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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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. "Studying the origin of the new discovered class of weak CN stars in the Magellanic Clouds using stellar variability" "How do stars merge? Studying the merger between low and intermediate-mass main-sequence
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: Full-time Duration: 3.5 years fixed-term appointment Supervisory Team: Professor Philip Russo (Main Supervisor) and others TBC Remuneration: A PhD annual stipend for 3.5 years of full-time PhD enrolment
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is desirable. In its assessment, the selection committee will prioritise applicants who hold an Australian (or equivalent international) Honours or Masters degree (in a relevant field), with a
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My primary areas of research activity are two fold: first, studing thermonuclear (X-ray) bursts from accreting neutron stars; and second, searches for optical counterparts of gravitational-wave
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primary structures that would otherwise be replaced to be certified under the current certification regulation/policy. Candidate Requirements Applicants will be considered provided that they fulfil
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Duration: 3.5 years fixed-term appointment Supervisory Team: Professor Elizabeth Manias (Main Supervisor) The successful candidate will be supported by a multidisciplinary project team with expertise in
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domestic candidate have the necessary qualifications, such as a research masters or honours year to meet the selection requirements into the doctoral program (see Monash University PhD entry requirements
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work rights. Candidates must have a bachelor's degree with honours or a master's in a relevant discipline, with strong academic results. The project would ideally suit candidates with a background in
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for admission to a PhD, detailed here: www.monash.edu/admissions/entry-requirements/minimum . Candidate Requirements Undergraduate Honours degree or Master's by research degree in a relevant discipline (Health