- Abstract:
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The next generation direct dark matter experiment CRESST-III has a high potential to significantly increase the sensitivity to low-mass WIMPs (mx ≲10 GeV/c2). We present the new CRESST detector module: it consists of a 24 g CaWO4 crystal operated as a phonon detector and a 20x20 mm^2 silicon-on-sapphire light detector. The phonon energy threshold is lowered to ~100 eV and a light detector resolution of typically 5 eV is achieved. A fully-scintillating inner detector housing is realised wh...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Publisher's version
- Files:
-
-
(pdf, 1.8MB)
-
- Publisher copy:
- 10.1088/1742-6596/718/4/042048
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- Publisher:
- Institute of Physics Publisher's website
- Volume:
- 718
- Issue:
- 4
- Pages:
- 042048
- Publication date:
- 2016-08-05
- Acceptance date:
- 2016-05-03
- DOI:
- ISSN:
-
1742-6588 and 1742-6596
- Pubs id:
-
pubs:641119
- URN:
-
uri:79597257-0ea6-4922-ba7a-8ae7a14400f6
- UUID:
-
uuid:79597257-0ea6-4922-ba7a-8ae7a14400f6
- Local pid:
- pubs:641119
- Copyright holder:
- Kraus et al
- Copyright date:
- 2016
- Notes:
- Content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. Published under licence by IOP Publishing Ltd
Conference item
The CRESST-III low-mass WIMP detector
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German Research Foundation
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Helmholtz Alliance for Astroparticle Phyiscs
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Maier-Leibnitz-Laboratorium
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Science & Technology Facilities Council
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