A Stress-relax Model for Stellar Flares. This project aims to improve our ability to predict solar and stellar flares by developing a theoretical model for the build-up and release of magnetic stress in stellar atmospheres. Solar flares are the most energetic events in the solar system, and together with associated coronal mass ejections can create hazardous conditions in our local space environment. Stellar flares are thousands of times more energetic and produce dangerous space weather for exo ....A Stress-relax Model for Stellar Flares. This project aims to improve our ability to predict solar and stellar flares by developing a theoretical model for the build-up and release of magnetic stress in stellar atmospheres. Solar flares are the most energetic events in the solar system, and together with associated coronal mass ejections can create hazardous conditions in our local space environment. Stellar flares are thousands of times more energetic and produce dangerous space weather for exoplanets orbiting flare stars. Expected outcomes include insight into the flare mechanism, and new approaches to flare prediction. The major potential benefit is improved solar and stellar space weather forecasting to protect human safety and infrastructure.Read moreRead less
Measuring critical background in the Australian search for dark matter. This project aims to develop ultra-sensitive detector technology essential for SABRE, a world-wide experiment with detectors in both the Northern and Southern Hemispheres which are operated together to directly detect the dark matter halo of our Milky Way galaxy. Dark matter makes up nearly five times more mass in the universe than everything we can see, yet it has never been detected in the laboratory. SABRE South will be i ....Measuring critical background in the Australian search for dark matter. This project aims to develop ultra-sensitive detector technology essential for SABRE, a world-wide experiment with detectors in both the Northern and Southern Hemispheres which are operated together to directly detect the dark matter halo of our Milky Way galaxy. Dark matter makes up nearly five times more mass in the universe than everything we can see, yet it has never been detected in the laboratory. SABRE South will be installed in the Stawell Underground Physics Laboratory in a goldmine in Victoria, Australia. Dark matter is not the only thing SABRE can detect. The project will measure all possible types of naturally occurring radiation, from space, the surrounding rock, and the detectors themselves, that can blind SABRE to dark matter.Read moreRead less
Australia’s first direct-detection dark matter search, at Stawell Gold Mine. This project aims to develop an underground integrated laboratory at Stawell Gold Mine in Victoria to host the Southern Hemisphere's first-ever direct-detection dark matter experiment. Following the Higgs boson discovery, the direct detection of dark matter is seen as the next major challenge for particle physics. This project sees Australian physicists team up with local and international partners in research and indus ....Australia’s first direct-detection dark matter search, at Stawell Gold Mine. This project aims to develop an underground integrated laboratory at Stawell Gold Mine in Victoria to host the Southern Hemisphere's first-ever direct-detection dark matter experiment. Following the Higgs boson discovery, the direct detection of dark matter is seen as the next major challenge for particle physics. This project sees Australian physicists team up with local and international partners in research and industry to join the search for dark matter. This Australian experiment aims to help to confirm or deny current results from Northern Hemisphere experiments. As the mine nears the end of its working life as a gold mine, this project is expected to benefit the local economy and provide opportunities for education and outreach.Read moreRead less
Revealing the atoms that control performance in photoactive perovskites. This project aims to develop new electron microscopy techniques that will unambiguously determine the elusive structures of photoactive perovskite compounds under static and operational conditions, while correlating crystal structure with solar cell device performance. Photoactive perovskites are promising photovoltaic materials, however, many are sensitive to air and irradiation. This has impeded a huge international resea ....Revealing the atoms that control performance in photoactive perovskites. This project aims to develop new electron microscopy techniques that will unambiguously determine the elusive structures of photoactive perovskite compounds under static and operational conditions, while correlating crystal structure with solar cell device performance. Photoactive perovskites are promising photovoltaic materials, however, many are sensitive to air and irradiation. This has impeded a huge international research effort to determine their structure reliably at the atomic scale. With these new techniques applied to leading compounds and devices, it is expected this project will reveal the structural effects controlling electrical properties and device performance and so enable the design of superior perovskite photovoltaics.Read moreRead less
Testing fundamental physics with solar twin stars. This project aims to test the variation of fundamental physical constants across our galaxy by using twins of our Sun, a new probe that unlocks a 1000-fold sensitivity gain. The standard model of nature's laws cannot explain fundamental constants, like electromagnetism's strength, alpha. By discovering distant solar twins, the project intends to probe alpha in regions of very different Dark Matter density, opening an unexplored discovery space ....Testing fundamental physics with solar twin stars. This project aims to test the variation of fundamental physical constants across our galaxy by using twins of our Sun, a new probe that unlocks a 1000-fold sensitivity gain. The standard model of nature's laws cannot explain fundamental constants, like electromagnetism's strength, alpha. By discovering distant solar twins, the project intends to probe alpha in regions of very different Dark Matter density, opening an unexplored discovery space. Expected outcomes include the most precise astronomical measurement of a fundamental constant, and the first test of variations in alpha across our Galaxy's Dark Matter field.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
Advanced metallisation for III-V Photovoltaic Solar Power Systems. This project aims to augment the overall electrical efficiency of concentrator photovoltaic solar systems that provide large-scale generation of cheap, clean electricity. Existing concentrator solar cells are highly efficient (>40%) but their performance is hampered by thick front-metal contacts that shade the cell. The project is expected to develop a new concentrator solar cell metalisation and insulation technology. The benefi ....Advanced metallisation for III-V Photovoltaic Solar Power Systems. This project aims to augment the overall electrical efficiency of concentrator photovoltaic solar systems that provide large-scale generation of cheap, clean electricity. Existing concentrator solar cells are highly efficient (>40%) but their performance is hampered by thick front-metal contacts that shade the cell. The project is expected to develop a new concentrator solar cell metalisation and insulation technology. The benefit of the project will be a direct increase in the system efficiency and simplified manufacturing of the concentrator solar receiver, which in turn reduces the cost of the concentrator power plant constructed by our Australian project partner RayGen Resources Pty Ltd.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE200100201
Funder
Australian Research Council
Funding Amount
$530,000.00
Summary
A major upgrade to the Australia Telescope Compact Array. This project aims to upgrade the $150m CSIRO Australia Telescope Compact Array ("the telescope"), by replacing the signal processing electronics and doubling the bandwidth. This will significantly enhance the performance of the telescope, enabling more ambitious science by the 450 researchers and students who use it each year. For example, it will enable the telescope to study radio counterparts to Gravitational Wave sources, and it will ....A major upgrade to the Australia Telescope Compact Array. This project aims to upgrade the $150m CSIRO Australia Telescope Compact Array ("the telescope"), by replacing the signal processing electronics and doubling the bandwidth. This will significantly enhance the performance of the telescope, enabling more ambitious science by the 450 researchers and students who use it each year. For example, it will enable the telescope to study radio counterparts to Gravitational Wave sources, and it will enable it to make detailed observations of initial discoveries made with the Australian Square Kilometre Array Pathfinder and other Australian telescopes. In short, it will enable Australian researchers to do more ambitious research, and make more discoveries, across broad areas of astrophysics.Read moreRead less