Black holes accreting at extreme rates . The release of gravitational energy as mass is dumped onto a black hole powers some of the most extreme phenomena in the Universe. This project aims to use a new X-ray telescope to find the most disruptive stellar-mass and supermassive black holes in the Universe, and characterise their outflows with some of the world's most sensitive radio telescopes. This research will answer fundamental questions identified by the astronomical community regarding how b ....Black holes accreting at extreme rates . The release of gravitational energy as mass is dumped onto a black hole powers some of the most extreme phenomena in the Universe. This project aims to use a new X-ray telescope to find the most disruptive stellar-mass and supermassive black holes in the Universe, and characterise their outflows with some of the world's most sensitive radio telescopes. This research will answer fundamental questions identified by the astronomical community regarding how black holes grow, how they generate powerful outflows, and how much energy they can deposit into the surrounding environment. It will forge strong links with international partners, strengthen Australian expertise in this high-impact area of science, and stimulate public outreach work.Read moreRead less
Feeding the faintest black holes: the nature of low-luminosity accretion. The overwhelming majority of black holes are found in an extremely faint quiescent state. This project aims to improve understandings of this large population of black holes, determining the geometry of the inflowing gas, the source of the faint X-ray emission, and the fraction of energy pumped outwards in fast-moving jets. Building on recent ground-breaking results, this project aims to conduct a survey to detect a new po ....Feeding the faintest black holes: the nature of low-luminosity accretion. The overwhelming majority of black holes are found in an extremely faint quiescent state. This project aims to improve understandings of this large population of black holes, determining the geometry of the inflowing gas, the source of the faint X-ray emission, and the fraction of energy pumped outwards in fast-moving jets. Building on recent ground-breaking results, this project aims to conduct a survey to detect a new population of black holes in dense star clusters, providing new laboratories to explore accretion physics. It aims to measure the distances of the black holes and their motion through space, test evidence for the existence of event horizons, and provide new insights into how black holes form and how they affect their surroundings.Read moreRead less
The origin and nature of relativistic jets in X-ray binaries. This project uses Australia's world-class radio telescopes together with space-based X-ray telescopes to find out how and why black holes accelerate matter outwards in powerful, narrow beams moving close to the speed of light. The project will measure the enormous energy carried by these beams and how they collide with and deform the surrounding gas.
Developmental Origins Of Adult Cardiovascular Disease: Vascular Health In The Raine Cohort
Funder
National Health and Medical Research Council
Funding Amount
$1,087,427.00
Summary
The Raine study is a unique long term experiment that has collected extensive pre-birth and childhood data in ~3000 young Australians, who are now 27 years old. We plan to measure the artery health of 1200 of these volunteers and to determine what factors, both before and after birth, influence the presence of early atherosclerosis in humans. This study will guide strategies aimed at early prevention of heart attacks and stroke in humans, by defining the major risk factors.
Cosmic powerhouses: The birth, death, and legacy of black hole jets. This project targets relativistic jets powered by supermassive black holes - the most powerful systems in the Universe. Theoretically, the enormous energies released have a profound influence on how galaxies evolve; empirically, observations reveal signatures of their impact across cosmic time. However, fundamental questions remain about how these jets are triggered and what impact they have on galaxies. The project will addres ....Cosmic powerhouses: The birth, death, and legacy of black hole jets. This project targets relativistic jets powered by supermassive black holes - the most powerful systems in the Universe. Theoretically, the enormous energies released have a profound influence on how galaxies evolve; empirically, observations reveal signatures of their impact across cosmic time. However, fundamental questions remain about how these jets are triggered and what impact they have on galaxies. The project will address these questions using novel supercomputer models of black hole jets in realistic cosmological environments, then confront these predictions with new data from Square Kilometre Array (SKA) pathfinding radio telescopes. This will substantially enhance Australia’s leadership capacity in a strategically important area.Read moreRead less
