Beta/gamma and alpha backgrounds in CRESST-II Phase 2
arXiv:1410.4188 · doi:10.1088/1475-7516/2015/06/030
Abstract
The experiment CRESST-II aims at the detection of dark matter with scintillating CaWO crystals operated as cryogenic detectors. Recent results on spin-independent WIMP-nucleon scattering from the CRESST-II Phase 2 allowed to probe a new region of parameter space for WIMP masses below 3 GeV/c. This sensitivity was achieved after background levels were reduced significantly. We present extensive background studies of a CaWO crystal, called TUM40, grown at the Technische Universität München. The average beta/gamma rate of 3.51/[kg keV day] (1-40 keV) and the total intrinsic alpha activity from natural decay chains of mBq/kg are the lowest reported for CaWO detectors. Contributions from cosmogenic activation, surface-alpha decays, external radiation and intrinsic alpha/beta emitters are investigated in detail. A Monte-Carlo based background decomposition allows to identify the origin of the majority of beta/gamma events in the energy region relevant for dark matter search.
17 pages, 7 figures, 3 tables
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- Annual Modulation in Direct Dark Matter Searches
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- A prototype detector for the CRESST-III low-mass dark matter search
- Radioactive contamination of scintillators
- A detector module with highly efficient surface-alpha event rejection operated in CRESST-II Phase 2
- Dark-Photon Search using Data from CRESST-II Phase 2
- Radiopurity of a kg-scale PbWO cryogenic detector produced from archaeological Pb for the RES-NOVA experiment
- Limits on momentum-dependent asymmetric dark matter with CRESST-II
- Cosmogenic activation in double beta decay experiments
- Cryogenic phonon-scintillation detectors with PMT readout for rare event search experiments
- High-Dimensional Bayesian Likelihood Normalisation for CRESST's Background Model