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-loss from AGB and RSG stars to study the release of elements and material into the Interstellar Medium. Simulating the mixing of elements and material released from SNe within the ISM - tracing and
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cosmolgy, galaxy evoltion and stellar astrophysics. Students in my group primarily perform numerical simulations of stars, in order to study broad questions related to the origin of the elements in
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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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supergiant stars right before the explosion Searching different astrophysical channels that produce r-process elements Connecting the properties of long-duration gamma-ray bursts and associated supernovae web
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stellar interiors, birth properties of black holes and neutron stars, supernova light curves and spectra, gravitational waves, neutrino astrophysics, the production of heavy elements stellar explosions, and
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-ray speckle-based imaging, a simple and flexible technique using just a piece of sandpaper as an optical element to access the phase-contrast and dark-field image modalities. Using this method, I
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of their remnants (including predictions for GW sources); mixing and transport processes in the stellar interior; nucleosynthesis and the origin of elements, including galacto-chemical evolution - which elements
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degree in a relevant field, with a significant research component and first-class honours/H1 (or equivalent). Desirable attributes include: training in qualitative, quantitative, or mixed methods
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, the selection committee will prioritise applicants who hold an Australian (or equivalent international) Honours or Master’s degree in a relevant field, with a significant research component and first-class
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Honours (H1) in Civil Engineering, Materials Engineering, Environmental Engineering, Chemical Engineering, or a closely related field; or A Master’s degree with a substantial research component Application