Dark Matter Search Results from the CDMS II Experiment

被引：626

作者：

Ahmed, Z. ^{[2
]}

Akerib, D. S. ^{[3
]}

Arrenberg, S. ^{[19
]}

Bailey, C. N. ^{[3
]}

Balakishiyeva, D. ^{[17
]}

Baudis, L. ^{[19
]}

Bauer, D. A. ^{[4
]}

Brink, P. L. ^{[10
]}

Bruch, T. ^{[19
]}

Bunker, R. ^{[14
]}

Cabrera, B. ^{[10
]}

Caldwell, D. O. ^{[14
]}

Cooley, J. ^{[1
]}

Cushman, P. ^{[18
]}

Daal, M. ^{[13
]}

DeJongh, F. ^{[4
]}

Dragowsky, M. R. ^{[3
]}

Duong, L. ^{[18
]}

Fallows, S. ^{[18
]}

Figueroa-Feliciano, E.

Filippini, J. ^{[2
]}

Fritts, M. ^{[18
]}

Golwala, S. R. ^{[2
]}

Grant, D. R. ^{[3
]}

Hall, J. ^{[4
]}

Hennings-Yeomans, R. ^{[3
]}

Hertel, S. A. ^{[6
]}

Holmgren, D. ^{[4
]}

Hsu, L. ^{[4
]}

Huber, M. E. ^{[15
,16
]}

Kamaev, O. ^{[18
]}

Kiveni, M. ^{[11
]}

Kos, M. ^{[11
]}

Leman, S. W. ^{[6
]}

Mahapatra, R. ^{[12
]}

Mandic, V. ^{[18
]}

McCarthy, K. A. ^{[6
]}

Mirabolfathi, N. ^{[13
]}

Moore, D. ^{[2
]}

Nelson, H. ^{[14
]}

Ogburn, R. W. ^{[10
]}

Phipps, A. ^{[13
]}

Pyle, M. ^{[10
]}

Qiu, X. ^{[18
]}

Ramberg, E. ^{[4
]}

Rau, W. ^{[7
]}

Reisetter, A. ^{[8
,18
]}

Saab, T. ^{[17
]}

Sadoulet, B. ^{[5
,13
]}

Sander, J.

机构：

[1] So Methodist Univ, Dept Phys, Dallas, TX 75275 USA

[2] CALTECH, Div Phys Math & Astron, Pasadena, CA 91125 USA

[3] Case Western Reserve Univ, Dept Phys, Cleveland, OH 44106 USA

[4] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA

[5] Univ Calif Berkeley, Lawrence Berkeley Lab, Berkeley, CA 94720 USA

[6] MIT, Dept Phys, Cambridge, MA 02139 USA

[7] Queens Univ, Dept Phys, Kingston, ON K7L 3N6, Canada

[8] St Olaf Coll, Dept Phys, Northfield, MN 55057 USA

[9] Santa Clara Univ, Dept Phys, Santa Clara, CA 95053 USA

[10] Stanford Univ, Dept Phys, Stanford, CA 94305 USA

[11] Syracuse Univ, Dept Phys, Syracuse, NY 13244 USA

[12] Texas A&M Univ, Dept Phys, College Stn, TX 77843 USA

[13] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[14] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA

[15] Univ Colorado, Dept Phys, Denver, CO 80217 USA

[16] Univ Colorado, Dept Elect Engn, Denver, CO 80217 USA

[17] Univ Florida, Dept Phys, Gainesville, FL 32611 USA

[18] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA

[19] Univ Zurich, Inst Phys, CH-8057 Zurich, Switzerland

来源：

SCIENCE | 2010年 / 327卷 / 5973期

基金：

美国国家科学基金会; 加拿大自然科学与工程研究理事会;

关键词：

D O I：

10.1126/science.1186112

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

Astrophysical observations indicate that dark matter constitutes most of the mass in our universe, but its nature remains unknown. Over the past decade, the Cryogenic Dark Matter Search (CDMS II) experiment has provided world-leading sensitivity for the direct detection of weakly interacting massive particle (WIMP) dark matter. The final exposure of our low-temperature germanium particle detectors at the Soudan Underground Laboratory yielded two candidate events, with an expected background of 0.9 +/- 0.2 events. This is not statistically significant evidence for a WIMP signal. The combined CDMS II data place the strongest constraints on the WIMP-nucleon spin-independent scattering cross section for a wide range of WIMP masses and exclude new parameter space in inelastic dark matter models.

引用

页码：1619 / 1621

页数：3

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