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Akerib DS, Attisha MJ, Bailey CN, Baudis L, Bauer DA, Brink PL, Brusov PP, Bunker R, Cabrera B, Caldwell DO, Chang CL, Cooley J, Crisler MB, Cushman P, Daal M, Dixon R, Dragowsky MR, Driscoll DD, Duong L, Ferril R, Filippini J, Gaitskell RJ, Golwala SR, Grant DR, Hennings-Yeomans R, Holmgren D, Huber ME, Kamat S, Leclercq S, Lu A, Mahapatra R, Mandic V, Meunier P, Mirabolfathi N, Nelson H, Nelson R, Ogburn RW, Perera TA, Pyle M, Ramberg E, Rau W, Reisetter A, Ross RR, Sadoulet B, Sander J, Savage C, Schnee RW, Seitz DN, Serfass B, Sundqvist KM, Thompson JPF, Wang G, Yellin S, Yoo J, Young BA. Limits on spin-independent interactions of weakly interacting massive particles with nucleons from the two-tower run of the cryogenic dark matter search. Phys Rev Lett 2006; 96:011302. [PMID: 16486434 DOI: 10.1103/physrevlett.96.011302] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 09/09/2005] [Indexed: 05/06/2023]
Abstract
We report new results from the Cryogenic Dark Matter Search (CDMS II) at the Soudan Underground Laboratory. Two towers, each consisting of six detectors, were operated for 74.5 live days, giving spectrum-weighted exposures of 34 (12) kg d for the Ge (Si) targets after cuts, averaged over recoil energies 10-100 keV for a weakly interacting massive particle (WIMP) mass of 60 GeV/c2. A blind analysis was conducted, incorporating improved techniques for rejecting surface events. No WIMP signal exceeding expected backgrounds was observed. When combined with our previous results from Soudan, the 90% C.L. upper limit on the spin-independent WIMP-nucleon cross section is 1.6 x 10(-43) cm2 from Ge and 3 x 10(-42) cm2 from Si, for a WIMP mass of 60 GeV/c2. The combined limit from Ge (Si) is a factor of 2.5 (10) lower than our previous results and constrains predictions of supersymmetric models.
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Affiliation(s)
- D S Akerib
- Department of Physics, Case Western Reserve University, Cleveland, Ohio 44106, USA
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Akerib DS, Alvaro-Dean J, Armel-Funkhouser MS, Attisha MJ, Baudis L, Bauer DA, Beaty J, Brink PL, Bunker R, Burke SP, Cabrera B, Caldwell DO, Callahan D, Castle JP, Chang CL, Choate R, Crisler MB, Cushman P, Dixon R, Dragowsky MR, Driscoll DD, Duong L, Emes J, Ferril R, Filippini J, Gaitskell RJ, Haldeman M, Hale D, Holmgren D, Huber ME, Johnson B, Johnson W, Kamat S, Kozlovsky M, Kula L, Kyre S, Lambin B, Lu A, Mahapatra R, Manalaysay AG, Mandic V, May J, McDonald R, Merkel B, Meunier P, Mirabolfathi N, Morrison S, Nelson H, Nelson R, Novak L, Ogburn RW, Orr S, Perera TA, Perillo Isaac MC, Ramberg E, Rau W, Reisetter A, Ross RR, Saab T, Sadoulet B, Sander J, Savage C, Schmitt RL, Schnee RW, Seitz DN, Serfass B, Smith A, Smith G, Spadafora AL, Sundqvist K, Thompson JPF, Tomada A, Wang G, Williams J, Yellin S, Young BA. First results from the Cryogenic Dark Matter Search in the Soudan Underground Laboratory. Phys Rev Lett 2004; 93:211301. [PMID: 15600991 DOI: 10.1103/physrevlett.93.211301] [Citation(s) in RCA: 8] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/04/2004] [Indexed: 05/24/2023]
Abstract
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 x 10(-43) cm2 at a WIMP mass of 60 GeV/c2.
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Affiliation(s)
- D S Akerib
- Department of Physics, Case Western Reserve University, Cleveland, Ohio 44106, USA
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