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Current reseach is in the areas of: Development of biomimetic structures as ultrasound contrast agents Deep tissue imaging using photoacoustic contrast agents All optical photoacoustic sensors
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I supervise projects considering the evolution of accretion discs and their connection to observations. In particular, I consider discs that are warped or distorted (not flat). This geometry has
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LHCb experiment Searching for matter-antimatter differences in charm hadron decays Developing new probes to characterise proton-proton collisions web page For further details or alternative project
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in galaxies: how gas and dust form molecular clouds, how stars are born from these environments, and how stellar evolution and feedback return material back to the interstellar medium. Stars are born
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materials and we utilise these non-absorbed X-rays to massively increase image contrast and reduce radiation exposure using coherent synchrotron radiation. We have developed these “phase contrast” and “dark
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I supervise projects in particle physics. My main emphasis is on phenomenology, comparison of predictions with experimental measurements. I follow developments in flavour physics: weak decays
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Energy Market Operator (AEMO) launched the Zema Energy Studies Scholarship in March 2019, world-class PhD program to develop the nation’s future energy leaders. The Zema Scholarship aims to create a cohort
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datasets developed by Turning Point, including the National Ambulance Surveillance System and population-based resources involving the National Health Data Hub to answer these questions. This work will
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the development of numerical methods for astorphysical fluid dynamics and radiation transport. Projects may employ a range of approaches from analytic modelling and numerical calculations on desktop
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the Universe, e.g., where did the carbon in your bodies come from? What type of star made it? Generally we study stars in their final phases of evolution, when they become ageing red giants which is when