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Probing spin-dependent dark matter interactions with $$^6$$Li

Abstract:
Using CaWO$_4$ crystals as cryogenic calorimeters, the CRESST experiment searches for nuclear recoils caused by the scattering of potential Dark Matter particles. A reliable identification of a potential signal crucially depends on an accurate background model. In this work we introduce an improved normalisation method for CRESST's model of the electromagnetic backgrounds. Spectral templates, based on Geant4 simulations, are normalised via a Bayesian likelihood fit to experimental background data. Contrary to our previous work, no assumption of partial secular equilibrium is required, which results in a more robust and versatile applicability. Furthermore, considering the correlation between all background components allows us to explain 82.7% of the experimental background within [1 keV, 40 keV], an improvement of 18.6% compared to our previous method.Comment: 24 pages, 14 figures, submitted to EPJ
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1140/epjc/s10052-022-10140-3

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Role:
Author
ORCID:
0000-0002-8768-290X
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Role:
Author
ORCID:
0000-0002-3817-6015
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Role:
Author
ORCID:
0000-0001-6260-0325
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Role:
Author
ORCID:
0000-0002-2374-7620


Publisher:
SpringerOpen
Journal:
The European Physical Journal C More from this journal
Volume:
82
Issue:
3
Pages:
207
Article number:
207
Publication date:
2022-03-09
DOI:
EISSN:
1434-6052
ISSN:
1434-6044


Language:
English
Keywords:
Pubs id:
1248792
Local pid:
pubs:1248792
Source identifiers:
W4220952207
Deposit date:
2026-04-10
ARK identifier:
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