704 postdoctoral-image-processing-in-computer-science-"Prof" positions at Monash University in Australia
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Training Program Coordinator Job No.: 680641 Location: Clayton campus Employment Type: Part-time, fraction (0.5) Duration: 12-month fixed-term appointment Remuneration: Pro-rata of $96,768
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synchrotron X-ray characterisation of solution-processed semiconductor films Supervisor: Prof. Chris McNeill, Department of Materials Science and Engineering (Email: christopher.mcneill@monash.edu ) For further
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Australian Research Council (ARC) Funded PhD Opportunity at Faculty of Engineering: High-Speed Rail and Sustainable City Sizes in Australia Location: Clayton campus Department/Unit: Monash Institute
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group, we synthesise these functional nanomaterials from the bottom-up, using protocols of molecular beam epitaxy and on-surface supramolecular chemistry. We study these systems by means
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My research focuses on strongly interacting quantum systems at the interface between condensed matter physics and ultracold atomic gases. In particular, I am interested in the interplay between few- and many-body physics in scenarios ranging from superfluids to quantum impurity problems to...
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" "Searching for physics beyond general relativity with gravitational-waves" (with Prof Paul Lasky) "Improving the sensitivity of gravitational-wave detectors" (with Prof Paul Lasky) "Detecting dark matter with
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between theoretical and computational high-energy physics. The research contributes to the world-leading PYTHIA Monte Carlo Event Generator, which serves as the baseline for the majority of experimental
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stars using stellar evolution" (with Prof Ilya Mandel) "The impact of new carbon burning rates on the AGB-supernovae mass boundary" (with Prof Alexander Heger) "The connection between novae and Type Ia
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the next generation of standard models with GAMBIT" "Using the Higgs boson to search for dark matter particles and other new physics" "Detecting dark matter with the Cherenkov Telescope Array (with Prof Eric
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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