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
Radio follow-up of gravitational wave events. This project aims to use three Australian radio telescopes to search for and monitor radio waves from future gravitational wave events. The detection of gravitational waves and electromagnetic radiation from a neutron star merger was a scientific breakthrough, with important implications for physics and astronomy. The observations from this project will provide key information to reveal what causes some of the most energetic events in the Universe, t ....Radio follow-up of gravitational wave events. This project aims to use three Australian radio telescopes to search for and monitor radio waves from future gravitational wave events. The detection of gravitational waves and electromagnetic radiation from a neutron star merger was a scientific breakthrough, with important implications for physics and astronomy. The observations from this project will provide key information to reveal what causes some of the most energetic events in the Universe, their environment and how they evolve. The outcomes of this project include increased international collaboration with this global effort, and new techniques for automatic data processing and analysis, as well as engaging future students as we build Australian expertise in a new area of research.Read moreRead less
Illuminating the cosmic web with Fast Radio Bursts. This project aims to establish the use of millisecond-duration Fast Radio Bursts as a wholly new means to map out the distribution of matter in the Universe. This project expects to localise 100s of bursts using novel infrastructure deployed on Australia's largest radio telescopes. Expected outcomes include an understanding of the processes that shape both the large-scale structures of the Universe, and the extreme conditions that exist at the ....Illuminating the cosmic web with Fast Radio Bursts. This project aims to establish the use of millisecond-duration Fast Radio Bursts as a wholly new means to map out the distribution of matter in the Universe. This project expects to localise 100s of bursts using novel infrastructure deployed on Australia's largest radio telescopes. Expected outcomes include an understanding of the processes that shape both the large-scale structures of the Universe, and the extreme conditions that exist at the sites of Fast Radio Bursts. This should provide significant benefits to our fundamental knowledge of the Universe, inspire students into careers in science, technology, engineering and mathematics, and develop signal processing techniques of application to both the Square Kilometre Array and industry.Read moreRead less
Violation of fundamental symmetries in atoms, molecules and nuclei. This theoretical project aims to predict enhanced effects of parity (P), time reversal (T), CP and Lorentz invariance violation, which may be measured using atomic spectroscopy and nuclear physics methods. This project expects to contribute to search for physics beyond standard model, including standard model extensions predicting axion, dark matter and T,P-violating electric dipole moments. Expected outcomes include predictions ....Violation of fundamental symmetries in atoms, molecules and nuclei. This theoretical project aims to predict enhanced effects of parity (P), time reversal (T), CP and Lorentz invariance violation, which may be measured using atomic spectroscopy and nuclear physics methods. This project expects to contribute to search for physics beyond standard model, including standard model extensions predicting axion, dark matter and T,P-violating electric dipole moments. Expected outcomes include predictions of new enhanced effects in nuclei, atoms and molecules. By-products and benefits include development of high precision computer codes for atomic calculations, which are expected to have numerous applications including photon and electron processes, properties of superheavy elements and atomic clocks.Read moreRead less
Violation of fundamental symmetries in atomic phenomena. Violation of the fundamental symmetries is predicted by unification theories of elementary particles. The aim of this project is to propose new enhanced effects of parity, time reversal and Lorentz invariance violations and perform their calculations needed to test unification theories in atomic and nuclear phenomena. By-products of this project include development of high precision computer codes for atomic calculations and theory of pro ....Violation of fundamental symmetries in atomic phenomena. Violation of the fundamental symmetries is predicted by unification theories of elementary particles. The aim of this project is to propose new enhanced effects of parity, time reversal and Lorentz invariance violations and perform their calculations needed to test unification theories in atomic and nuclear phenomena. By-products of this project include development of high precision computer codes for atomic calculations and theory of processes involving atoms and nuclei in chaotic excited states. These codes and theory are expected to have numerous applications (e.g. search for Dark Matter and atomic spectra of superheavy elements, atomic clocks and electron and photon processes).
