Weighing the Universe using fast radio bursts. Fast radio bursts are a newly-discovered astronomical phenomenon whose millisecond-timescale emission occurs at cosmological distances, rendering them exceptional probes of the matter that lies in intergalactic space. This project aims to measure the positions and obtain the distances to these bursts to make a direct measurement of the density of ordinary matter in the Universe, at least 50 per cent of which is believed to remain undetected in inter ....Weighing the Universe using fast radio bursts. Fast radio bursts are a newly-discovered astronomical phenomenon whose millisecond-timescale emission occurs at cosmological distances, rendering them exceptional probes of the matter that lies in intergalactic space. This project aims to measure the positions and obtain the distances to these bursts to make a direct measurement of the density of ordinary matter in the Universe, at least 50 per cent of which is believed to remain undetected in intergalactic space. This project will measure the distribution of this missing matter, and find how it has evolved throughout the history of the Universe. This will provide significant benefits, such as addressing two fundamental questions about our Universe: how much matter does it contain, and has a large fraction of it hitherto evaded detection in intergalactic space?Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE200100008
Funder
Australian Research Council
Funding Amount
$700,000.00
Summary
Australian Seismic Imaging Array. The project aims to create a facility for developing techniques for imaging the deep earth and the surface motion in ambient seismic waves created by wind, waves and human activity. The techniques will enable sources of seismic vibrations to be identified and suppressed, and will allow mapping techniques to be developed for monitoring and discovery of resources such as ground water. Gravitational wave researchers will benefit from the ability to suppress seismic ....Australian Seismic Imaging Array. The project aims to create a facility for developing techniques for imaging the deep earth and the surface motion in ambient seismic waves created by wind, waves and human activity. The techniques will enable sources of seismic vibrations to be identified and suppressed, and will allow mapping techniques to be developed for monitoring and discovery of resources such as ground water. Gravitational wave researchers will benefit from the ability to suppress seismic vibrations, while geophysicists will benefit from new techniques and training. Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE110100129
Funder
Australian Research Council
Funding Amount
$550,000.00
Summary
Equipment and instrumentation for breaking the quantum measurement barrier. This equipment will support Australia's partnership in the international effort to detect gravitational waves, which would allow the first direct observation of black holes and mark the beginning of exploration of the gravitational wave spectrum.
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE160100144
Funder
Australian Research Council
Funding Amount
$650,000.00
Summary
Equipment for International Collaboration in Next Generation GW Detectors. Equipment for international collaboration in next-generation gravitational wave detectors:
This project aims to create a silicon optics research facility which combines Australian capabilities in silicon manufacturing at nanometre precision, with revolutionary crystalline mirror technology. The equipment is designed to enable international teams of physicists to research the optical and acoustic properties of silicon in ....Equipment for International Collaboration in Next Generation GW Detectors. Equipment for international collaboration in next-generation gravitational wave detectors:
This project aims to create a silicon optics research facility which combines Australian capabilities in silicon manufacturing at nanometre precision, with revolutionary crystalline mirror technology. The equipment is designed to enable international teams of physicists to research the optical and acoustic properties of silicon in high optical power and high precision silicon measurement systems. Research facilitated by this equipment may pave the way for the next generation of ultra-low-noise systems required for gravitational wave detection, while opening the possibility of multiple new applications in precision measurement devices. Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE110100212
Funder
Australian Research Council
Funding Amount
$160,000.00
Summary
Deep investigations of galaxies and pulsars. A new detector for the Parkes radio telescope will be made which will enable the use of new techniques for removing radio interference and, as a result, will allow researchers to detect fainter and more distant objects in the Universe than previously possible.
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE150100155
Funder
Australian Research Council
Funding Amount
$370,000.00
Summary
An Ultra-wideband Radio Receiver for the Parkes 64-metre Radio Telescope. An ultra-wideband radio receiver for the Parkes 64-metre radio telescope: This project aims to construct a state-of-the-art ultra-wide-band receiver and signal processing system for the Parkes 64-metre radio telescope. The receiver will operate across the entire 700 megahertz to four gigahertz band with outstanding sensitivity and polarimetric performance, providing a unique capability for high-time-resolution wide-bandwid ....An Ultra-wideband Radio Receiver for the Parkes 64-metre Radio Telescope. An ultra-wideband radio receiver for the Parkes 64-metre radio telescope: This project aims to construct a state-of-the-art ultra-wide-band receiver and signal processing system for the Parkes 64-metre radio telescope. The receiver will operate across the entire 700 megahertz to four gigahertz band with outstanding sensitivity and polarimetric performance, providing a unique capability for high-time-resolution wide-bandwidth astronomy. It is expected to deliver enhanced science outcomes for a wide range of projects and greatly improve the telescope's operational efficiency, extending its lifetime into the Square Kilometre Array era. Key science projects include tests of theories of relativistic gravitation, including the search for gravitational waves, probing neutron star interiors and investigations of the magnetic structure of our galaxy.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE140100121
Funder
Australian Research Council
Funding Amount
$720,000.00
Summary
Equipment for International Collaboration in Gravitational Wave Detection. Equipment for international collaboration in gravitational wave detection: This project will allow the Australian Consortium for Gravitational Astronomy to install optical equipment at its dedicated research facility, and to install data analysis pipelines on new iVEC Pawsey Centre GPU-enabled supercomputers. The equipment is required for research aimed at stabilising instabilities in the new international gravitational w ....Equipment for International Collaboration in Gravitational Wave Detection. Equipment for international collaboration in gravitational wave detection: This project will allow the Australian Consortium for Gravitational Astronomy to install optical equipment at its dedicated research facility, and to install data analysis pipelines on new iVEC Pawsey Centre GPU-enabled supercomputers. The equipment is required for research aimed at stabilising instabilities in the new international gravitational wave detectors currently being commissioned in the USA and Europe. Real time data from the new detectors will be analysed using innovative new techniques. Scientists across Australia will be able to rapidly localise potential gravitational wave sources to direct robotic telescope observations. This could enable the first detection of gravitational waves.Read moreRead less
Detection and Localisation of Gravitational Waves using Pulsar Timing Array. This project aims to contribute to one of the most significant breakthroughs in science - the direct detection of gravitational waves. It will develop innovative techniques to detect and localise gravitational waves in the nanohertz frequency band from radio timing data of millisecond pulsars. The technique developed by this project will help maximise the scientific output of Australia's legendary Parkes Radio Telescope ....Detection and Localisation of Gravitational Waves using Pulsar Timing Array. This project aims to contribute to one of the most significant breakthroughs in science - the direct detection of gravitational waves. It will develop innovative techniques to detect and localise gravitational waves in the nanohertz frequency band from radio timing data of millisecond pulsars. The technique developed by this project will help maximise the scientific output of Australia's legendary Parkes Radio Telescope, and boost the opportunities of the first detections of gravitational waves using the upcoming radio telescopes, Five hundred meter Aperture Spherical Telescope (FAST) and Square Kilometre Array (SKA).Read moreRead less