The SABRE South experiment at the Stawell Underground Physics Laboratory

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. MewsW. 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, M. J. Zurowski

    Research output: Contribution to journalConference articlepeer-review

    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.

    Original languageEnglish
    Article number1127
    JournalProceedings of Science
    Volume414
    Publication statusPublished - 2022
    Event41st International Conference on High Energy Physics, ICHEP 2022 - Bologna, Italy
    Duration: 6 Jul 202213 Jul 2022

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