Linkage Infrastructure, Equipment And Facilities - Grant ID: LE120100181
Funder
Australian Research Council
Funding Amount
$650,000.00
Summary
Strengthening merit-based access and support at the new National Computing Infrastructure petascale supercomputing facility. World-leading high-performance computing is fundamental to Australia's international research success. This facility will provide access to the new National Computational Infrastructure facility by world-leading researchers from six research universities, and sustain ground-breaking work in an increasingly competitive environment.
Stawell Underground Physics Laboratory: Dark matter detector development. This project aims to develop ultra-sensitive detector technology essential for SABRE, a Northern and Southern Hemisphere dual-detector experiment. The SABRE facilities operate to directly detect galactic dark matter. Dark matter makes up 23% of the observable universe but the evidence for its existence is indirect. The direct detection of dark matter would be a discovery on par with gravitational waves and the Higgs boson. ....Stawell Underground Physics Laboratory: Dark matter detector development. This project aims to develop ultra-sensitive detector technology essential for SABRE, a Northern and Southern Hemisphere dual-detector experiment. The SABRE facilities operate to directly detect galactic dark matter. Dark matter makes up 23% of the observable universe but the evidence for its existence is indirect. The direct detection of dark matter would be a discovery on par with gravitational waves and the Higgs boson. This project is an opportunity for Australian research to continue to lead the way in the biggest scientific discoveries of the century and provides opportunities for Australian science in numerous fields ranging from biology to fundamental physics.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE200100078
Funder
Australian Research Council
Funding Amount
$250,000.00
Summary
A particle detector array for the Murchison Widefield Array. The project will construct a particle detector array for the Murchison Widefield Array radio telescope. The array will identify cosmic ray interactions in the Earth's atmosphere, and trigger radio observations. The outcome will be a new capability to study the origin of the highest-energy particles in nature, cosmic rays, and discover new physical processes at energies unreachable by the Large Hadron Collider.
The anticipated benefits ....A particle detector array for the Murchison Widefield Array. The project will construct a particle detector array for the Murchison Widefield Array radio telescope. The array will identify cosmic ray interactions in the Earth's atmosphere, and trigger radio observations. The outcome will be a new capability to study the origin of the highest-energy particles in nature, cosmic rays, and discover new physical processes at energies unreachable by the Large Hadron Collider.
The anticipated benefits are the establishment of the Murchison Widefield Array as a world-leading instrument for astroparticle physics; to lay the foundations for future research with the Square Kilometre Array; and to provide answers to long-standing scientific questions of public interest.Read moreRead less
Detecting cosmic rays using precision radio imaging. This project's aim is to identify the source of the highest-energy particles in nature, cosmic rays, and discover new physical processes at energies unreachable by the Large Hadron Collider.
It will do this by using the Murchison Widefield Array radio telescope to detect the sub-microsecond pulses from cosmic ray interactions in the Earth's atmosphere. The project's intended outcome is a sample of thousands of cosmic ray events, and a new tec ....Detecting cosmic rays using precision radio imaging. This project's aim is to identify the source of the highest-energy particles in nature, cosmic rays, and discover new physical processes at energies unreachable by the Large Hadron Collider.
It will do this by using the Murchison Widefield Array radio telescope to detect the sub-microsecond pulses from cosmic ray interactions in the Earth's atmosphere. The project's intended outcome is a sample of thousands of cosmic ray events, and a new technique to analyse the structure within them.
