Issue |
EPJ Web Conf.
Volume 232, 2020
Heavy Ion Accelerator Symposium (HIAS 2019)
|
|
---|---|---|
Article Number | 01002 | |
Number of page(s) | 6 | |
Section | Facilities and Applications | |
DOI | https://doi.org/10.1051/epjconf/202023201002 | |
Published online | 06 April 2020 |
https://doi.org/10.1051/epjconf/202023201002
SABRE and the Stawell Underground Physics Laboratory Dark Matter Research at the Australian National University
1
Department of Nuclear Physics, Research School of Physics, The Australian National University, Canberra, ACT 2601, Australia
2
School of Physics, The University of Melbourne, Melbourne, VIC 3010, Australia
3
School of Science, The University of New South Wales, UNSW Canberra, Canberra, ACT 2612, Australia
* e-mail: lindsey.bignell@anu.edu.au
Published online: 6 April 2020
The direct detection of dark matter is a key problem in astroparticle physics that generally requires the use of deep-underground laboratories for a low-background environment where the rare signals from dark matter interactions can be observed. This work reports on the Stawell Underground Physics Laboratory – currently under construction and the first such laboratory in the Southern Hemisphere – and the associated research program. A particular focus will be given to ANU’s contribution to SABRE, a NaI:Tl dark matter, direct detection experiment that aims to confirm or refute the long-standing DAMA result. Preliminary measurements of the NaI:Tl quenching factor and characterisation of the SABRE liquid scintillator veto are reported.
© The Authors, published by EDP Sciences, 2020
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