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  • Funded Activity

    Discovery Projects - Grant ID: DP170103625

    Funder
    Australian Research Council
    Funding Amount
    $360,000.00
    Summary
    Smart searches for continuous gravitational waves with advanced LIGO. This project aims to detect continuous gravitational waves from neutron stars, by using smart signal processing methods developed for engineering applications like mobile telephony. The first direct detection of Einstein's gravitational waves from two merging black holes by the Laser Interferometer Gravitational Wave Observatory in 2015 began a new era of human discovery. This project is expected to progress gravitational wave .... Smart searches for continuous gravitational waves with advanced LIGO. This project aims to detect continuous gravitational waves from neutron stars, by using smart signal processing methods developed for engineering applications like mobile telephony. The first direct detection of Einstein's gravitational waves from two merging black holes by the Laser Interferometer Gravitational Wave Observatory in 2015 began a new era of human discovery. This project is expected to progress gravitational wave science and Australia's role in it, and generate insights about the origin of neutron stars and the physics of bulk nuclear matter under extremes of gravity, density and magnetisation which cannot be replicated on Earth.
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    Funded Activity

    Linkage Infrastructure, Equipment And Facilities - Grant ID: LE130100032

    Funder
    Australian Research Council
    Funding Amount
    $990,000.00
    Summary
    Australian partnership in advanced Laser Interferometer Gravitational-Wave Observatory (LIGO) - continuation. Advanced Laser Interferometer Gravitational-Wave Obervatory (LIGO) will be the first gravitational wave observatory capable of frequent observation of known sources of gravitational waves leading to the birth of gravitational wave astronomy. By playing a key role in this facility, Australia will reap the scientific rewards of being part of the most exciting frontier of physics in the 2 .... Australian partnership in advanced Laser Interferometer Gravitational-Wave Observatory (LIGO) - continuation. Advanced Laser Interferometer Gravitational-Wave Obervatory (LIGO) will be the first gravitational wave observatory capable of frequent observation of known sources of gravitational waves leading to the birth of gravitational wave astronomy. By playing a key role in this facility, Australia will reap the scientific rewards of being part of the most exciting frontier of physics in the 21st century.
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    Funded Activity

    Discovery Projects - Grant ID: DP140100986

    Funder
    Australian Research Council
    Funding Amount
    $575,000.00
    Summary
    Quantum enhancement of long baseline gravitational wave detectors. This project will design and construct a quantum optical system which when used in future long baseline gravitational wave detectors will enhance sensitivity across their detection frequency band, from 10 Hz to 10 kHz. This project will use this system on small scale optical sensors to prove the concept. In so doing, it will use squeezing to reduce quantum radiation pressure noise for the first time. This system will then be read .... Quantum enhancement of long baseline gravitational wave detectors. This project will design and construct a quantum optical system which when used in future long baseline gravitational wave detectors will enhance sensitivity across their detection frequency band, from 10 Hz to 10 kHz. This project will use this system on small scale optical sensors to prove the concept. In so doing, it will use squeezing to reduce quantum radiation pressure noise for the first time. This system will then be ready for deployment on an early upgrade of Advanced LIGO increasing the science output of this detector, turning gravitational wave detection into gravitational wave astronomy.
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    Funded Activity

    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.
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    Funded Activity

    Discovery Projects - Grant ID: DP160100760

    Funder
    Australian Research Council
    Funding Amount
    $755,400.00
    Summary
    Instrumentation for the era of gravitational wave science. This project aims to study noise sources that limit the low-frequency performance of gravitational wave antenna: thermal noise, quantum radiation pressure noise and Newtonian noise. Gravitational wave detection is a new way in which to observe our universe. Although detectors such as advanced LIGO (Laser Interferometer Gravitational-Wave Observatory) should detect gravitational waves, further sensitivity improvement, particularly at low .... Instrumentation for the era of gravitational wave science. This project aims to study noise sources that limit the low-frequency performance of gravitational wave antenna: thermal noise, quantum radiation pressure noise and Newtonian noise. Gravitational wave detection is a new way in which to observe our universe. Although detectors such as advanced LIGO (Laser Interferometer Gravitational-Wave Observatory) should detect gravitational waves, further sensitivity improvement, particularly at low frequencies, will be needed to provide event rates necessary for astronomy. Expected project outcomes will support the development of the first free mass interferometer to operate at 120K using silicon optics, a vital facility for the world community. Pushing the boundaries of measurement may also drive innovation in optical sensing with potential applications in defence, security and exploration.
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    Funded Activity

