The triple–alpha reaction leading to the formation of stable carbon in the Universe is one of the most important nuclear astrophysical processes.  This project is aiming to improve our knowledge of the triple-alpha reaction rate from the direct observation of the electron-positron pair decays of the Hoyle state in ¹²C.

The Cretaceous–Tertiary (K–T) mass extinction about 66 million yearsa go is believed to be caused by a massive impact, most likely an asteroid or a comet. Within this project we will analyse a sample from this time to search for supernova-signatures.

Detection of supernova‐produced (radio)nuclides in terrestrial archives gives insight into massive star nucleosynthesis; when and where are heavy elements formed. Direct observation of radioactive nuclides from stars and the interstellar medium would provide first experimental constraints on production rate.s We will use the most sensitive technique, accelerator mass spectrometry.

Multiple projects are available to support the SABRE dark matter particle experiment. These include local experiments at ANU, computer simulations to predict backgrounds and the overall experimental sensitivity, data acquisition system development and analysis of the SABRE measurement data.

A fundamental scientific question is a better understanding of the elemental abundances and the isotopic pattern of our solar system which is a fingerprint of stellar nucleosynthesis. We perform nucleosynthesis in the laboratory at the ANU via a new and powerful tool, accelerator mass spectrometry, to elucidate open questions in these processes.

This experiment will characterise dark matter detector material. Lowest levels of natural radioactivity in high purity samples will be analysed via ultra-senstive single atom counting using acclerator mass spectrometry.

Motivated by exciting prospects for measurements of the magnetism of rare isotopes produced by the new radioactive beam accelerators internationally, this experimental and computational project seeks to understand the enormous magnetic fields produced at the nucleus of highly charged ions by their atomic electron configuration.

This project aims to develop biophysics and radiobiological applications of beams from the Heavy Ion Accelerator Facility with a view to advancing the medical applications of nuclear technology.

This project aims to develop biophysics and radiobiological applications of beams from the Heavy Ion Accelerator Facility with a view to advancing the medical applications of nuclear technology.

The measurement of the lifetimes of excited nuclear states is foundational for understanding nuclear excitations. This project covers three measurement methods that together span the nuclear lifetime range from about 100 femtoseconds to many nanoseconds. The project can include equipment development, measurement, and the development of analysis methodology (programming and computation). 

This project will develop an R&D prototype particle detector as part of the CYGNUS dark matter collaboration

Following nuclear decay involving electron capture and/or internal conversion the  daughter atom will be ionised, resulting the emission of a cascade of X-rays and Auger electros. The project is aiming to develop a new model required for basic science and applications, including cancer treatment.

Nuclear data are urgently required in national security, non-proliferation, nuclear criticality safety, medical applications, fundamental science and for the design of advanced reactor concepts (fusion, e.g. ITER), or next generation nuclear power plants (Gen IV, accelerator driven systems, ...).

This project evaluates data at the interface of nuclear, atomic and solid-state physics with a view to discovering new physics and providing reliable data on the magnetic moments of short-lived nuclear quantum states. It assists the International Atomic Energy Agency to provide reliable nuclear data for research and applications.

Investigate the internal structure of atomic nuclei by constructing the spectrum of excited states using time-correlated, gamma-ray coincidence spectroscopy.

Motivated by exciting prospects for measurements of the magnetism of rare isotopes produced by the new radioactive beam accelerators internationally, this experimental and computational project seeks to understand the enormous magnetic fields produced at the nucleus of highly charged ions by their atomic electron configuration.

Nuclear data are urgently required in national security, non-proliferation, nuclear criticality safety, medical applications, fundamental science and for the design of advanced reactor concepts (fusion, e.g. ITER), or next generation nuclear power plants (Gen IV, accelerator driven systems, ...).

Coulomb excitation is a reaction mechanism that proceeds via purely electromagnetic interactions and enables measurement of the nuclear shape. A new program of Coulomb excitation measurements is planned to understand how collective nuclear motion can emerge in a nucleus made of ~100 nucleons.

The measurement of the lifetimes of excited nuclear states is foundational for understanding nuclear excitations. This project covers three measurement methods that together span the nuclear lifetime range from about 100 femtoseconds to many nanoseconds. The project can include equipment development, measurement, and the development of analysis methodology (programming and computation). 

The triple–alpha reaction leading to the formation of stable carbon in the Universe is one of the most important nuclear astrophysical processes.  This project is aiming to improve our knowledge of the triple-alpha reaction rate from the direct observation of the electron-positron pair decays of the Hoyle state in ¹²C.

This project will develop an R&D prototype particle detector as part of the CYGNUS dark matter collaboration

This project seeks to develop and use a new proton-gamma detector system to investigate the level structure of a range of nuclei in the N=Z=20 to 28 region, specifically to determine the electric monopole strengths between 0+ states and invesitgate the presence and degree of shape coexistence in this region.

High energy heavy ion beams can be use to effectively treat cancerous tumours, but nuclear reactions of the ¹²C beam spread the dose, potentially harming healthy tissue. This project will investigate nuclear reaction cross sections relevant to heavy ion therapy.

