The origin and evolution of heavy elements in the early universe. Everything in our Solar System, including all life on Earth, was created long ago out of material forged inside fiery stellar furnaces. The latest theoretical simulations of element production in red giant stars reveals the processes that gave us our existence, as well as help us to understand the origin of the galaxy that we inhabit.
Precision pair spectroscopy of the Hoyle state. This project aims to develop a novel new spectrometer to observe and characterise electron-positron pairs of high energy nuclear transitions with unprecedented precision. Building on unique Australian expertise and equipment, the outcomes will include new applications of electron spectroscopy to nuclear structure studies, and a better understanding of element synthesis in the universe, including the formation of 12C in the universe.
The origin of the elements heavier than iron. This research investigates the cosmic origin of the elements heavier than iron, as they are produced by nuclear reactions inside stars. The study of these elements in stars and meteorites will help us to understand the origin and history of the Solar System, of old stars and of stellar clusters and galaxies.
Developing a complete understanding of nuclear fission. This project aims to develop a reliable predictive model of nuclear fission. Nuclear fission is an important process in fundamental physics and technologies spanning energy, medicine and materials science. It was recently found that fission still holds many secrets, since existing models fail to describe new fission measurements for nuclei lighter than the well-known uranium region. This project plans to exploit world-leading Australian res ....Developing a complete understanding of nuclear fission. This project aims to develop a reliable predictive model of nuclear fission. Nuclear fission is an important process in fundamental physics and technologies spanning energy, medicine and materials science. It was recently found that fission still holds many secrets, since existing models fail to describe new fission measurements for nuclei lighter than the well-known uranium region. This project plans to exploit world-leading Australian research equipment to map out unknown fission characteristics in large regions of the nuclear chart, providing a complete microscopic understanding of nuclear fission. This is designed to lead to the first predictive model applicable to the entire nuclear chart, including nuclei of astrophysical importance.Read moreRead less
Laboratory studies of Nucleosynthesis via Accelerator Mass Spectrometry. This project aims at laboratory studies of stellar nucleosynthesis applying ultra-sensitive accelerator mass spectrometry (AMS) measurements. The project will focus on reactions which are essential to open questions in modelling nucleosynthesis in stars, that is where no data exist at all, or are scarce and discrepant; in particular for neutron- and charged-particle induced reactions relevant to the s-and p-process where an ....Laboratory studies of Nucleosynthesis via Accelerator Mass Spectrometry. This project aims at laboratory studies of stellar nucleosynthesis applying ultra-sensitive accelerator mass spectrometry (AMS) measurements. The project will focus on reactions which are essential to open questions in modelling nucleosynthesis in stars, that is where no data exist at all, or are scarce and discrepant; in particular for neutron- and charged-particle induced reactions relevant to the s-and p-process where an extremely sensitive detection method is required. New data for key nuclear reactions will be connected with theory, for testing and improving theoretical predictions. They will be highly beneficial for modelling the respective nucleosynthesis processes in stars and for our understanding of the elemental abundance of our solar system.Read moreRead less
Creating superheavy elements and isotopes. This project aims to measure properties, probabilities and timescales of competing quasifission processes, by combining Australian accelerator and detector capabilities with exotic radioactive targets. In 2015, nuclear fusion created superheavy elements with atomic numbers 113 to 118. The race is now on to create elements 119 and 120, as their production and properties should pin down the location of the predicted superheavy Island of Stability, but 3-f ....Creating superheavy elements and isotopes. This project aims to measure properties, probabilities and timescales of competing quasifission processes, by combining Australian accelerator and detector capabilities with exotic radioactive targets. In 2015, nuclear fusion created superheavy elements with atomic numbers 113 to 118. The race is now on to create elements 119 and 120, as their production and properties should pin down the location of the predicted superheavy Island of Stability, but 3-fragment quasifission is a major impediment to their formation. This project will evaluate quassification processes on the nuclear reactions proposed to form new superheavy elements and is expected to identify the best reactions for their discovery. The synthesis of new elements tests quantum physics, relativistic chemistry and element creation in the cosmos, and offers high profile returns on investments.Read moreRead less