    Discovery Projects - Grant ID: DP150102988

    Funder
    Australian Research Council
    Funding Amount
    $384,700.00
    Summary
    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).
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    Active Funded Activity

    Linkage Infrastructure, Equipment And Facilities - Grant ID: LE210100002

    Funder
    Australian Research Council
    Funding Amount
    $3,000,000.00
    Summary
    Australian Partnership in Advanced LIGO+: continuation. The aim of this project is, in collaboration with the USA and UK, to complete the installation and commissioning of the Advanced LIGO+ facilities in the USA in order to bring them to design sensitivity. These facilities expect to increase the event rate of gravitational wave signals by a factor of 125. This should lead to daily detections and the observation of new sources of gravitational waves. Given that only 5% of the universe is detect .... Australian Partnership in Advanced LIGO+: continuation. The aim of this project is, in collaboration with the USA and UK, to complete the installation and commissioning of the Advanced LIGO+ facilities in the USA in order to bring them to design sensitivity. These facilities expect to increase the event rate of gravitational wave signals by a factor of 125. This should lead to daily detections and the observation of new sources of gravitational waves. Given that only 5% of the universe is detectable by telescopes, the impact of gravitational wave detections on our understanding of the universe is inestimable. Australian partnership intends to enable our physicists and astronomers to be at the vanguard of this brand new field and inspire a new generation to study the physical sciences.
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    Active Funded Activity

    Discovery Early Career Researcher Award - Grant ID: DE210100550

    Funder
    Australian Research Council
    Funding Amount
    $458,127.00
    Summary
    Superior performance optical coatings for next-generation interferometry. This project aims to investigate fundamental noise in optical coatings, a limiting factor for state-of-the-art astronomical observatories, global timing standards, and photonics applications. Gravitational wave detectors, marvels of precision engineering that have produced ground-breaking discoveries in fundamental science, are particularly afflicted by coating noise. The proposed experiment plans to operate at cryogenic t .... Superior performance optical coatings for next-generation interferometry. This project aims to investigate fundamental noise in optical coatings, a limiting factor for state-of-the-art astronomical observatories, global timing standards, and photonics applications. Gravitational wave detectors, marvels of precision engineering that have produced ground-breaking discoveries in fundamental science, are particularly afflicted by coating noise. The proposed experiment plans to operate at cryogenic temperatures with unprecedented sensitivity to conduct feasibility studies of deposition methods, coating materials, and layer structures. The goal is to deploy innovative methods to develop Australian-made optical coatings with superior performance and merit for the most demanding scientific and industrial applications.
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    Funded Activity

    Discovery Projects - Grant ID: DP160103456

    Funder
    Australian Research Council
    Funding Amount
    $735,700.00
    Summary
    Capturing gravitational wave and electromagnetic flashes from binary merger. This project aims to contribute to one of the most momentous and long-anticipated discoveries in physics: the first detection of gravitational waves. The project plans to develop innovative technologies to detect gravitational waves using laser interferometers and enable prompt follow-up observations of gravitational wave sources by conventional telescopes. The outcome of this research would greatly help probe the natur .... Capturing gravitational wave and electromagnetic flashes from binary merger. This project aims to contribute to one of the most momentous and long-anticipated discoveries in physics: the first detection of gravitational waves. The project plans to develop innovative technologies to detect gravitational waves using laser interferometers and enable prompt follow-up observations of gravitational wave sources by conventional telescopes. The outcome of this research would greatly help probe the nature of matter and gravity at extreme densities.
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    Funded Activity

    Linkage Infrastructure, Equipment And Facilities - Grant ID: LE170100217

    Funder
    Australian Research Council
    Funding Amount
    $850,000.00
    Summary
    Australian Partnership in Advanced LIGO+. This project aims to improve the sensitivity of the Advanced Laser Interferometer Gravitational wave Observatory (aLIGO). aLIGO’s detection of gravitational waves proved general relativity in the strong field limit and the existence of black hole binary systems. The increased sensitivity will enable daily detections and new classes of events, opening the field of gravitational wave astronomy. Since telescopes can detect only 5% of the stuff in the univer .... Australian Partnership in Advanced LIGO+. This project aims to improve the sensitivity of the Advanced Laser Interferometer Gravitational wave Observatory (aLIGO). aLIGO’s detection of gravitational waves proved general relativity in the strong field limit and the existence of black hole binary systems. The increased sensitivity will enable daily detections and new classes of events, opening the field of gravitational wave astronomy. Since telescopes can detect only 5% of the stuff in the universe, this is expected to greatly improve understanding of the universe. This Australian partnership will put its physicists and astronomers at the vanguard of this field and inspire the next generation to study the physical sciences.
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