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Hunting for the Invisible: Dark Matter Research

SABRE South aims to unveil the mysteries of dark matter deep underground.

E. Barberio, T. Baroncelli, V. U. Bashu, L. J. Bignell, I. Bolognino, G. Brooks, S. S. Chun, F. Dastgiri, A. R. Duffy, M. B. Froehlich, T. Fruth, G. Fu, G. C. Hill, R. S. James, K. Janssens, S. Kapoor, G. J. Lane, K. T. Leaver, P. McGee, L. J. McKie, P. C. McNamara, J. McKenzie, W. J. D. Melbourne, M. Mews, G. Milana, L. J. Milligan, J. Mould, K. J. Rule, F. Scutti, Z. Slavkovská, O. Stanley, A. E. Stuchbery, B. Suerfu, G. N. Taylor, D. Tempra, T. Tunningly, P. Urquijo, A. G. Williams, Y. Xing, M. J. Zurowski

― 6 min read


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Table of Contents

In the vast universe, stars and galaxies glow brightly. But guess what? There’s a whole lot of stuff out there that doesn’t shine at all. Scientists call this invisible matter "Dark Matter." Think of it as that elusive sock in the laundry that always disappears. We can’t see dark matter directly, but we know it's there because of the way regular matter behaves. It's like knowing there's a ghost in your house because your doors mysteriously creak open!

Enter the SABRE South Detector

SABRE South is a special detector built to hunt down Signals from dark matter. It’s located deep underground at the Stawell Underground Physics Laboratory (SUPL) in Australia. Why so deep? Well, being underground helps shield the detector from other particles and noise that could confuse the results. It’s like hiding from the bright lights of a disco while trying to find the perfect tune!

What is SABRE?

SABRE stands for Sodium Iodide with Active Background REjection. It’s a mouthful, but it basically means the detector is made of sodium iodide crystals that keep unwanted signals at bay. The goal is to see if there’s a pattern in how dark matter might interact with those crystals.

How Does It Work?

The SABRE South detector uses really pure sodium iodide crystals, which are like high-tech pebbles that catch signals from dark matter. These crystals are special because they can pick up tiny energy changes that might happen if dark matter interacts with them.

The Crystal Setup

SABRE South has seven of these crystals, arranged and sealed up in copper containers. It's like wrapping your grandma’s prized cookies in a secure box so no one can mess with them! The total weight of the crystals is either 35 or 50 kilograms. Each crystal is connected to fancy devices called photomultiplier tubes (PMTs) that help detect incoming signals.

The Active Veto

In addition to the crystals, SABRE South has an active veto system. Imagine having a bouncer at a club who stops unwanted guests. This veto system uses a liquid scintillator – which is just a fancy term for a special liquid that can glow – to identify any Background Noise from other sources. If something suspicious happens, it alerts the system!

Challenges of Finding Dark Matter

Detecting dark matter is like fishing without knowing what’s in the water. You can throw out your line, but if you catch a boot instead of a fish, it’s a bit disappointing. The problem is that dark matter is thought to interact really rarely with regular matter. Scientists expect that any signals would be very faint and might get overshadowed by noise from other sources.

Understanding Modulation Patterns

One of the ways to find dark matter is by looking for changes in the signal over time. As the Earth moves through the galactic halo of dark matter, it’s expected that the detector might see a "modulation" – fancy talk for patterns that repeat. For example, the signal might be stronger at different times of the year.

The Science Behind It

Looking for the DAMA/LIBRA Signal

SABRE South is designed to check a previous claim made by another detector called DAMA/LIBRA, which thought it detected a dark matter signal. They reported a constant modulation that suggested something funky was happening. So, SABRE South aims to find out if that signal is real or just a ghost!

Background Noise and Radiogenic Events

The main issue for the SABRE South team is background noise. Just like how people chatting can drown out your favorite song, other radiation sources can obscure the signals they are looking for. That’s where the active veto system comes in handy, trying to keep things as quiet as possible.

The Location Matters

SABRE South is in a very cool spot – 1,025 meters underground! It’s like being deep in a cave, away from all the noise. The rock above acts like a blanket, keeping out unwanted signals. The deeper you go, the better shielded you are, making it easier to focus on the task at hand.

