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Exclusion Limits on the WIMP-Nucleon Cross-Section from the Cryogenic Dark Matter Search

Authors :
M. B. Crisler
H. N. Nelson
R. Bunker
S. Eichblatt
J. Emes
T. A. Shutt
E. E. Haller
P. L. Brink
Alexander Bolozdynya
Josef Jochum
B. L. Dougherty
R. L. Dixon
Ronald R. Ross
G. Smith
M. J. Penn
Stephen H. White
R. W. Schnee
J. Hellmig
A. Da Silva
Bernard Sadoulet
J. P. Castle
Andrew Sonnenschein
A. C. Cummings
F. P. Lipschultz
A. Lu
John M. Martinis
B. Neuhauser
Kent D. Irwin
Peter D. Barnes
A. L. Spadafora
J. D. Taylor
P. Shestople
R. Abusaidi
W. Stockwell
Betty A. Young
Boris Pritychenko
R. M. Clarke
P. Colling
Vuk Mandic
Blas Cabrera
Sunil Golwala
A. K. Davies
D. Driscoll
R. J. Gaitskell
D. N. Seitz
D. S. Akerib
Daniel E. Hale
Sae Woo Nam
D. A. Bauer
M. C. Perillo Isaac
D. O. Caldwell
Tarek Saab
Thushara Perera
S. J. Yellin
Martin E. Huber
A. R. Smith
Publication Year :
2000
Publisher :
arXiv, 2000.

Abstract

The Cryogenic Dark Matter Search (CDMS) employs low-temperature Ge and Si detectors to search for Weakly Interacting Massive Particles (WIMPs) via their elastic-scattering interactions with nuclei while discriminating against interactions of background particles. For recoil energies above 10 keV, events due to background photons are rejected with >99.9% efficiency, and surface events are rejected with >95% efficiency. The estimate of the background due to neutrons is based primarily on the observation of multiple-scatter events that should all be neutrons. Data selection is determined primarily by examining calibration data and vetoed events. Resulting efficiencies should be accurate to about 10%. Results of CDMS data from 1998 and 1999 with a relaxed fiducial-volume cut (resulting in 15.8 kg-days exposure on Ge) are consistent with an earlier analysis with a more restrictive fiducial-volume cut. Twenty-three WIMP candidate events are observed, but these events are consistent with a background from neutrons in all ways tested. Resulting limits on the spin-independent WIMP-nucleon elastic-scattering cross-section exclude unexplored parameter space for WIMPs with masses between 10-70 GeV c^{-2}. These limits border, but do not exclude, parameter space allowed by supersymmetry models and accelerator constraints. Results are compatible with some regions reported as allowed at 3-sigma by the annual-modulation measurement of the DAMA collaboration. However, under the assumptions of standard WIMP interactions and a standard halo, the results are incompatible with the DAMA most likely value at >99.9% CL, and are incompatible with the model-independent annual-modulation signal of DAMA at 99.99% CL in the asymptotic limit.<br />40 pages, 49 figures (4 in color), submitted to Phys. Rev. D; v.2:clarified conclusions, added content and references based on referee's and readers' comments; v.3: clarified introductory sections, added figure based on referee's comments

Details

Database :
OpenAIRE
Accession number :
edsair.doi.dedup.....462b23cfd8b1a5fed82934eadb80abe8
Full Text :
https://doi.org/10.48550/arxiv.astro-ph/0002471