Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0454166
Funder
Australian Research Council
Funding Amount
$1,305,029.00
Summary
Nanoscale Materials Characterization Facility. We request a transmission and a scanning electron microscope, each with specialist electron probes smaller than a nanometre, which can selectively analyse the atomic structure and chemistry of sub-nanometre regions of material.
These capabilities are essential to advance a large range of research projects at the cutting-edge of materials science and engineering, undertaken by Victoria's leading research institutions: five Victorian universities, ....Nanoscale Materials Characterization Facility. We request a transmission and a scanning electron microscope, each with specialist electron probes smaller than a nanometre, which can selectively analyse the atomic structure and chemistry of sub-nanometre regions of material.
These capabilities are essential to advance a large range of research projects at the cutting-edge of materials science and engineering, undertaken by Victoria's leading research institutions: five Victorian universities, the CSIRO, Nanotechnology Victoria Ltd, the Victorian Centre for Advanced Materials Manufacturing and the CRC for Microtechnology. Together they have contributed $2.58 million to this project.
This state-of-the-art facility will include the highest spatial resolution microscope in Australia.
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Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0219038
Funder
Australian Research Council
Funding Amount
$320,000.00
Summary
Focused Ion Beam System for multidisciplinary applications. A Focused Ion Beam (FIB)system to be housed in a central facility and configured for maximum flexibility and utility over a very wide range of disciplines and applications. It will be used for micromachining and nanoscale fabrication, as an imaging device sensitive to crystal orientation and as a preparation device for scanning and transmission electron microscopy. It will support research including electronic and opto-electronic mater ....Focused Ion Beam System for multidisciplinary applications. A Focused Ion Beam (FIB)system to be housed in a central facility and configured for maximum flexibility and utility over a very wide range of disciplines and applications. It will be used for micromachining and nanoscale fabrication, as an imaging device sensitive to crystal orientation and as a preparation device for scanning and transmission electron microscopy. It will support research including electronic and opto-electronic materials, nanotechnology, complex mesoscale structures, earth sciences, small system optics, fracture behaviour of polymers and biocomposites.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0989127
Funder
Australian Research Council
Funding Amount
$400,000.00
Summary
A High-Throughput Neutron Spectrometer for The Study of Atomic and Molecular Motion at ANSTO. Neutron scattering enables new science across a broad range of disciplines, and for this reason it is undergoing major expansion in the USA, Europe, Japan and Australia. Various diffactometers and spectrometers have recently been built at ANSTO, but an instrumental option for a high-throughput cross-discipline spectroscopy is urgently needed. Fortunately, it is fairly straightforward to add this type of ....A High-Throughput Neutron Spectrometer for The Study of Atomic and Molecular Motion at ANSTO. Neutron scattering enables new science across a broad range of disciplines, and for this reason it is undergoing major expansion in the USA, Europe, Japan and Australia. Various diffactometers and spectrometers have recently been built at ANSTO, but an instrumental option for a high-throughput cross-discipline spectroscopy is urgently needed. Fortunately, it is fairly straightforward to add this type of option to an existing spectrometer that will broaden its user-base from specialised applications in physics to more general applications in physics, chemistry, materials-science and biology. This additional option provides a totally new way for Australian scientists to study atomic and molecular motions. Read moreRead less
Development of Advanced Detection Systems for Accelerator Mass Spectrometry. This project aims to expand significantly the range of isotopes available for accelerator mass spectrometry at the Australian National University to include the ability to detect manganese-53, nickel-59 and uranium-236 to ultra-sensitive concentrations. To achieve this, my extensive experience in fundamental nuclear physics will be exploited to develop a gas-filled magnet for the detection of mangnese-53 and nickel-59, ....Development of Advanced Detection Systems for Accelerator Mass Spectrometry. This project aims to expand significantly the range of isotopes available for accelerator mass spectrometry at the Australian National University to include the ability to detect manganese-53, nickel-59 and uranium-236 to ultra-sensitive concentrations. To achieve this, my extensive experience in fundamental nuclear physics will be exploited to develop a gas-filled magnet for the detection of mangnese-53 and nickel-59, and a time-of-flight detector to detect uranium-236. This project has applications in the topical areas of climate change and nuclear safeguards, as well as applications in the earth sciences and the management of nuclear waste.Read moreRead less
Discovering the First Generation of Stars in the Galaxy - The Most Metal-Poor Stars. The most metal-poor stars carry a fossil record of the early chemical and dynamical evolution of the Galaxy. The most interesting objects are those with the lowest metal abundances representing the earliest generation of stars in the Galaxy. The aim of the present project is to extend the mining of the HES objective spectra to identify extremely metal-deficient giants, which together with the already identified ....Discovering the First Generation of Stars in the Galaxy - The Most Metal-Poor Stars. The most metal-poor stars carry a fossil record of the early chemical and dynamical evolution of the Galaxy. The most interesting objects are those with the lowest metal abundances representing the earliest generation of stars in the Galaxy. The aim of the present project is to extend the mining of the HES objective spectra to identify extremely metal-deficient giants, which together with the already identified dwarfs will be further distilled using 6dF and the DBS. We anticipate trebling the total number of the most metal deficient stars known and targeting these for observations with 8m telescopes.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0989541
