The SABRE South experiment at the Stawell Underground Physics Laboratory
M. Mews*, 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, 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. Zurowskiet al. (click to show)
Pre-published on:
November 25, 2022
Published on:
June 15, 2023
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.
DOI: https://doi.org/10.22323/1.414.1127
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