Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0238884
Funder
Australian Research Council
Funding Amount
$220,000.00
Summary
Development of the CANGAROO III Very High Energy Gamma-ray telescope. This international project will explore the only part of the electromagnetic spectrum yet to be subjected to detailed astronomical study. CANGAROO III will span the energy range from ~100GeV to >10TeV, expanding upwards the range of satellite observations, and downwards the range accessible from previous ground-based systems. Gamma-ray observations have opened a new window on the universe and it is clear that there is much to ....Development of the CANGAROO III Very High Energy Gamma-ray telescope. This international project will explore the only part of the electromagnetic spectrum yet to be subjected to detailed astronomical study. CANGAROO III will span the energy range from ~100GeV to >10TeV, expanding upwards the range of satellite observations, and downwards the range accessible from previous ground-based systems. Gamma-ray observations have opened a new window on the universe and it is clear that there is much to be discovered with this new instrument. This project will provide an Australian infrastructure contribution to support the multi-million dollar contribution of our Japanese partners, and thus provide Australian access to a key astrophysical field at very modest cost.Read moreRead less
The Dawn of Extreme Gamma Ray Astronomy. This project aims to reveal the highest energy cosmic-ray particles in our galaxy, produced in extreme and still unknown astrophysical processes. Their interaction with nuclei in space produces the highest energy gamma ray light. Our project will make use of this extreme gamma ray light with upgraded and next-generation gamma-ray telescope arrays. With accompanying data from Australian radio telescopes, and computer models of the cosmic ray interactions, ....The Dawn of Extreme Gamma Ray Astronomy. This project aims to reveal the highest energy cosmic-ray particles in our galaxy, produced in extreme and still unknown astrophysical processes. Their interaction with nuclei in space produces the highest energy gamma ray light. Our project will make use of this extreme gamma ray light with upgraded and next-generation gamma-ray telescope arrays. With accompanying data from Australian radio telescopes, and computer models of the cosmic ray interactions, our project can finally determine from where these cosmic rays originate, yielding insight into our galaxy's evolution. Complex machine learning methods will be needed in a project that provides a world-leading student training ground, motivated by a century old mystery in astronomy.Read moreRead less
ARC Complex Open Systems Research Network. Complexity is the common frontier in the physical, biological and social sciences. This Network will link specialists in all three sciences through five generic conceptual and mathematical theme activities. It will promote research into how subsystems self-organise into new emergent structures when assembled into an open, non-equilibrium system. Outcomes will include new technologies and software tools and deeper understanding of fundamental questions i ....ARC Complex Open Systems Research Network. Complexity is the common frontier in the physical, biological and social sciences. This Network will link specialists in all three sciences through five generic conceptual and mathematical theme activities. It will promote research into how subsystems self-organise into new emergent structures when assembled into an open, non-equilibrium system. Outcomes will include new technologies and software tools and deeper understanding of fundamental questions in science. An essential function of the network will be introducing researchers end users to new tools and broadening the horizons of graduate students.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE120100158
Funder
Australian Research Council
Funding Amount
$750,000.00
Summary
The Nanten2 sub-millimetre telescope. The millimetre-wavelength sky holds the key for understanding how stars form in the coldest regions of interstellar space: the molecular clouds of our Galaxy. A new frontline facility in Chile will be used in an international research endeavour to map their structures, in order to find out how they form and what causes stars to be born inside them.
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
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE110100038
Funder
Australian Research Council
Funding Amount
$150,000.00
Summary
The NANTEN2 Observatory sub-millimetre wave telescope. The millimetre-wavelength sky holds the key to understanding how stars form in the coldest regions of interstellar space: the molecular clouds of our Galaxy. This new frontline facility in Chile will be used in an international research endeavour to map these cold regions and the stars they contain in order to find out how they form and what causes stars to be born within them.
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE150100076
Funder
Australian Research Council
Funding Amount
$150,068.00
Summary
Australian Participation in the Belle II Experiment. Australian participation in the Belle II experiment: This project will provide membership for Australian scientists of one of the key contemporary particle physics experiments, the Belle II experiment in Japan, and contribute to the purchase and installation of equipment for the Japanese facility. The Belle II experiment aims to search for a deeper theory of nature which will add significantly to our ability to answer questions such as why the ....Australian Participation in the Belle II Experiment. Australian participation in the Belle II experiment: This project will provide membership for Australian scientists of one of the key contemporary particle physics experiments, the Belle II experiment in Japan, and contribute to the purchase and installation of equipment for the Japanese facility. The Belle II experiment aims to search for a deeper theory of nature which will add significantly to our ability to answer questions such as why there is a preponderance of matter over antimatter in the Universe, and what is the nature of the dark matter which pervades it. This project will allow Australian scientists to pursue these questions in the coming years, with the additional benefit of increasing Australia's research profile in fundamental physics and its engagement with basic science in the Asia-Pacific region.Read moreRead less