Imaging the spatial distribution of forces that bind quarks to a proton. This project will perform supercomputer simulations to resolve the distribution of forces acting on quarks inside the proton. New knowledge will be generated in the area of fundamental strong-interaction physics by developing innovative approaches to image novel features that have not been possible in the past. The outcomes will therefore open new research possibilities by expanding the capacity of the international communi ....Imaging the spatial distribution of forces that bind quarks to a proton. This project will perform supercomputer simulations to resolve the distribution of forces acting on quarks inside the proton. New knowledge will be generated in the area of fundamental strong-interaction physics by developing innovative approaches to image novel features that have not been possible in the past. The outcomes will therefore open new research possibilities by expanding the capacity of the international community to study strong interaction physics—including direct relevance to experimental research at the recently-upgraded Jefferson Lab in the US. In analogy to Rutherford's atomic model, the results will have benefit to future generations of humanity with a deeper understanding of the structure of matter.Read moreRead less
Nuclear vibrations under scrutiny in near-spherical and deformed nuclei. This Project aims to elucidate the nature of nuclear vibrations. Evidence is mounting that nuclear excitations long identified as vibrations cannot truly be so. This shakes the foundations of nuclear theory. Coulomb excitation and transfer reaction experiments are to be developed to probe the structure of these quantum states. Expected outcomes include clarification of their true nature and a deeper understanding of why nuc ....Nuclear vibrations under scrutiny in near-spherical and deformed nuclei. This Project aims to elucidate the nature of nuclear vibrations. Evidence is mounting that nuclear excitations long identified as vibrations cannot truly be so. This shakes the foundations of nuclear theory. Coulomb excitation and transfer reaction experiments are to be developed to probe the structure of these quantum states. Expected outcomes include clarification of their true nature and a deeper understanding of why nuclei differ from other many-body quantum systems that do vibrate. Anticipated benefits include enduring methodologies to facilitate international research engagement, and rigorous hands-on training in nuclear methods, to help meet Australia’s need for nuclear-qualified personnel in health, mining, industry and security.Read moreRead less
Supercomputing the tomography of the proton. This project aims to produce theoretical determinations of the quark and gluon distributions of the proton through advanced supercomputer simulations. The project will generate new knowledge in the area of fundamental strong-interaction physics by developing innovative approaches to image structures that have not been possible in the past. This project expects to expand the capacity of the international community to study strong interaction physics, i ....Supercomputing the tomography of the proton. This project aims to produce theoretical determinations of the quark and gluon distributions of the proton through advanced supercomputer simulations. The project will generate new knowledge in the area of fundamental strong-interaction physics by developing innovative approaches to image structures that have not been possible in the past. This project expects to expand the capacity of the international community to study strong interaction physics, including direct relevance to experimental research at the recently-upgraded Jefferson Lab in the US. In analogy to Rutherford's atomic model, the results will have benefit to future generations of humanity with a deeper understanding of the structure of matter.Read moreRead less
Emergent Phenomena in the Foundation of Matter. This project aims to explore the finite-matter-density features of the relativistic field theory of the strong interactions, Quantum Chromodynamics (QCD). Drawing on national supercomputing resources, this project will undertake QCD calculations of unprecedented complexity to discover emergent phenomena in the ground-state quantum fields that form the foundation of matter. By studying their evolution under temperature and matter density and explori ....Emergent Phenomena in the Foundation of Matter. This project aims to explore the finite-matter-density features of the relativistic field theory of the strong interactions, Quantum Chromodynamics (QCD). Drawing on national supercomputing resources, this project will undertake QCD calculations of unprecedented complexity to discover emergent phenomena in the ground-state quantum fields that form the foundation of matter. By studying their evolution under temperature and matter density and exploring their contribution to the structure of the nucleon and its excitations, the research will advance theoretical understanding and challenge experimental programs. Benefits include transferable skills in advanced analytical techniques, high-performance computing, and scientific data visualisation.Read moreRead less