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CRESST - status and future

Abstract:
We present results on WIMP dark matter interaction, obtained using cryogenic phonon-scintillation detectors. The targets are CaWO4 scintillating crystals with phonon sensors, while scintillation is detected with an associated cryogenic light detector. The combination of phonon and light signals leads to a strong suppression of nonnuclear recoil backgrounds. Results obtained before the upgrade of CRESST are presented and a status report on the upgrade itself is given.
Publication status:
Published

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Publisher copy:
10.1016/j.nuclphysbps.2007.08.156

Authors

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Particle Physics
Role:
Author


Journal:
NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS More from this journal
Volume:
173
Pages:
104-107
Publication date:
2007-11-01
Event title:
7th UCLA Symposium on Sources and Detection of Dark Matter and Dark Energy in the Universe
DOI:
ISSN:
0920-5632


Keywords:
Pubs id:
pubs:11367
UUID:
uuid:e9007ec5-5982-401e-9a3b-64c8a96a5e26
Local pid:
pubs:11367
Source identifiers:
11367
Deposit date:
2012-12-19
ARK identifier:

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