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First results from the Cryogenic Dark Matter Search in the Soudan Underground Laboratory.

Authors :
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 JP
Tomada A
Wang G
Williams J
Yellin S
Young BA
Source :
Physical review letters [Phys Rev Lett] 2004 Nov 19; Vol. 93 (21), pp. 211301. Date of Electronic Publication: 2004 Nov 16.
Publication Year :
2004

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.

Details

Language :
English
ISSN :
0031-9007
Volume :
93
Issue :
21
Database :
MEDLINE
Journal :
Physical review letters
Publication Type :
Academic Journal
Accession number :
15600991
Full Text :
https://doi.org/10.1103/PhysRevLett.93.211301