Nanotribology and Nanorheometry: A Fundamental Study of the Dynamic Interactions of Particles and Surfaces at the Molecular Level. Friction and deformation occur from the mutual motion and interaction of microscopic particles and surfaces. This research aims to develop new theories and measurement techniques for these non-equilibrium phenomena by combining mathematical analysis and numerical computations with dynamic force measurement, surface modification, and surface characterisation on nanom ....Nanotribology and Nanorheometry: A Fundamental Study of the Dynamic Interactions of Particles and Surfaces at the Molecular Level. Friction and deformation occur from the mutual motion and interaction of microscopic particles and surfaces. This research aims to develop new theories and measurement techniques for these non-equilibrium phenomena by combining mathematical analysis and numerical computations with dynamic force measurement, surface modification, and surface characterisation on nanometre and molecular length scales. These insights and data will be critically important in designing low-friction surfaces that save energy and wear, in developing nanoscopic probes for the mechanical and structural properties of soft polymeric and bio-materials, and in making high performance coatings that control adhesion and particle aggregation in technologically advanced applications.Read moreRead less
Pulsed oscillating mass analyser. Mass spectrometers are ubiquitous components in chemical analysis, but are often large and expensive. We have developed a new method for mass analysis, which is smaller and cheaper than existing technology. However, the analyser needs further research to determine whether it has the performance specifications to match the other technologies. The objective of this research is to characterise, explore and extend the prototype and to develop the appropriate math ....Pulsed oscillating mass analyser. Mass spectrometers are ubiquitous components in chemical analysis, but are often large and expensive. We have developed a new method for mass analysis, which is smaller and cheaper than existing technology. However, the analyser needs further research to determine whether it has the performance specifications to match the other technologies. The objective of this research is to characterise, explore and extend the prototype and to develop the appropriate mathematical algorithm for mass analysis. Success in this project may lead to a new mass analyser that can be incorporated into analytical instruments, many of which are manufactured in Australia.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0561136
Funder
Australian Research Council
Funding Amount
$376,352.00
Summary
36-megapixel CCD camera for wide-field astronomy. This project aims to design and build a state-of-the-art 36-megapixel charge-coupled device (CCD) camera for wide-field imaging on a robotic telescope at Siding Spring Observatory. The camera will employ a mosaic of two 18-megapixel CCDs, which are amongst the largest ever fabricated. This new facility will have an unprecedented ability to obtain precision photometry over a wide field, and will enable breakthroughs in research into areas as diver ....36-megapixel CCD camera for wide-field astronomy. This project aims to design and build a state-of-the-art 36-megapixel charge-coupled device (CCD) camera for wide-field imaging on a robotic telescope at Siding Spring Observatory. The camera will employ a mosaic of two 18-megapixel CCDs, which are amongst the largest ever fabricated. This new facility will have an unprecedented ability to obtain precision photometry over a wide field, and will enable breakthroughs in research into areas as diverse as detection of extra-solar planets and nearby supernovae. The camera will also lead to collaborative research with ANU's newly-funded Skymapper telescope, as well as the Anglo-Australian Observatory's 6dF and 2dF instruments.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0775637
Funder
Australian Research Council
Funding Amount
$450,000.00
Summary
An Australian Attosecond Science Facility. The laser facility requested here will provide Australian researchers with the ability to take snapshots of physical and biological processes at unprecedented time resolution. Such a facility will enable Australian researchers to remain competitive and continue to contribute significantly to scientific research on an international scale. The facility will provide excellent training for research higher degree students, preparing them for work in high-tec ....An Australian Attosecond Science Facility. The laser facility requested here will provide Australian researchers with the ability to take snapshots of physical and biological processes at unprecedented time resolution. Such a facility will enable Australian researchers to remain competitive and continue to contribute significantly to scientific research on an international scale. The facility will provide excellent training for research higher degree students, preparing them for work in high-tech industries based on cutting-edge discoveries in physics and biology.Read moreRead less
Direct deep-ultraviolet tunable laser sources generating continuous and ultra-short-pulse radiation for photonics applications. This project will develop two versatile and efficient sources of tunable deep-ultraviolet laser radiation. These sources are an enabling photonics technology that will have impact in the applied fields of precision spectroscopy and flow cytometry for detection of biological agents. The proposed ultrafast laser source will enable new fundamental research probing high-ene ....Direct deep-ultraviolet tunable laser sources generating continuous and ultra-short-pulse radiation for photonics applications. This project will develop two versatile and efficient sources of tunable deep-ultraviolet laser radiation. These sources are an enabling photonics technology that will have impact in the applied fields of precision spectroscopy and flow cytometry for detection of biological agents. The proposed ultrafast laser source will enable new fundamental research probing high-energy processes, such as ultrafast chemical reactions, on the femtosecond timescale.
