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for physics beyond general relativity with gravitational-waves" (with Prof Eric Thrane) "Improving the sensitivity of gravitational-wave detectors" (with Prof Eric Thrane) web page For further details
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through theory and simulation and/or experimental design and testing; developing new image reconstruction algorithms for providing more information with less radiation; and applying our techniques
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and may include travel to one of our collaborator labs above. All the projects will make use of the world-class instruments at the Monash Centre for Electron Microscopy with unique electron-optics
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I supervise a wide range of PhD projects on experimental research into the electronic properties of novel quantum materials including topological insulators, graphene, and other atomically thin two-dimensional materials. I am interested in creating a low-power topological transistor, in which an...
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Help shape the future of solar energy. This iPhD project will develop a new technical framework for testing printed solar technologies—an emerging class of ultra-lightweight, flexible photovoltaics
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I study galaxies and active galactic nuclei, endeavouring to understand how galaxies grow, what regulates star formation within galaxies and what triggers active galactic nuclei. My students and I use imaging surveys at X-ray, optical, infrared and radio wavelengths to measure the emission from...
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Understanding factors related to student retention and experience in physics and astrophysics major units. Using quantitative (surveys) and qualitative data (interviews with students) this project aims to explore who takes physics and astrophysics major units, why they pursue them, and what...
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climate economy in Australia (Dr Svenja Keele ) Communicating Data to Advance Community and Ecological Wellbeing (Prof. Libby Lester ) Making Futures Together: Designing and Testing Creative Methods
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older adults”. This project will use a novel form of non-invasive brain stimulation combined with multimodal techniques to investigate how synchronising brain oscillations at specific frequencies can
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Observatory (LIGO) in order to understand the fate of massive stars, to probe how binary black holes form, and to understand the nature of matter at the most extreme possible densities. Occasionally, we