Composite CaWO4 detectors for the CRESST-II experiment

Journal article

CRESST-II, standing for Cryogenic Rare Events Search with Superconducting Thermometers phase II, is an experiment searching for Dark Matter. In the LNGS facility in Gran Sasso, Italy, a cryogenic detector setup is operated in order to detect WIMPs by elastic scattering off nuclei, generating phononic lattice excitations and scintillation light. The thermometers used in the experiment consist of a tungsten thin-film structure evaporated onto the CaW04 absorber crystal. The process of evaporation causes a decrease in the scintillation light output. This, together with the need of a big-scale detector production for the upcoming EURECA experiment lead to investigations for producing thermometers on smaller crystals which are glued onto the absorber crystal. In our Run 31 we tested composite detectors for the first time in the Gran Sasso setup. They seem to produce higher light yields as hoped and could provide an additional time based discrimination mechanism for low light yield clamp events. © 2009 American Institute of Physics.

Authors: Kiefer, M; Angloher, G; Bauer, M; Bavykina, I; Bento, A

• Journal: AIP Conference Proceedings
• Volume: 1185
• Pages: 651-654
• Publication date: 2009-01-01
• DOI: 10.1063/1.3292426
• EISSN: 1551-7616
• ISSN: 0094-243X
• Language: English
• Keywords: Epoxy; CaW04; WIMP; Glue; Low temperature detectors; Scintillation detectors; Dark Matter