Building the Detector Complex

The Construction Process

Constructing the SABRE South detector wasn’t exactly a walk in the park. It involved careful planning and precise building techniques to ensure everything was perfect. The aim was to create an environment where every event could be measured without interference.

The Veto Shield

To further protect the detector, the team built a shielding structure around it made of layers of steel and high-density polyethylene (HDPE). This is like wearing layers of clothes in winter – the more layers, the less cold you feel! This shielding helps reduce noise from outside, ensuring the detector can focus on catching those elusive dark matter signals.

What to Expect from SABRE South

Expected Performance

By utilizing ultra-pure sodium iodide crystals and a sophisticated veto system, SABRE South is expected to detect signals with a sensitivity that could rule out or confirm the previous dark matter claims. If successful, it could change how we understand the universe and its contents!

Data Collection and Analysis

Once everything is set up and running, the real work starts. The detector will gather data, which scientists will analyze carefully. They’ll look for patterns, filtering out noise to see if there’s any hint of that tricky dark matter.

Funding and Support

SABRE South isn't just the product of a few people’s daydreams. It’s funded and supported by various organizations, making it a collaborative effort. It's like a big team project where everyone plays a part to try to uncover the universe's secrets.

Conclusion

In a nutshell, the SABRE South detector is a highly sophisticated machine designed to search for the elusive dark matter. By building it deep underground, equipping it with ultra-pure crystals, and using smart noise-reduction techniques, the team hopes to shed light on one of science's biggest mysteries.

So, while we may still not have that missing sock, with detectors like SABRE South, we might just be able to find out what’s lurking in the shadows of the universe!

Original Source

Title: The SABRE South Technical Design Report Executive Summary

Abstract: In this Technical Design Report (TDR) we describe the SABRE South detector to be built at the Stawell Underground Physics Laboratory (SUPL). The SABRE South detector is designed to test the long-standing DAMA/LIBRA signal of an annually modulating rate consistent with dark matter by using the same target material. SABRE South uses seven ultra-high purity NaI(Tl) crystals (with a total target mass of either 35 kg or 50 kg), hermetically sealed in copper enclosures that are suspended within a liquid scintillator active veto. High quantum efficiency and low background Hamamatsu R11065 photomultiplier tubes are directly coupled to both ends of the crystal, and enclosed with the crystal in an oxygen free high thermal conductivity copper enclosure. The active veto system consists of 11.6 kL of linear alkylbenzene (LAB) doped with a mixture of fluorophores and contained in a steel vessel, which is instrumented with at least 18 Hamamatsu R5912 photomultipliers. The active veto tags key radiogenic backgrounds intrinsic to the crystals, such as ${^{40}}$K, and is expected to suppress the total background by 27% in the 1-6 keV region of interest. In addition to the liquid scintillator veto, a muon veto is positioned above the detector shielding. This muon veto consists of eight EJ-200 scintillator modules, with Hamamatsu R13089 photomultipliers coupled to both ends. With an expected total background of 0.72 cpd/kg/keV, SABRE South can test the DAMA/LIBRA signal with 5$\sigma$ discovery or 3$\sigma$ exclusion after two years of data taking.

Authors: E. Barberio, T. Baroncelli, V. U. Bashu, L. J. Bignell, I. Bolognino, G. Brooks, S. S. Chun, F. Dastgiri, A. R. Duffy, M. B. Froehlich, T. Fruth, G. Fu, G. C. Hill, R. S. James, K. Janssens, S. Kapoor, G. J. Lane, K. T. Leaver, P. McGee, L. J. McKie, P. C. McNamara, J. McKenzie, W. J. D. Melbourne, M. Mews, G. Milana, L. J. Milligan, J. Mould, K. J. Rule, F. Scutti, Z. Slavkovská, O. Stanley, A. E. Stuchbery, B. Suerfu, G. N. Taylor, D. Tempra, T. Tunningly, P. Urquijo, A. G. Williams, Y. Xing, M. J. Zurowski

Last Update: 2024-11-25 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2411.13889

Source PDF: https://arxiv.org/pdf/2411.13889

Licence: https://creativecommons.org/licenses/by/4.0/

Changes: This summary was created with assistance from AI and may have inaccuracies. For accurate information, please refer to the original source documents linked here.

Thank you to arxiv for use of its open access interoperability.

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