Extreme astrophysics in the age of gravitational waves. This project aims to probe the most catastrophic explosions in the universe. It will use gravitational wave astronomy to detect an exotic effect that causes space to permanently deform following cataclysmic events, determine the origin of binary black holes by measuring statistical properties of many mergers, and use observations of colliding neutron stars to understand the physics of the biggest explosions in the Universe. This project wil ....Extreme astrophysics in the age of gravitational waves. This project aims to probe the most catastrophic explosions in the universe. It will use gravitational wave astronomy to detect an exotic effect that causes space to permanently deform following cataclysmic events, determine the origin of binary black holes by measuring statistical properties of many mergers, and use observations of colliding neutron stars to understand the physics of the biggest explosions in the Universe. This project will lay the framework for the next decade of the new field of gravitational-wave astronomy.Read moreRead less
Discovery Early Career Researcher Award - Grant ID: DE180100346
Funder
Australian Research Council
Funding Amount
$328,075.00
Summary
Probing extreme astrophysics via rapid response to cosmic explosions. This project aims to reveal the radio emission properties of particular classes of gravitational wave events through the utilisation and further development of rapid-response observing systems on Australian radio telescopes. The project will use Australian radio telescopes to rapidly and automatically obtain observations of short-duration gamma-ray bursts, which are thought to be a subclass of gravitational wave events. It is ....Probing extreme astrophysics via rapid response to cosmic explosions. This project aims to reveal the radio emission properties of particular classes of gravitational wave events through the utilisation and further development of rapid-response observing systems on Australian radio telescopes. The project will use Australian radio telescopes to rapidly and automatically obtain observations of short-duration gamma-ray bursts, which are thought to be a subclass of gravitational wave events. It is anticipated such observations will provide vital insight into the early-time radio signatures of gravitational wave events and that rapid-response experiments will contribute invaluable knowledge towards optimising transient science conducted with the Square Kilometre Array.Read moreRead less
SkyMapper and the Southern Sky Survey. The Southern Sky Survey is the first digital imaging survey of the entire southern hemisphere sky. The resulting information on a billion stellar and galaxy images underpins a number of significant national science programs of international prominence. These include the discovery of the oldest stars in our galaxy, fossils from its formation.
“Beacons in the Night” unveiling how galaxies light up dark matter. How dark matter influences the formation and evolution of galaxies is to this day an outstanding question in astrophysics. To answer it, world-class facilities and a unique combination of observations and theory are required. This DP team, a world-class team of observers and theorists, will tackle this question by leveraging on two multi-million dollar projects: the MAGPI galaxy survey and the hydrodynamical simulations suite EA ....“Beacons in the Night” unveiling how galaxies light up dark matter. How dark matter influences the formation and evolution of galaxies is to this day an outstanding question in astrophysics. To answer it, world-class facilities and a unique combination of observations and theory are required. This DP team, a world-class team of observers and theorists, will tackle this question by leveraging on two multi-million dollar projects: the MAGPI galaxy survey and the hydrodynamical simulations suite EAGLE-XL. MAGPI will deliver exquisite kinematics for hundreds of galaxies in the middle ages of the Universe, providing a view to the effect of dark matter on galaxies at this critical time, while EAGLE-XL represents the technological frontier in simulations and provides the best interpretative framework for MAGPI.Read moreRead less
Putting Einstein to the test: Probing gravity with gravitational waves. This project aims to capitalise on the momentous discovery of gravitational waves by the Laser Interferometer Gravitational-wave Observatory (LIGO). In 2016, the LIGO Scientific Collaboration announced the first detection of gravitational waves coming from the collision of two massive black holes approximately one billion light years from Earth. The project aims to use proprietary LIGO data, of multiple gravitational-wave ob ....Putting Einstein to the test: Probing gravity with gravitational waves. This project aims to capitalise on the momentous discovery of gravitational waves by the Laser Interferometer Gravitational-wave Observatory (LIGO). In 2016, the LIGO Scientific Collaboration announced the first detection of gravitational waves coming from the collision of two massive black holes approximately one billion light years from Earth. The project aims to use proprietary LIGO data, of multiple gravitational-wave observations, to perform unprecedented tests of Einstein's theory of gravity in regions of the Universe where new physics is most likely to occur - at the surfaces of black holes. The project is designed to develop the foundation of gravitational-wave astronomy for the next three-to-five years.Read moreRead less