Solving the mystery of ultra luminous fast radio burst emission . Fast Radio Bursts are a recently discovered inexplicable astronomical phenomenon whose millisecond-timescale emission is generated by regions less than 300 kilometres across yet so luminous it is visible at cosmological distances. Using the Australian Square Kilometre Array Pathfinder we have already localised these bursts, which made the front cover of Science, and recently used them to find the missing baryonic matter in the Uni ....Solving the mystery of ultra luminous fast radio burst emission . Fast Radio Bursts are a recently discovered inexplicable astronomical phenomenon whose millisecond-timescale emission is generated by regions less than 300 kilometres across yet so luminous it is visible at cosmological distances. Using the Australian Square Kilometre Array Pathfinder we have already localised these bursts, which made the front cover of Science, and recently used them to find the missing baryonic matter in the Universe. Next, we will scrutinise these bursts at three nanosecond time resolution, reaching the timescale necessary to probe the mechanism by which their ultra-luminous radiation is generated. This project will reveal previously inaccessible properties of the radiation to unlock the secrets of how they are produced.Read moreRead less
Discovery Early Career Researcher Award - Grant ID: DE170100891
Funder
Australian Research Council
Funding Amount
$338,324.00
Summary
Probing cosmic transients through gravitational wave observations. This project aims to use recently discovered gravitational waves to discover what drives cataclysmic astrophysical events, how often they occur and their history. The first detection of gravitational waves has changed astronomy. This project will apply analysis and data mining to gravitational wave and gamma-ray burst data. The results are expected to reveal the connection between gamma ray bursts, gravitational wave sources and ....Probing cosmic transients through gravitational wave observations. This project aims to use recently discovered gravitational waves to discover what drives cataclysmic astrophysical events, how often they occur and their history. The first detection of gravitational waves has changed astronomy. This project will apply analysis and data mining to gravitational wave and gamma-ray burst data. The results are expected to reveal the connection between gamma ray bursts, gravitational wave sources and fast radio bursts, substantially advancing understanding of the Universe.Read moreRead less
Detecting cosmic rays using precision radio imaging. This project's aim is to identify the source of the highest-energy particles in nature, cosmic rays, and discover new physical processes at energies unreachable by the Large Hadron Collider.
It will do this by using the Murchison Widefield Array radio telescope to detect the sub-microsecond pulses from cosmic ray interactions in the Earth's atmosphere. The project's intended outcome is a sample of thousands of cosmic ray events, and a new tec ....Detecting cosmic rays using precision radio imaging. This project's aim is to identify the source of the highest-energy particles in nature, cosmic rays, and discover new physical processes at energies unreachable by the Large Hadron Collider.
It will do this by using the Murchison Widefield Array radio telescope to detect the sub-microsecond pulses from cosmic ray interactions in the Earth's atmosphere. The project's intended outcome is a sample of thousands of cosmic ray events, and a new technique to analyse the structure within them.
The anticipated benefits are the establishment of the Murchison Widefield Array as a world-leading instrument for astroparticle physics, new knowledge of high-energy astro and particle physics, and advances and training in fast signal processing methods.Read moreRead less
The Carina Nebula: a massive star factory and the anchor for calibrating extragalactic star formation. Massive stars are vital to the life cycle of a galaxy, providing material and controlling the environment where new stars are made. This project will use the Australia Telescope to map the spectacular Carina Nebula, a hotbed of massive stars, to provide a picture of its stars and gas and a template for understanding star formation in distant galaxies.
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE240100044
Funder
Australian Research Council
Funding Amount
$860,000.00
Summary
Cryogenic Experimental Laboratory for Low-background Australian Research. This project aims to build an open-access cryogenic facility in the only deep-underground physics laboratory in the southern hemisphere. This facility, called the Cryogenic Experimental Laboratory for Low-background Australian Research (CELLAR), will provide extreme shielding from sources of noise, enabling ultra-precise experiments for fundamental science and emerging applications. The expected outcomes include a deeper u ....Cryogenic Experimental Laboratory for Low-background Australian Research. This project aims to build an open-access cryogenic facility in the only deep-underground physics laboratory in the southern hemisphere. This facility, called the Cryogenic Experimental Laboratory for Low-background Australian Research (CELLAR), will provide extreme shielding from sources of noise, enabling ultra-precise experiments for fundamental science and emerging applications. The expected outcomes include a deeper understanding of astrophysics, alongside technological advances in emerging quantum technologies. CELLAR’s unique capabilities will attract strong international collaborations with multidisciplinary teams, educating the next generation of scientists and advancing the growth of Australian high-technology industries.Read moreRead less