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PhD candidate will be integrated into an established research program funded by the Australian Research Council, with access to a large longitudinal dataset and to funding for qualitative fieldwork
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plasma‑filled bubbles are injected into water to create nitrogen oxides (NOₓ) directly from the air. Because the bubbles are so small, they provide a large contact area, making the process highly efficient
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comparing our experimental observations to predictions made using the Standard Model of Particle Physics. I am a member of the LHCb collaboration, one of the four large experiments at the Large Hadron
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understand where stars form, how stellar feedback changes their surroundings, and how matter moves through galaxies over time shaping them. Most of my research uses large astronomical data sets across
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understand our place in the cosmos. I am a member of most large stellar spectroscopic surveys (e.g., Gaia, SDSS-V, 4MOST, GALAH, Gaia-ESO), providing access to pan-optic data across all visible and infrared
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of mesons and baryons and their role as indirect probes for physics beyond the standard model. I also follow searches for new physics at the large hadron collider (LHC) and use them to constrain new particles
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- and many-body physics in scenarios ranging from superfluids to quantum impurity problems to light-matter coupled systems. A large part of my work is carried out within the Australian Centre
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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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We have several PhD opportunities available in areas such as Multimodal Large Language Models (MLLM) for human understanding, MLLM safety, and Generative AI. If you have published in top-tier
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process should be directed to; Dr Melinda (Millie) McCabe, Senior Project Co-ordinator, E: [email protected] . Applications Close: Monday 31 August 2026, 11:55pm AEST Supporting a diverse workforce