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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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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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the most interesting thermonuclear reactions occur deep in their interiors; the red giant phase is also when stars are more likely to interact with a gravitionally bound companion, if they have one! Students
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Health & Safety Connecting you to resources to ensure your safety and wellbeing on campus. Search for our Health & Safety documents such as procedures, requirements, guidances, registers, forms, safety bulletins and templates. If you are unable to find the document you’re searching for, please...
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environments and embrace different cultures. I initially wanted to become a psychiatrist, so I pursued an undergraduate degree in medical science at UNSW. While studying, I developed a stronger interest in
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environment for all members of our community, we ask users to abide by these Terms of Service. View Online Privacy Statement This privacy statement relates only to the information automatically collected from
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I am an experimental particle physicist and I specialise in the study of particles containing the beauty and charm quarks. My research aims to help improve our understanding our universe by comparing our experimental observations to predictions made using the Standard Model of Particle...
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, the University of Melbourne’s main Parkville campus is a well-known city landmark, with unique cultural, architectural and landscape features and facilities. Our other campuses are spread across Melbourne and
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role. Content creators Designers Developers View web publishing guidelines Project Management Roles and responsibilities by project stage. Getting accessibility advice Procurement questions Tender
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-class honours (H1) Bachelor’s degree or equivalent in the relevant research area (completed or near completion) have applied for admission to a PhD program at an Australian university or have completed