Funder
Australian Research Council
Funding Amount
$1,000,000.00
Summary
High Field Solid State and Multinuclear NMR Spectrometer for Structure/Function Analysis of Materials. Projects requiring the proposed infrastructure are aligned with two of the National Research Priorities. The research will lead to the development of novel materials, polymers and drugs, in particular nanoporous molecular frameworks, as well as reactive catalysts. The understanding of protein structure, disease and metabolic pathways which will be established using the proposed equipment will c ....High Field Solid State and Multinuclear NMR Spectrometer for Structure/Function Analysis of Materials. Projects requiring the proposed infrastructure are aligned with two of the National Research Priorities. The research will lead to the development of novel materials, polymers and drugs, in particular nanoporous molecular frameworks, as well as reactive catalysts. The understanding of protein structure, disease and metabolic pathways which will be established using the proposed equipment will contribute to the priority area 'Promoting and Maintaining Good Health'. In addition, the new equipment will extend capabilities and postgraduate training in chemistry, nanotechnology, and biomedicine (the priority area of 'Frontier Technologies for Building and Transforming Australian Industries').Read moreRead less
Star Formation at Millimetre Wavelengths with the CSIRO Australia Telescope. The newly-upgraded CSIRO Australia Telescope Compact Array, together with the CSIRO Mopra Telescope, provide a unique and powerful combination for studying the millimetre-wave emission from molecules and cold dust in star formation regions. We propose to combine the astrophysical expertise of UNSW with the instrumental expertise of CSIRO to use these instruments to study the processes of star formation. There are two pa ....Star Formation at Millimetre Wavelengths with the CSIRO Australia Telescope. The newly-upgraded CSIRO Australia Telescope Compact Array, together with the CSIRO Mopra Telescope, provide a unique and powerful combination for studying the millimetre-wave emission from molecules and cold dust in star formation regions. We propose to combine the astrophysical expertise of UNSW with the instrumental expertise of CSIRO to use these instruments to study the processes of star formation. There are two parallel themes to this research: to commission and develop optimal techniques for using the new instruments, and to make use of them to explore the poorly-understood processes that cause stars to form.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0347403
Funder
Australian Research Council
Funding Amount
$222,000.00
Summary
An ultra-wideband digital filterbank for the Mopra Radiotelescope. We seek funding to equip the Mopra radiotelescope with an ultra-wide-bandwidth digital filter bank. This will greatly improve the efficiency of the observatory, increasing the speed at which spectroscopic data is acquired by a factor of 8, and the speed of acquiring continuum data by a factor of 32. Once equipped in this way, Mopra, which is already the largest millimetre-wave radiotelescope in the southern hemisphere, will enjo ....An ultra-wideband digital filterbank for the Mopra Radiotelescope. We seek funding to equip the Mopra radiotelescope with an ultra-wide-bandwidth digital filter bank. This will greatly improve the efficiency of the observatory, increasing the speed at which spectroscopic data is acquired by a factor of 8, and the speed of acquiring continuum data by a factor of 32. Once equipped in this way, Mopra, which is already the largest millimetre-wave radiotelescope in the southern hemisphere, will enjoy an unbeatable edge over all other competing observatories around the world through its combination of collecting area and bandpass.Read moreRead less
Exposure dating with manganese-53, neon-21 and beryllium-10: a new toolkit for studying long-term landscape evolution. Australia today is the driest inhabited continent but this was not always the case. Tens of millions of years ago the climate of Australia was considerably wetter. Then, several million years ago, aridity in Australia developed producing most of the desert features of the red Centre that we see today. The age of our deserts and other arid features are not, however, well known. T ....Exposure dating with manganese-53, neon-21 and beryllium-10: a new toolkit for studying long-term landscape evolution. Australia today is the driest inhabited continent but this was not always the case. Tens of millions of years ago the climate of Australia was considerably wetter. Then, several million years ago, aridity in Australia developed producing most of the desert features of the red Centre that we see today. The age of our deserts and other arid features are not, however, well known. This project will determine the age of desertification in Australia, thereby enhancing our understanding of such processes and the response of our landscape to changing climate.
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Global Gravitational Wave Astronomy. To listen to the universe with gravitational waves needs a global array of gravitational wave observatories, and one of these must be in the southern hemisphere - in Australia. By definitively answering outstanding questions about an Australian gravitational wave observatory - Where should it be? How sensitive? What astronomy will it aid? - we make the case for the international community to help build this observatory, investing hundreds of millions of dolla ....Global Gravitational Wave Astronomy. To listen to the universe with gravitational waves needs a global array of gravitational wave observatories, and one of these must be in the southern hemisphere - in Australia. By definitively answering outstanding questions about an Australian gravitational wave observatory - Where should it be? How sensitive? What astronomy will it aid? - we make the case for the international community to help build this observatory, investing hundreds of millions of dollars in rural Australia and keeping Australia on the cutting edge of all branches of astronomy. As a flagship client of advanced data GRID technologies, we will also shape the growth of Australian knowledge of, and infrastructure for, next-generation communications technologies.Read moreRead less