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modelling astrophysical phenomena. The PhD project will focus on developing theoretical methods to generate accurate data to meet this demand. The student will gain expertise in high-performance computational
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N/A Footnotes for the table Masters Programs at AQF9 where the second-year research component qualifies for an RTP 1 EFTSL research project similar to Honours that is part of a coursework Masters
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Change lives and change the world with an impactful PhD as a component of the Long-term Trials of Drought Resilient Farming Practices Grants, Future Drought Fund (Australian Government) project
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Characterization Techniques Study the advanced electrochemical characterization methods. Gain deep insights into the reaction models associated with PCFCs. 3) Understanding of Electrocatalytic Performance and
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can occur that are very different to the macroscopic world. Our group develops methods to measure and ‘see’ this atomic detail using some of the world’s most powerful electron microscopes. We apply
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I supervise a wide range of projects stellar astronomy. They include modelling stars in 1D or 3D, deciphering the origin of the elements (stellar nucleosynthesis), and observing using optical
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development and application of a range of geochronological methods and mineral characterization techniques (primarily (U-Th)/He dating, U-Th disequilibrium and U-Pb dating, ToF-SIMS, etc.). The project will
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applied physics other related disciplines. Demonstrated knowledge in at least one of the following areas: porous media flow computational fluid dynamics (CFD) pore-network modelling lattice Boltzmann method
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considered in the current models. whether there are common points in multiple models. This will identify potentially critical points for new models. identify upstream and downstream points not previously
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Conventional x-ray imaging is firmly established as an invaluable tool in medicine, security, research and manufacturing. However, conventional methods extract only a fraction of the sample