101. First Results from the Cryogenic Dark Matter Search in the Soudan Underground Lab
- Author
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J. Emes, D. S. Akerib, Daniel E. Hale, Ronald R. Ross, K. M. Sundqvist, R. L. Dixon, S. Burke, J. P. Castle, R. W. Schnee, D. N. Seitz, D. D. Driscoll, R. Mahapatra, B. Johnson, M. Kozlovsky, P. Cushman, Scott P. Orr, C. Savage, Laura Baudis, Betty A. Young, Astrid Tomada, E. J. Ramberg, A. G. Manalaysay, D. Callahan, Bernard Sadoulet, Jasmine L. May, M. J. Attisha, J. P. F. Thompson, L. Novak, R. McDonald, J. Beaty, R. J. Gaitskell, Wendy Johnson, Donald J. Holmgren, P. L. Brink, B. Serfass, M. C. Perillo Isaac, David O. Caldwell, B. Merkel, G. Wang, B. Lambin, M. R. Dragowsky, A. Lu, G. Smith, Alan R. Smith, R. H. Nelson, M. S. Armel-Funkhouser, S. Morrison, J. Williams, Jeffrey P. Filippini, S. Kyre, L. Duong, Martin E. Huber, Vuk Mandic, M. Crisler, M. Haldeman, D. A. Bauer, J. Sander, Blas Cabrera, J. Alvaro-Dean, N. Mirabolfathi, R. Choate, P. Meunier, R. W. Ogburn, C. L. Chang, H. N. Nelson, L. Kula, A. L. Spadafora, R. Bunker, A. Reisetter, R. Schmitt, W. Rau, Tarek Saab, S. Kamat, R. Ferril, Thushara Perera, and S. J. Yellin
- Subjects
Physics ,Particle physics ,010308 nuclear & particles physics ,Physics::Instrumentation and Detectors ,Dark matter ,Astrophysics (astro-ph) ,Astrophysics::Instrumentation and Methods for Astrophysics ,General Physics and Astronomy ,FOS: Physical sciences ,Elementary particle ,Supersymmetry ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,7. Clean energy ,01 natural sciences ,Nuclear physics ,Baryon ,WIMP ,Weakly interacting massive particles ,0103 physical sciences ,Neutralino ,High Energy Physics::Experiment ,Cryogenic Dark Matter Search ,010306 general physics ,Nuclear Experiment - Abstract
We report the first results from a search for weakly interacting massive particles (WIMPs) in the Cryogenic Dark Matter Search (CDMS) 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--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, ruling out a significant range of neutralino supersymmetric models. The minimum of this limit curve at the 90% C.L. is 4 x 10^{-43} cm^2 at a WIMP mass of 60 GeV., Comment: 4 pages, 5 figures, submitted to Phys. Rev. Lett; minor clarifications in response to referee's comments
- Published
- 2004
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