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CRESST-II: dark matter search with scintillating absorbers

✍ Scribed by G. Angloher; C. Bucci; C. Cozzini; F. von Feilitzsch; T. Frank; D. Hauff; S. Henry; Th. Jagemann; J. Jochum; H. Kraus; B. Majorovits; J. Ninkovic; F. Petricca; F. Pröbst; Y. Ramachers; W. Rau; W. Seidel; M. Stark; S. Uchaikin; L. Stodolsky; H. Wulandari


Publisher
Elsevier Science
Year
2005
Tongue
English
Weight
327 KB
Volume
138
Category
Article
ISSN
0920-5632

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✦ Synopsis


In the CRESST-II experiment, scintillating CaWO 4 crystals are used as absorbers for direct WIMP (weakly interacting massive particles) detection. Nuclear recoils can be discriminated against electron recoils by measuring phonons and scintillation light simultaneously. The absorber crystal and the silicon light detector are read out by tungsten superconducting phase transition thermometers (W-SPTs). Results on the sensitivity of the phonon and the light channel, radiopurity, the scintillation properties of CaWO 4 , and on the WIMP sensitivity are presented.


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The aim of CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) is to search for particle dark matter via elastic scattering off nuclei. The experiment is located at the Laboratori Nazionali del Gran Sasso (LNGS), Italy, and it uses low-background cryogenic detectors with supercond