The Cretaceous–Tertiary (K–T) mass extinction about 66 million yearsa go is believed to be caused by a massive impact, most likely an asteroid or a comet. Within this project we will analyse a sample from this time to search for supernova-signatures.

Fusion probabilities at high energies are significantly smaller than theoretical predicted, in part due to disintegration of the projectile nucleus into lighter nuclei (breakup) on timescales faster than 10^-21 s. This project will help us understand these fast, complex breakup processes and their influence on fusion.

The project is aiming to develop a high resolution conversion electron spectrometer to study electric monopole transitions in atomic nuclei. 

A reading course on the connections between the representation theory of Lie groups and the properties of fundamental particles within quantum field theory, using Howard Georgi's "Lie Groups in Particle Physics: from Isospin to Unified Theories".

Analytic solutions of real-world quantum mechanics problems are rare, and in practise we must use numerical methods to obtain solutions. This project will give you practical experience in solving the static and time-dependent Schrödinger equations using a computer.

Detection of supernova‐produced (radio)nuclides in terrestrial archives gives insight into massive star nucleosynthesis; when and where are heavy elements formed. Direct observation of radioactive nuclides from stars and the interstellar medium would provide first experimental constraints on production rate.s We will use the most sensitive technique, accelerator mass spectrometry.

Nuclei are complex quantum systems and thus require advanced modelling to understand their structure properties. This project uses such models to interpret experimental data taken at the ANU and at overseas nuclear facilities.

Electric monopole (E0) transitions between nuclear states with same parity and spin are very sensitive tools to examine structural changes. This project is aiming to develop a new high resolution setup to measure angular correlations between conversion electrons and gamma rays.

Compact particle detectors using exotic, new scintillator materials and silicon photomultipliers are being developed for varied roles in our nuclear structure research program.

Exotic nuclei, in their long-lived ground and excited states, are produced in nuclear reactions, transported through an 8T superconducting solenoid magnet to separate them in time and space from the intense beam-induced background, before studying their decay with an array of electron and gamma-ray detectors.

Following nuclear decay involving electron capture and/or internal conversion the  daughter atom will be ionised, resulting the emission of a cascade of X-rays and Auger electros. The project is aiming to develop a new model required for basic science and applications, including cancer treatment.

Superheavy elements can only be created in the laboratory by the fusion of two massive nuclei. Our measurements give the clearest information on the characteristics and timescales of quasifission, the major competitor to fusion in these reactions.

Multiple projects are available to support the SABRE dark matter particle experiment. These include local experiments at ANU, computer simulations to predict backgrounds and the overall experimental sensitivity, data acquisition system development and analysis of the SABRE measurement data.

This research project, with both experimental and theoretical angles, is developing a new perspective on the transition from a quantum superposition to effectively irreversible outcomes in quantum collisions.

A fundamental scientific question is a better understanding of the elemental abundances and the isotopic pattern of our solar system which is a fingerprint of stellar nucleosynthesis. We perform nucleosynthesis in the laboratory at the ANU via a new and powerful tool, accelerator mass spectrometry, to elucidate open questions in these processes.

This project evaluates data at the interface of nuclear, atomic and solid-state physics with a view to discovering new physics and providing reliable data on the magnetic moments of short-lived nuclear quantum states. It assists the International Atomic Energy Agency to provide reliable nuclear data for research and applications.

Contribute to the development of a new experimental research program at the ANU Heavy Ion Accelerator Facility and investigate the internal structure of atomic nuclei with nucleon transfer reactions. Interested students will have the opportunity to undertake research projects in nuclear instrumentation, software development and fundamental physics. 

This experiment will characterise dark matter detector material. Lowest levels of natural radioactivity in high purity samples will be analysed via ultra-senstive single atom counting using acclerator mass spectrometry.

This project builds on our established track record of developing novel methods to measure magnetic moments of picosecond-lived excited states in atomic nuclei, and the theoretical interpretation of those measurements. Students will help establish new methodologies to underpin future international research at the world's leading radioactive beam laboratories.

 

Analytic solutions of real-world quantum mechanics problems are rare, and in practise we must use numerical methods to obtain solutions. This project will give you practical experience in solving the static and time-dependent Schrödinger equations using a computer.

This research project, with both experimental and theoretical angles, is developing a new perspective on the transition from a quantum superposition to effectively irreversible outcomes in quantum collisions.

Fusion probabilities at high energies are significantly smaller than theoretical predicted, in part due to disintegration of the projectile nucleus into lighter nuclei (breakup) on timescales faster than 10^-21 s. This project will help us understand these fast, complex breakup processes and their influence on fusion.

A reading course on the connections between the representation theory of Lie groups and the properties of fundamental particles within quantum field theory, using Howard Georgi's "Lie Groups in Particle Physics: from Isospin to Unified Theories".

Nuclei are complex quantum systems and thus require advanced modelling to understand their structure properties. This project uses such models to interpret experimental data taken at the ANU and at overseas nuclear facilities.

This project builds on our established track record of developing novel methods to measure magnetic moments of picosecond-lived excited states in atomic nuclei, and the theoretical interpretation of those measurements. Students will help establish new methodologies to underpin future international research at the world's leading radioactive beam laboratories.