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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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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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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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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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; trying to understand why certain elements are more abundant than others; or how the different populations of stars in globular clusters arose. How can we better approximate mixing during core He burning
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the optimisation of extrusion conditions and enhancing product quality attributes. This role will involve a deep investigation to understand the influence of ingredient physico-chemical properties, extrusion
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sequence dataHOW TO APPLYPlease ensure that you are eligible for admission into the Graduate Research program at Monash University prior to applying.To apply, please send your CV, a copy of your full
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well as other research-related expenses. Please note: applicants who already hold a PhD will not be considered. Current Monash PhD students in the first year (12 months) of candidature (whether pre or post