The anticipated benefits are the establishment of the Murchison Widefield Array as a world-leading instrument for astroparticle physics, new knowledge of high-energy astro and particle physics, and advances and training in fast signal processing methods.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE160100080
Funder
Australian Research Council
Funding Amount
$195,000.00
Summary
Detector system for the First Australian Experiment on Dark Matter. Detector system for the first Australian experiment on dark matter:
This project involves the installation of equipment for an experiment to detect our galaxy's dark matter via nuclear recoil. Here in the Southern Hemisphere, we have a crucial advantage in the search for dark matter via direct detection, which will allow us to independently test the most persistent and enigmatic signal in the worldwide dark matter detection eff ....Detector system for the First Australian Experiment on Dark Matter. Detector system for the first Australian experiment on dark matter:
This project involves the installation of equipment for an experiment to detect our galaxy's dark matter via nuclear recoil. Here in the Southern Hemisphere, we have a crucial advantage in the search for dark matter via direct detection, which will allow us to independently test the most persistent and enigmatic signal in the worldwide dark matter detection effort. The detector system, called SABRE South, is designed to be paired with a matching one in the Northern Hemisphere. The research program is addressing one of the most important unsolved problems of contemporary science.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE170100162
Funder
Australian Research Council
Funding Amount
$415,000.00
Summary
Full scale detector system for dark matter. This project aims to complete a detector system to detect dark matter via nuclear recoil in the Stawell Underground Physics Laboratory (SUPL). The Southern Hemisphere location and the ultra-pure crystals are a crucial advantage in the search for dark matter via direct detection. The detector system will provide the sensitivity needed to test the most persistent and enigmatic signal in the world-wide dark matter direct detection search and ensure Austra ....Full scale detector system for dark matter. This project aims to complete a detector system to detect dark matter via nuclear recoil in the Stawell Underground Physics Laboratory (SUPL). The Southern Hemisphere location and the ultra-pure crystals are a crucial advantage in the search for dark matter via direct detection. The detector system will provide the sensitivity needed to test the most persistent and enigmatic signal in the world-wide dark matter direct detection search and ensure Australian leadership in this field. The discovery of dark matter is expected to be as important as that of the Higgs boson and gravitational waves.Read moreRead less
Structure of Hadronic Excitations from Lattice Quantum Chromodynamics. Quantum chromodynamics describes the fundamental strong interactions between quarks and gluons as they compose hadrons such as the proton or neutron. Beyond these lowest-energy systems, the quantum mechanical excitation spectra display a rich and complex structure. Remarkably, little is known about the internal structure of these states. The central goal of this project is to unveil the nature of hadrons and their excited sta ....Structure of Hadronic Excitations from Lattice Quantum Chromodynamics. Quantum chromodynamics describes the fundamental strong interactions between quarks and gluons as they compose hadrons such as the proton or neutron. Beyond these lowest-energy systems, the quantum mechanical excitation spectra display a rich and complex structure. Remarkably, little is known about the internal structure of these states. The central goal of this project is to unveil the nature of hadrons and their excited states using the first principles approach of lattice gauge theory. By elucidating aspects of hadron structure in terms of the most fundamental non-perturbative quark and gluon fields, the project will create new knowledge impacting on renowned experimental programs at international facilities.Read moreRead less
ARC Centre of Excellence for Dark Matter Particle Physics. The Centre of Excellence for Dark Matter Particle Physics will deliver breakthroughs in our understanding of the Universe through the pursuit of the discovery of dark matter particles which comprise 80% of the mass of the universe. It assembles for the first time a strong and diverse team of physicists from particle, nuclear, and quantum physics as well as particle astrophysics. It will deliver high-profile experiments using new cutting- ....ARC Centre of Excellence for Dark Matter Particle Physics. The Centre of Excellence for Dark Matter Particle Physics will deliver breakthroughs in our understanding of the Universe through the pursuit of the discovery of dark matter particles which comprise 80% of the mass of the universe. It assembles for the first time a strong and diverse team of physicists from particle, nuclear, and quantum physics as well as particle astrophysics. It will deliver high-profile experiments using new cutting-edge technologies. The Centre will exploit the unique geographical location of the first underground physics lab in the Southern Hemisphere. The ultra-sensitive detectors and ultra-low radiation techniques will translate into a broad range of industrial applications and train a new generation of scientists.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE180100042
Funder
Australian Research Council
Funding Amount
$621,834.00
Summary
Australian dark matter detector for high mass axions. This project aims to provide the necessary equipment to allow an Australian Dark Matter Axion Haloscope, with significantly increased sensitivity by providing a milliKelvin environment and a 14 T magnet to drive axion-to-photon conversions. Dark matter is a fundamental component of the universe yet the nature of its composition is still unknown. There is growing evidence that it is comprised of axions, a low energy, weakly interacting particl ....Australian dark matter detector for high mass axions. This project aims to provide the necessary equipment to allow an Australian Dark Matter Axion Haloscope, with significantly increased sensitivity by providing a milliKelvin environment and a 14 T magnet to drive axion-to-photon conversions. Dark matter is a fundamental component of the universe yet the nature of its composition is still unknown. There is growing evidence that it is comprised of axions, a low energy, weakly interacting particle. The precision measurement tools developed by this project will have the potential to contribute both to the economy, via commercialisation, and to national security, via future applications to radar, communication and the development of engineered quantum systems.Read moreRead less