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you as a result of your visit to websites controlled by The University of Melbourne. View Privacy at The University of Melbourne Detailed information about privacy, including statements, and policies
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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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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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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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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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brings about. Some relevant areas of interest include: Sociology of consumption in particular how people respond to social and economic incentives and barriers to energy efficient homes; Environmental
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Status: Open Applications open: 8/11/2023 Applications accepted at any time View printable version [.pdf] About this scholarship Description/Applicant information Three PhD positions are immediately
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and approximate costing of the field work, and a statement of the funds available and how the grant funds will be used. A brief reference from your supervisor. Applications to be submitted via email to