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Space RAdiation Monitoring System (SRAMS) for safe space missions. The goal of the project is to develop a comprehensive space radiation monitoring system (SRAMS) that can evaluate: i) the radiation related hazards for astronauts, ii) the radiation damage in electronics during space missions and iii) the ground radiation facility environment used in radiation hardness assurance tests. SRAMS will also address important issue in space by minimizing manned or satellite space mission aborts due to s ....Space RAdiation Monitoring System (SRAMS) for safe space missions. The goal of the project is to develop a comprehensive space radiation monitoring system (SRAMS) that can evaluate: i) the radiation related hazards for astronauts, ii) the radiation damage in electronics during space missions and iii) the ground radiation facility environment used in radiation hardness assurance tests. SRAMS will also address important issue in space by minimizing manned or satellite space mission aborts due to space radiation adverse effects on astronaut’s health and electronics failure, and translates into an enormous economic value proposition. SRAMS will be paramount for leveraging the quantifiable standards of the space-radiation qualification facilities that are important for boosting the Australian Space industry. Read moreRead less
Counting neutrinos to per-mill accuracy. This Project aims to supply the most precise to-date calculation of a critical parameter in cosmology, the effective number of neutrinos, in the context of the standard model of particle physics. Crucial to the correct interpretation of cosmological observations, this parameter enables the reconstruction of the universe's timeline from which to infer its properties. The expected outcome is a number of 4-digit significance that can be used in all future co ....Counting neutrinos to per-mill accuracy. This Project aims to supply the most precise to-date calculation of a critical parameter in cosmology, the effective number of neutrinos, in the context of the standard model of particle physics. Crucial to the correct interpretation of cosmological observations, this parameter enables the reconstruction of the universe's timeline from which to infer its properties. The expected outcome is a number of 4-digit significance that can be used in all future cosmological computations/analyses. Besides raising Australia's international profile in basic science research, this project expects to provide significant societal benefits via the training of HDRs in advanced mathematical modelling and computing, transferable skills across many sectors.Read moreRead less
Discovery Early Career Researcher Award - Grant ID: DE210101593
Funder
Australian Research Council
Funding Amount
$462,948.00
Summary
Developing new tools to search for dark matter. This project aims to propose and assist in the development of novel approaches, based on atomic, molecular and optical technologies, to detect dark matter in the laboratory, and thereby establish the identity and microscopic properties of dark matter. The origin and nature of dark matter remains one of the most important outstanding problems in contemporary science. The intended outcome of this project is that the use of our novel methods will enab ....Developing new tools to search for dark matter. This project aims to propose and assist in the development of novel approaches, based on atomic, molecular and optical technologies, to detect dark matter in the laboratory, and thereby establish the identity and microscopic properties of dark matter. The origin and nature of dark matter remains one of the most important outstanding problems in contemporary science. The intended outcome of this project is that the use of our novel methods will enable us to search for forms of dark matter that have remained largely unprobed to date. This in turn is expected to open up new opportunities in the global hunt for dark matter that should improve our chances of finally discovering the nature and properties of dark matter.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE210100107
Funder
Australian Research Council
Funding Amount
$672,000.00
Summary
The next generation fast radio burst detector for Australia. This project intends to provide a next-generation fast radio burst detector for the Australian Square Kilometre Array Pathfinder. The project expects to both transform our understanding of fast radio bursts, enigmatic flashes of radio waves of unknown origin, but also use the bursts as tools to study the cosmic web of matter that resides in intergalactic space. To do so, the project aims to deliver a more sensitive detection system ca ....The next generation fast radio burst detector for Australia. This project intends to provide a next-generation fast radio burst detector for the Australian Square Kilometre Array Pathfinder. The project expects to both transform our understanding of fast radio bursts, enigmatic flashes of radio waves of unknown origin, but also use the bursts as tools to study the cosmic web of matter that resides in intergalactic space. To do so, the project aims to deliver a more sensitive detection system capable of localising a large sample of fast radio bursts to greater distances, found commensal to other observations. This should provide significant benefit, including the resolutions to key open astrophysical questions and improved scientific outcomes for transient searches with the Square Kilometre Array.Read moreRead less