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The CRESST-III low-mass WIMP detector

Abstract:
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 which efficiently rejects events from surface alpha decays. The CaWO4 sticks holding the target crystal are also operated as calorimeters to discriminate all possible artefacts related to the support structure. A projection for the sensitivity to spin-independent WIMP-nucleon scattering is given for the first phase of CRESSTIII which will start beginning of 2016.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1088/1742-6596/718/4/042048

Authors



Publisher:
Institute of Physics
Host title:
Journal of Physics: Conference Series
Journal:
Journal of Physics: Conference Series More from this journal
Volume:
718
Issue:
4
Pages:
042048
Publication date:
2016-08-01
Acceptance date:
2016-05-03
DOI:
ISSN:
1742-6588 and 1742-6596


Pubs id:
pubs:641119
UUID:
uuid:79597257-0ea6-4922-ba7a-8ae7a14400f6
Local pid:
pubs:641119
Source identifiers:
641119
Deposit date:
2016-11-29

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