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; trying to understand why certain elements are more abundant than others; or how the different populations of stars in globular clusters arose. How can we better approximate mixing during core He burning
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and quantum impurities. A large part of my work is carried out within the Australian Centre of Excellence for Future Low-Energy Electronics Technologies (FLEET), where I am currently leading
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to which the candidate will be granted access, including single dedicated machines, national facilities, and commercial providers. In particular, support will be given by the Australian SKA Regional Centre
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to understand glass structures. Students in my team will be able to perform measurements at the Monash Centre for Electron Microscopy or the Australian Synchrotron. They will have the opportunity to collaborate
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formed? Why does the velocity distribution of hypervelocity stars ejected from the Galactic centre not match expectations? How are the birth masses and natal kicks of neutron stars and black holes
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I supervise a wide range of projects in gravitational-wave astronomy. This work is carried out within the Centre of Excellence for Gravitational-wave Discovery: OzGrav. As a member of my team, you
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energy. Within the Cherenkov Telescope Array (CTA) Consortium I study the possibility of detecting dark matter in the centre of our galaxy and beyond. With my colleagues in the Compact Linear Collider
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My work focuses on experimental research in quantum sensing and quantum microscopy using the nitrogen-vacancy (NV) centre in diamond. In particular, we are interested in applying quantum sensing
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national training centre (NTC), to be immersed in their daily high performance training environment working alongside and being mentored by professionals across the fields of sport science and sport medicine
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within the Centre of Excellence for Astrophysics in 3D: ASTRO 3D. As a member of my group, you will have the opportunity to interact with astronomers across Australia and the world, in fields as diverse as