Published February 16, 2006
| public
Book Section - Chapter
The SuperCDMS Experiment
- Creators
- Schnee, R. W.
- Akerib, D. S.
- Attisha, M. J.
- Bailey, C. N.
- Baudis, L.
- Bauer, D. A.
- Brink, P. L.
- Brusov, P. P.
- Bunker, R.
- Cabrera, B.
- Caldwell, D. O.
- Chang, C. L.
- Cooley, J.
- Crisler, M. B.
- Cushman, P.
- Denes, P.
- Dragowsky, M. R.
- Duong, L.
- Filippini, J.
- Gaitskell, R. J.
-
Golwala, S. R.
- Grant, D. R.
- Hennings-Yeomans, R.
- Holmgren, D.
- Huber, M. E.
- Irwin, K.
- Lu, A.
- Mahapatra, R.
- Meunier, P.
- Mirabolfathi, N.
- Nelson, H.
- Ogburn, R. W.
- Ramberg, E.
- Reisetter, A.
- Saab, T.
- Sadoulet, B.
- Sander, J.
- Seitz, D. N.
- Serfass, B.
- Sundqvist, K. M.
- Thompson, J-P. F.
- Yellin, S.
- Yoo, J.
- Young, B. A.
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
- Eprint ID
- 101967
- DOI
- 10.1007/3-540-26373-x_20
- Resolver ID
- CaltechAUTHORS:20200318-101419532
- Created
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2020-03-18Created from EPrint's datestamp field
- Updated
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2021-11-16Created from EPrint's last_modified field