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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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leader of a new nanophotonics laboratory led by Prof. Stefan Maier at Monash, my team will have the opportunity to work with colleagues from an interdisciplinary environment and collaborators around the
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will have the opportunity to interact with gravitational-wave researchers throughout Australia and around the world. Students in my group use data from the Laser Interferometer Gravitational-wave
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theoretical colleagues. All research takes place within our dynamic particle physics research group with academics and postdocs, as well as graduate and undergraduate students. Some work will be purely
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with leading researchers in glass science/engineering and diffraction physics/crystallography in Australia and around the world. "Local structure and symmetry in metallic glasses" (with Assoc Prof Scott
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As part of the establishment grant for the Monash Assistive Technology and Society (MATS) Centre (https://www.monash.edu/mats/about), the Faculty of IT is providing a scholarship to support the
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My research focusses on understanding stars: their evolution and chemical composition, and how they move throughout our galaxy. Most of what we know about the universe comes from starlight, but
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, as well as at the Australian Synchrotron and other Synchrotrons around the world. Students in my group work on growing materials atom by atom (often only a single atomic layer thick)and then study the
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, with particular focus on modelling and simulation. Some example projects include: "The impact of stellar rotation on the nucleosynthesis in the first generation of stars" "Stripping of planets by
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As a pregnancy approaches term (the point at which the foetus is considered fully developed), decisions are made about the timing of birth and the way babies are born. These decisions are incredibly