Abstract
Recently low-mass dark matter direct searches have been hindered by a low-energy background, drastically reducing the physics reach of the experiments. In the CRESST-III experiment, this signal is characterised by a significant increase of events below 200 eV. As the origin of this background is still unknown, it became necessary to develop new detector designs to reach a better understanding of the observations. Within the CRESST collaboration, three new different detector layouts have been developed, and they are presented in this contribution.
| Originalsprache | Englisch |
|---|---|
| Seiten (von - bis) | 393-401 |
| Seitenumfang | 9 |
| Fachzeitschrift | Journal of Low Temperature Physics |
| Jahrgang | 216 |
| Ausgabenummer | 1-2 |
| DOIs | |
| Publikationsstatus | Veröffentlicht - Juli 2024 |
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