The SABRE South Experiment at the Stawell Underground Physics Laboratory
I. Bolognino

TL;DR
The SABRE South experiment at SUPL aims to detect dark matter-induced annual modulation signals using ultra-pure NaI(Tl) crystals, with a focus on background mitigation and site-specific effects, to test DAMA/LIBRA's findings.
Contribution
This paper details the setup, background mitigation strategies, and site-specific considerations for the SABRE South dark matter detection experiment at SUPL.
Findings
Construction of SUPL underground lab completed in 2022
Background understanding and mitigation strategies developed
Commissioning of SABRE South expected in 2023
Abstract
The SABRE (Sodium iodide with Active Background REjection) experiment aims to detect an annual rate modulation from dark matter interactions in ultra-high purity NaI(Tl) crystals in order to provide a model independent test of the signal observed by DAMA/LIBRA. It is made up of two separate detectors; SABRE South located at the Stawell Underground Physics Laboratory (SUPL), in regional Victoria, Australia, and SABRE North at the Laboratori Nazionali del Gran Sasso (LNGS). SABRE South is designed to disentangle seasonal or site-related effects from the dark matter-like modulated signal by using an active veto and muon detection system. Ultra-high purity NaI(Tl) crystals are immersed in a linear alkyl benzene (LAB) based liquid scintillator veto, further surrounded by passive steel and polyethylene shielding and a plastic scintillator muon veto. Significant work has been undertaken to…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Atomic and Subatomic Physics Research · Particle physics theoretical and experimental studies
