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including but not limited to data loss prevention (DLP), web application firewalls (WAF), API gateways, and cloud native security services across cloud platforms such as AWS, Microsoft Azure, or GCP. The role
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ChaptersToggle ACT NSW NT QLD SA TAS VIC WA PublicationsToggle NAWIC Journal Podcast Blog NAWIC in the News Chapter News Learning HubToggle Learning Hub Committee Access Our Policies Research Counselling and
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4 Cs Of Diamonds Learn About Natural Diamonds Lab Grown Diamonds Coloured Gemstones Precious Metals How To Care For Your Jewellery How To Measure Your Ring Size Blog Guides Engagement Ring Guide
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agency deadline) Directly to SSHRC : October 17, 2024 (8 p.m. eastern) How to apply See Application process Results announced April 2025 Apply Web CV, application and instructions Footnotes Footnote
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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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My research interests focus on the stars - primarily their structure, evolution and nucleosynthesis. This can involve modelling of mixing in stars, or effects of changing nuclear burning rates
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the development of numerical methods for astorphysical fluid dynamics and radiation transport. Projects may employ a range of approaches from analytic modelling and numerical calculations on desktop
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the evolution of massive binary stars into compact binaries as sources of gravitational-waves and astrophysical inference on gravitational-wave observations. My research group on massive binary evolution -- also
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for examining and imaging the magnetic fields from exotic conducting materials (e.g. superconductors, topological insulators), performing high bandwidth and high sensitivity vector magnetic sensing and developing
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is carried out within the LHCb collaboration that runs one of the four large experiments at the Large Hadron Collider at CERN as well as towards future collider developments. I supervise a number of