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computers to large-scale multi-dimensional simulations on high-end supercomputers, depending on your interests and inclinations. "Modelling extreme supernova explosions: From fast and faint to bright and
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difference between cold-related discomfort and illnesses such as hypothermia, and what to do about it if your heating is not working. 25 Jun 2025 News UoM Influenza Vaccination Program 2025 Program for 2025
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in a full-time program of research consistent with the objectives of Tour de Cure, leading to the awarding of a PhD or equivalent research doctorate. Applicants must be current holders of a PhD
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My research focuses on strongly interacting quantum systems at the interface between condensed matter physics and ultracold atomic gases. In particular, I am interested in the interplay between few- and many-body physics in scenarios ranging from superfluids to quantum impurity problems to...
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admission requirements. Meet university English language requirements. Not have previously completed a PhD. Be able to commence the Program in the year of the offer. Enrol as a full-time PhD student. Be
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analytical imaging methods, then working with collaborators to apply these methods to biomedical research, diagnostic imaging and beyond. Research projects vary from purely theoretical, to computational
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I supervise computational projects in electron microscopy imaging for investigating materials at atomic resolution. Some projects centre on analysing experimental data acquired by experimental
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My area of expertise is condensed matter theory. I am interested in the interplay between interactions and unconventional electronic properties of novel materials including graphene, topological insulators and Weyl semimetals. The former favours quantum states of matter (e.g. excitonic...
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-class honours (H1) Bachelor’s degree or equivalent in the relevant research area (completed or near completion) have applied for admission to a PhD program at an Australian university or have completed
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My research interests focus on the stars - primarily their structure, evolution and nucleosynthesis. This can involve modelling of mixing in stars, or effects of changing nuclear burning rates; trying to understand why certain elements are more abundant than others; or how the different...