The SABRE South experiment at the Stawell Underground Physics Laboratory
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(Published version)
Date
2022
Authors
Barberio, E.
Baroncelli, T.
Bignell, L.J.
Bolognino, I.
Brooks, G.
Dastgiri, F.
Duffy, A.R.
Froehlich, M.
Fu, G.
Gerathy, M.S.M.
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Conference paper
Citation
Proceedings of Science, 2022, vol.414, pp.1127-1-1127-4
Statement of Responsibility
E. Barberio, T. Baroncelli, L. J. Bignell, I. Bolognino, G. Brooks, F. Dastgiri, A. R. Duffy, M. Froehlich, G. Fu, M. S. M. Gerathy, G. C. Hill, S. Krishnan, G. J. Lane, G. Lawrence, K. T. Leaver, I. Mahmood, P. McGee, L. McKie, P. C. McNamara, M. Mews, W. J. D. Melbourne, G. Milana, L. J. Milligan, J. Mould, F. Scutti, Z. Slavkovská, N. J. Spinks, O. Stanley, A. E. Stuchbery, G. N. Taylor, P. Urquijo, A. G. Williams, Y. Y. Zhong, and M. J. Zurowski
Conference Name
International Conference on High Energy physics (ICHEP) (6 Jul 2022 - 13 Jul 2022 : Bologna, Italy)
Abstract
The SABRE (Sodium iodide with Active Background REjection) experiment aims to provide a model independent test of the signal observed by DAMA/LIBRA by detecting an annual modulation from dark matter interactions in ultra-high purity NaI(Tl) crystals. SABRE consists of two detectors: SABRE North, located at the Laboratori Nazionali del Gran Sasso (LNGS), and SABRE South, located at the newly completed Stawell Underground Physics Laboratory (SUPL) in Stawell, Australia - the first deep underground laboratory in the Southern Hemisphere. Here we present the status of both the SABRE South experiment and SUPL.
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© Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0).