field
- Updated
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2021-11-16Created from EPrint's last_modified field