ARC Centre of Excellence for Gravitational Wave Discovery. This Centre aims to explore the historic first detections of gravitational waves to understand the extreme physics of black holes and warped spacetime, and inspire the next generation of Australian scientists and engineers. The next-generation gravity wave detectors will enable a thousand-fold increase in detection volume and result in the new gravitational wave discoveries, triggering a new era of gravitational wave astrophysics. Buil ....ARC Centre of Excellence for Gravitational Wave Discovery. This Centre aims to explore the historic first detections of gravitational waves to understand the extreme physics of black holes and warped spacetime, and inspire the next generation of Australian scientists and engineers. The next-generation gravity wave detectors will enable a thousand-fold increase in detection volume and result in the new gravitational wave discoveries, triggering a new era of gravitational wave astrophysics. Building on decades of Australian investment in gravitational wave and pulsar science, this Centre will coalesce research activities into a focussed national programme whose discoveries are intended to experimentally validate Einstein’s General Theory of Relativity and educate the public about the wonders of Einstein's Universe.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE210100015
Funder
Australian Research Council
Funding Amount
$1,680,000.00
Summary
The Cherenkov Telescope Array - From Production towards Operation. The Cherenkov Telescope Array is a transformational facility in very-high-energy gamma-ray astronomy. It will be 10 times more sensitive than current instruments and will revolutionise many topics in high energy astrophysics, and in astro-particle physics such as dark matter. Over 1000 scientists from over 30 countries are involved and the first telescopes on the southern hemisphere site in Chile will be installed from about 2021 ....The Cherenkov Telescope Array - From Production towards Operation. The Cherenkov Telescope Array is a transformational facility in very-high-energy gamma-ray astronomy. It will be 10 times more sensitive than current instruments and will revolutionise many topics in high energy astrophysics, and in astro-particle physics such as dark matter. Over 1000 scientists from over 30 countries are involved and the first telescopes on the southern hemisphere site in Chile will be installed from about 2021. This project will ensure Australia's contribution to complete the facility, leading into its operations phase (starting in 2027). It will also fund unique optical astronomy hardware that will enable Australian scientific leadership in supporting some of the Cherenkov Telescope Array's Key Science Projects.
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Linkage Infrastructure, Equipment And Facilities - Grant ID: LE150100070
Funder
Australian Research Council
Funding Amount
$270,000.00
Summary
The Cherenkov Telescope Array. The Cherenkov Telescope Array: The Cherenkov Telescope Array (CTA) is a major advance in very high energy gamma-ray astronomy. It will be ten times more sensitive than current instruments and will transform many topics in high energy astrophysics concerning extreme particle acceleration, and in astro-particle physics such as dark matter. Over 1000 scientists from over 25 countries are involved and prototype telescopes are under construction. This project will enabl ....The Cherenkov Telescope Array. The Cherenkov Telescope Array: The Cherenkov Telescope Array (CTA) is a major advance in very high energy gamma-ray astronomy. It will be ten times more sensitive than current instruments and will transform many topics in high energy astrophysics concerning extreme particle acceleration, and in astro-particle physics such as dark matter. Over 1000 scientists from over 25 countries are involved and prototype telescopes are under construction. This project will enable a hardware contribution to the pre-production array of telescopes, bringing with it full membership, plus access to all data and core science programmes of CTA. Australian astronomers can then influence astrophysics goals of CTA, and add new scientific value to Australia's radio astronomical facilities.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE170100104
Funder
Australian Research Council
Funding Amount
$1,390,000.00
Summary
The Cherenkov Telescope Array - Production phase. This project aims to ensure Australia’s contribution to the five-year production phase of the Cherenkov Telescope Array (CTA), a very high energy gamma-ray astronomy instrument that is expected to transform both high energy astrophysics and astro-particle physics. Gamma-ray astronomy probes extreme processes in the Universe such as exploding stars, black holes, and mysterious dark matter. The project will maintain Australian access to all data an ....The Cherenkov Telescope Array - Production phase. This project aims to ensure Australia’s contribution to the five-year production phase of the Cherenkov Telescope Array (CTA), a very high energy gamma-ray astronomy instrument that is expected to transform both high energy astrophysics and astro-particle physics. Gamma-ray astronomy probes extreme processes in the Universe such as exploding stars, black holes, and mysterious dark matter. The project will maintain Australian access to all data and key science programmes of the CTA. Australian astronomers will be able to directly influence the major astrophysics goals of CTA, and link in with Australia's flagship astronomical infrastructure. This is expected to benefit astrophysics, big data processing, electronics, atmospheric physics and optics.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE210100002
Funder
Australian Research Council
Funding Amount
$3,000,000.00
Summary
Australian Partnership in Advanced LIGO+: continuation. The aim of this project is, in collaboration with the USA and UK, to complete the installation and commissioning of the Advanced LIGO+ facilities in the USA in order to bring them to design sensitivity. These facilities expect to increase the event rate of gravitational wave signals by a factor of 125. This should lead to daily detections and the observation of new sources of gravitational waves. Given that only 5% of the universe is detect ....Australian Partnership in Advanced LIGO+: continuation. The aim of this project is, in collaboration with the USA and UK, to complete the installation and commissioning of the Advanced LIGO+ facilities in the USA in order to bring them to design sensitivity. These facilities expect to increase the event rate of gravitational wave signals by a factor of 125. This should lead to daily detections and the observation of new sources of gravitational waves. Given that only 5% of the universe is detectable by telescopes, the impact of gravitational wave detections on our understanding of the universe is inestimable. Australian partnership intends to enable our physicists and astronomers to be at the vanguard of this brand new field and inspire a new generation to study the physical sciences.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
ARC Centre of Excellence for Gravitational Wave Discovery. ARC Centre of Excellence for Gravitational Wave Discovery. The mission of our Centre is to use gravitational waves to investigate the fundamental nature of relativistic gravity, ultra-dense matter, and cosmology. This will generate critical discoveries that cement Australia's leadership role in the gravitational wave mega-science instruments of the 2030s and 2040s. By bringing together a world-class team with broad and complementary expe ....ARC Centre of Excellence for Gravitational Wave Discovery. ARC Centre of Excellence for Gravitational Wave Discovery. The mission of our Centre is to use gravitational waves to investigate the fundamental nature of relativistic gravity, ultra-dense matter, and cosmology. This will generate critical discoveries that cement Australia's leadership role in the gravitational wave mega-science instruments of the 2030s and 2040s. By bringing together a world-class team with broad and complementary expertise we will develop core technologies for future detectors, discover new sources of gravitational waves, probe fundamental physics, and lay the foundations for an Australian gravitational wave observatory. Our discoveries will inspire Australia's youth to pursue high tech careers and position our staff and students to become leaders in both industry and academia.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