The key role of black holes in galaxy evolution. This project will determine the effect of black holes on galaxy formation using sophisticated supercomputer simulations of radiation, jets and winds interacting with multi-phase interstellar gas in the host galaxy. The results of these simulations will be calibrated against radio and optical observations and incorporated into larger scale simulations describing the growth of structure in the Universe and the evolution of galaxies. This research is ....The key role of black holes in galaxy evolution. This project will determine the effect of black holes on galaxy formation using sophisticated supercomputer simulations of radiation, jets and winds interacting with multi-phase interstellar gas in the host galaxy. The results of these simulations will be calibrated against radio and optical observations and incorporated into larger scale simulations describing the growth of structure in the Universe and the evolution of galaxies. This research is highly relevant to the future science programs of the Giant Magellan Telescope and the Square Kilometre Array.Read moreRead less
A Major Upgrade of the Pierre Auger Cosmic Ray Observatory. A major upgrade is under-way to enhance the sensitivity of the 3000 square kilometre Pierre Auger Observatory in its search for the origin of the highest energy cosmic rays, the most energetic particles known in the Universe. This follows an unexpected Auger result that indicates a significant fraction of these cosmic rays are heavy nuclei. This project, assisting the upgrade, is expected to significantly improve the observatory's abil ....A Major Upgrade of the Pierre Auger Cosmic Ray Observatory. A major upgrade is under-way to enhance the sensitivity of the 3000 square kilometre Pierre Auger Observatory in its search for the origin of the highest energy cosmic rays, the most energetic particles known in the Universe. This follows an unexpected Auger result that indicates a significant fraction of these cosmic rays are heavy nuclei. This project, assisting the upgrade, is expected to significantly improve the observatory's ability to identify the mass, and hence the electric charge, of the incoming cosmic rays, allowing astrophysical source directions to be identified for the low charge particles less affected by cosmic magnetic fields. The project will also contribute to the understanding of particle interactions at energies well beyond those explored at the Large Hadron Collider.Read moreRead less
Exploring the high energy sky with the Pierre Auger Observatory. Cosmic rays are enormously energetic particles that must originate in the most violent environments in the Universe. This work will use the 3000 sq km Pierre Auger Observatory, built in collaboration with Australian physicists, to pinpoint the origin of these rare particles, thus laying to rest one of the longest standing mysteries in astronomy.
The Dawn of Extreme Gamma Ray Astronomy. This project aims to reveal the highest energy cosmic-ray particles in our galaxy, produced in extreme and still unknown astrophysical processes. Their interaction with nuclei in space produces the highest energy gamma ray light. Our project will make use of this extreme gamma ray light with upgraded and next-generation gamma-ray telescope arrays. With accompanying data from Australian radio telescopes, and computer models of the cosmic ray interactions, ....The Dawn of Extreme Gamma Ray Astronomy. This project aims to reveal the highest energy cosmic-ray particles in our galaxy, produced in extreme and still unknown astrophysical processes. Their interaction with nuclei in space produces the highest energy gamma ray light. Our project will make use of this extreme gamma ray light with upgraded and next-generation gamma-ray telescope arrays. With accompanying data from Australian radio telescopes, and computer models of the cosmic ray interactions, our project can finally determine from where these cosmic rays originate, yielding insight into our galaxy's evolution. Complex machine learning methods will be needed in a project that provides a world-leading student training ground, motivated by a century old mystery in astronomy.Read moreRead less
Exploring the High Energy Universe with Neutrinos detected in IceCube. The project aims to use the high energy neutrinos observed by the IceCube detector at the South Pole to uncover
the nature of the most energetic objects in the Universe. This project expects to find out what distant objects made
the neutrinos, understand their distribution through the Universe, and see if they are also cosmic and gamma ray
acceleration and production sites. Expected outcomes of this project include solving th ....Exploring the High Energy Universe with Neutrinos detected in IceCube. The project aims to use the high energy neutrinos observed by the IceCube detector at the South Pole to uncover
the nature of the most energetic objects in the Universe. This project expects to find out what distant objects made
the neutrinos, understand their distribution through the Universe, and see if they are also cosmic and gamma ray
acceleration and production sites. Expected outcomes of this project include solving this long-standing mystery in
high-energy astrophysics, development of new data analysis techniques, training new scientists, and educating
the public. These should provide significant benefits to science and society, through a better educated and critical
thinking workforce and public, ready to face future challenges.Read moreRead less