Training through an APD fellowship in the national priority area of Frontier technologies: photonics will enhance Australia's expertise in this important area. Read moreRead less
Gamma-ray burst astronomy in the Swift era and beyond. The study of gamma-ray bursts is one of the most active and exciting fields in astrophysics, and touches on subjects that are of interest to all humans: e.g., to what extent was life on Earth shaped by cataclysmic explosions in our Galaxy? Australia's ROTSE-III telescope is the only facility in the southern hemisphere capable of rapidly (within 10 seconds) finding optical light from gamma-ray bursts. It will provide Australian astronomers ....Gamma-ray burst astronomy in the Swift era and beyond. The study of gamma-ray bursts is one of the most active and exciting fields in astrophysics, and touches on subjects that are of interest to all humans: e.g., to what extent was life on Earth shaped by cataclysmic explosions in our Galaxy? Australia's ROTSE-III telescope is the only facility in the southern hemisphere capable of rapidly (within 10 seconds) finding optical light from gamma-ray bursts. It will provide Australian astronomers with a competitive advantage in this high-profile field. The project will involve and inspire some of our best physics and engineering students.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0882778
Funder
Australian Research Council
Funding Amount
$201,224.00
Summary
Water vapour radiometers for millimetre-wave phase correction for the Australia Telescope. Australia has a tradition of excellence in astronomy. Inspired by wonder about the cosmos, it stimulates public interest in science, so leading to the training of highly skilled graduates. In turn, this drives the development of technologies needed to pursue the science. The nation has invested in the technology for millimetre-wave astronomy, building the first interferometer in our hemisphere. This equipm ....Water vapour radiometers for millimetre-wave phase correction for the Australia Telescope. Australia has a tradition of excellence in astronomy. Inspired by wonder about the cosmos, it stimulates public interest in science, so leading to the training of highly skilled graduates. In turn, this drives the development of technologies needed to pursue the science. The nation has invested in the technology for millimetre-wave astronomy, building the first interferometer in our hemisphere. This equipment will capitalise on this investment, extending the capabilities of the Australia Telescope to maintain it as a front line instrument, attracting the best scientists here to use it. This will help nurture a vigorous radio-science community, one able to actively participate in the billion-dollar investment being made internationally in the field.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
New Pulsar Instrumentation for Gravitation Wave Detection and Understanding the Emission Mechanism. Millisecond pulsar timing currently provides the most sensitive method of detecting long-period gravitational waves which permeate the Universe. Parkes leads the world in the discovery and timing of millisecond pulsars. This has motivated the development of three new advanced instruments including a cyrogenic dual-band receiver, a very wide-band correlator and a baseband recorder with an in-built ....New Pulsar Instrumentation for Gravitation Wave Detection and Understanding the Emission Mechanism. Millisecond pulsar timing currently provides the most sensitive method of detecting long-period gravitational waves which permeate the Universe. Parkes leads the world in the discovery and timing of millisecond pulsars. This has motivated the development of three new advanced instruments including a cyrogenic dual-band receiver, a very wide-band correlator and a baseband recorder with an in-built supercomputer. We aim to exploit these new technologies to systematically study the pulsar population. We will establish a timing array which can detect gravitational waves, enable GLAST to identify over 100 gamma-ray pulsars and study the pulsar emission mechanism at sub-microsecond time resolution.
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Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0228799
Funder
Australian Research Council
Funding Amount
$1,602,000.00
Summary
Australian Membership of the International Gemini Partnership. The International Gemini Partnership is an intergovernmental consortium formed to construct and operate two 8-metre optical/infrared telescopes, one in Chile, and the other in Hawaii. Australia joined the IGP in May 1998, taking approximately 5% of the partnership. The Gemini telescopes have been carefully engineered to exploit the superb atmospheric conditions at both sites, allowing users to address key astronomical problems in way ....Australian Membership of the International Gemini Partnership. The International Gemini Partnership is an intergovernmental consortium formed to construct and operate two 8-metre optical/infrared telescopes, one in Chile, and the other in Hawaii. Australia joined the IGP in May 1998, taking approximately 5% of the partnership. The Gemini telescopes have been carefully engineered to exploit the superb atmospheric conditions at both sites, allowing users to address key astronomical problems in ways not previously possible. Through membership of Gemini, Australian astronomers have access to the world-class facilities necessary to maintain their high international profile and great public visibility in Galactic and extragalactic astronomy, and also to enhance the national capacity to construct advanced scientific instrumentation. Australia has already won a contract to build one of the instruments.Read moreRead less