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Limits on WIMP dark matter using sapphire cryogenic detectors

Authors :
Monica Sisti
F. Pröbst
J. Marchese
M. Bruckmayer
T. Frank
O. Meier
V. Jörgens
D. Hauff
A. Rulofs
W. Seidel
R. Keeling
Susan Cooper
J. Schnagl
P. DiStefano
Y. Ramachers
Th. Jagemann
Leo Stodolsky
M. Stark
I. Sergeyev
G. Angloher
C. Cozzini
J. Jochum
F. von Feilitzsch
Sergey Uchaikin
C. Bucci
M Bühler
H. Kraus
L. Zerle
Urmas Nagel
M. Loidl
H. R. T. Wulandari
Institut de Physique Nucléaire de Lyon (IPNL)
Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL)
Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)
Flores, Sylvie
Source :
Astroparticle Physics, Astroparticle Physics, Elsevier, 2002, 18, pp.43-55
Publication Year :
2002
Publisher :
HAL CCSD, 2002.

Abstract

Data taken by CRESST with a cryogenic detector system based on 262 g sapphire crystals has been used to place limits on WIMP dark matter in the Galactic Halo. The experiment was especially sensitive for low-mass WIMPs with spin-dependent cross sections and improves on existing limits in this region. © 2002 Elsevier Science B.V. All rights reserved.

Details

Language :
English
ISSN :
09276505
Database :
OpenAIRE
Journal :
Astroparticle Physics, Astroparticle Physics, Elsevier, 2002, 18, pp.43-55
Accession number :
edsair.doi.dedup.....4011f8a431081dca8bdab96887e8489e