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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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, which are some of the most numerous stars in the Universe. "Weighing stars using stellar vibrations: Asteroseismic masses of Red Giant Stars using space telescope data" "Using optical telescope
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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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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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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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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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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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, 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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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