Phys. Rev. Lett.
93,
211301
(2004)
[5 pages]
First Results from the Cryogenic Dark Matter Search in the Soudan Underground Laboratory
D. S. Akerib et al. CDMS Collaboration
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D. S. Akerib1, J. Alvaro-Dean2, M. S. Armel-Funkhouser2, M. J. Attisha3, L. Baudis4,5, D. A. Bauer6, J. Beaty7, P. L. Brink5, R. Bunker8, S. P. Burke8, B. Cabrera5, D. O. Caldwell8, D. Callahan8, J. P. Castle5, C. L. Chang5, R. Choate6, M. B. Crisler6, P. Cushman7, R. Dixon6, M. R. Dragowsky1, D. D. Driscoll1, L. Duong7, J. Emes9, R. Ferril8, J. Filippini2, R. J. Gaitskell3, M. Haldeman6, D. Hale8, D. Holmgren6, M. E. Huber10, B. Johnson6, W. Johnson6, S. Kamat1, M. Kozlovsky6, L. Kula6, S. Kyre8, B. Lambin6, A. Lu2, R. Mahapatra8, A. G. Manalaysay1, V. Mandic2, J. May8, R. McDonald9, B. Merkel6, P. Meunier2, N. Mirabolfathi2, S. Morrison6, H. Nelson8, R. Nelson8, L. Novak5, R. W. Ogburn5, S. Orr6, T. A. Perera1, M. C. Perillo Isaac2, E. Ramberg6, W. Rau2, A. Reisetter7, R. R. Ross9,2,*, T. Saab5, B. Sadoulet9,2, J. Sander8, C. Savage8, R. L. Schmitt6, R. W. Schnee1, D. N. Seitz2, B. Serfass2, A. Smith9, G. Smith2, A. L. Spadafora9, K. Sundqvist2, J-P. F. Thompson3, A. Tomada5, G. Wang1, J. Williams6, S. Yellin8, and B. A. Young11 (CDMS Collaboration)
1Department of Physics, Case Western Reserve University, Cleveland, Ohio 44106, USA 2Department of Physics, University of California, Berkeley, California 94720, USA 3Department of Physics, Brown University, Providence, Rhode Island 02912, USA 4Department of Physics, University of Florida, Gainesville, Florida 32611, USA 5Department of Physics, Stanford University, Stanford, California 94305, USA 6Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA 7School of Physics & Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA 8Department of Physics, University of California, Santa Barbara, California 93106, USA 9Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA 10Department of Physics, University of Colorado–Denver, Denver, Colorado 80217, USA 11Department of Physics, Santa Clara University, Santa Clara, California 95053, USA
Received 4 May 2004; published 16 November 2004
We report the first results from a search for weakly interacting massive particles (WIMPs) in the Cryogenic Dark Matter Search experiment at the Soudan Underground Laboratory. Four Ge and two Si detectors were operated for 52.6 live days, providing 19.4 kg d of Ge net exposure after cuts for recoil energies between 10 and 100 keV. A blind analysis was performed using only calibration data to define the energy threshold and selection criteria for nuclear-recoil candidates. Using the standard dark-matter halo and nuclear-physics WIMP model, these data set the world's lowest exclusion limits on the coherent WIMP-nucleon scalar cross section for all WIMP masses above 15 GeV/c2, ruling out a significant range of neutralino supersymmetric models. The minimum of this limit curve at the 90% C.L. is 4×10-43 cm2 at a WIMP mass of 60 GeV/c2.
© 2004 The American Physical Society
URL:
http://link.aps.org/doi/10.1103/PhysRevLett.93.211301
DOI:
10.1103/PhysRevLett.93.211301
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