# Geant4-based electromagnetic background model for the CRESST dark matter   experiment

**Authors:** CRESST Collaboration: A.H. Abdelhameed, G. Angloher, P. Bauer, A., Bento, E. Bertoldo, R. Breier, C. Bucci, L. Canonica, A. D'Addabbo, S. Di, Lorenzo, A. Erb, F. v. Feilitzsch, N. Ferreiro Iachellini, S. Fichtinger, A., Fuss, P. Gorla, D. Hauff, M. Je\v{s}kovsk\'y, J. Jochum, J. Kaizer, A., Kinast, H. Kluck, H. Kraus, A. Langenk\"amper, M. Mancuso, V. Mokina, E., Mondrag\'on, M. Olmi, T. Ortmann, C. Pagliarone, V. Palu\v{s}ov\'a, L., Pattavina, F. Petricca, W. Potzel, P. Povinec, F. Pr\"obst, F. Reindl, J., Rothe, K. Sch\"affner, J. Schieck, V. Schipperges, D. Schmiedmayer, S., Sch\"onert, C. Schwertner, M. Stahlberg, L. Stodolsky, C. Strandhagen, R., Strauss, C. T\"urko\u{g}lu, I. Usherov, M. Willers, V. Zema, J. Zeman

arXiv: 1908.06755 · 2019-11-22

## TL;DR

This paper presents a Geant4-based simulation model that effectively explains a significant portion of the electromagnetic background in the CRESST dark matter experiment, aiding in background understanding and reduction.

## Contribution

The study develops a detailed Monte Carlo simulation model of electromagnetic backgrounds specific to CRESST, improving background estimation accuracy.

## Key findings

- Explains up to 68% of electromagnetic background in 1-40 keV range.
- Uses Geant4 simulations tailored to CRESST detector materials.
- Provides insights for background mitigation in dark matter searches.

## Abstract

The CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) dark matter search experiment aims for the detection of dark matter particles via elastic scattering off nuclei in $\mathrm{CaWO_4}$ crystals. To understand the CRESST electromagnetic background due to the bulk contamination in the employed materials, a model based on Monte Carlo simulations was developed using the Geant4 simulation toolkit. The results of the simulation are applied to the TUM40 detector module of CRESST-II phase 2. We are able to explain up to $(68 \pm 16)\,\mathrm{\%}$ of the electromagnetic background in the energy range between $1\,\mathrm{keV}$ and $40\,\mathrm{keV}$.

## Full text

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## Figures

33 figures with captions in the complete paper: https://tomesphere.com/paper/1908.06755/full.md

## References

35 references — full list in the complete paper: https://tomesphere.com/paper/1908.06755/full.md

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Source: https://tomesphere.com/paper/1908.06755