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Direct searches of dark matter with the SABRE South experiment
by Madeleine J. Zurowski
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Submission summary
| Authors (as registered SciPost users): | Madeleine Zurowski |
| Submission information | |
|---|---|
| Preprint Link: | scipost_202210_00015v2 (pdf) |
| Date accepted: | 2023-04-24 |
| Date submitted: | 2022-11-25 01:20 |
| Submitted by: | Zurowski, Madeleine |
| Submitted to: | SciPost Physics Proceedings |
| Proceedings issue: | 14th International Conference on Identification of Dark Matter (IDM2022) |
| Ontological classification | |
|---|---|
| Academic field: | Physics |
| Specialties: |
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| Approach: | Experimental |
Abstract
The SABRE (Sodium-iodide with Active Background REjection) South experiment is a direct dark matter detector, made of radio-pure NaI(Tl) crystals surrounded by a liquid scintillator veto. The achievement of ultra-low background rate is essential to provide a model independent test of the signal observed by the DAMA/LIBRA experiment whose claim has not been verified yet. The SABRE South experiment will be located at the Stawell Underground Physics Laboratory (SUPL), Australia, the first deep underground laboratory in the Southern Hemisphere. The laboratory will not only house rare event physics searches but also measurement facilities to support low background physics experiments and applications like radiobiology and quantum computing. The SABRE South detector commissioning is expected to occur in 2023. This paper details the setup and projections for the experiment, and a brief description of the underground laboratory.
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Published as SciPost Phys. Proc. 12, 029 (2023)