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computational while other work will involve time spent in the lab. Search for physics beyond the Standard Model in penguin decays in data from the LHCb experiment. Identify particle identification requirements
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requirements of, and being formally enrolled in, the relevant PhD program at QUT. What happens next? Only applicants who are successful in the project selection process and formally notified will be invited
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My work focuses on experimental research in quantum sensing and quantum microscopy using the nitrogen-vacancy (NV) centre in diamond. In particular, we are interested in applying quantum sensing for examining and imaging the magnetic fields from exotic conducting materials (e.g. superconductors,...
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use speech recognition Top Tools Digital tools Using TurnItIn with JAWS Accessibility statement regarding TurnItIn. Getting Started with Microsoft Word Dictate Take audio from the computer's microphone
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project support scholarship. The student will still require the award of a research scholarship from QUT as part of their admission to the higher degree by research (HDR) program. Preference will be given
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Connect with a peer Support Groups Information Forums IBD Service Locator Young Adult Support Youth Support Toggle Sub Navigation Camp Fearless Youth Empowerment Program Kids Fun Day For Health
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Duration: 3.5-year fixed-term appointment Remuneration: The successful applicant will receive a tax-free stipend of $37,145 per annum (2026 full-time rate), as per the Monash Research Training Program (RTP
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I supervise a wide range of projects in stellar astrophysics, with a focus on low and intermediate-mass stars, which have masses similar to or slightly larger than our Sun. This work is carried out within the Centre of Excellence for Astrophysics in 3D: ASTRO 3D. As a member of my group, you...
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Any HDR student wishing to study in biomedical research Eligibility criteria The successful candidate must meet the minimum academic entry requirement for admission into the Doctor of Philosophy program
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I work on the study of massive and supermassive stars (10-100,000 solar masses); the first generations of stars in the universe (Pop III stars); evolution of rotating massive stars and the spin of their remnants (including predictions for GW sources); mixing and transport processes in the...