176 web-programmer-developer-"https:"-"University-of-Cambridge"-"https:" PhD positions in Australia
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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
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inform or design future experiments. As a researcher in my group, you would not only develop imaging theory and analysis tools to answer science questions about where the atoms are, what they are, and how
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leading team, access world-class research facilities, publish in top journals, and develop expertise in soil and climate change science, fieldwork, laboratory methods, and environmental modelling.
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ferroelectrics for low-energy electronics" "hot-electron thermoelectricity in graphene for generating power from the cold night sky" "bilayer graphene negative-capacitance transistors" web page For further details
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the diverse range of knowledge and skills of CaLD customers and employees. This project aims to use social identity theory and role theory to develop a comprehensive conceptual model for the process by which
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The Mymobility Scholarship is funded by Zimmer Biomet to support a full-time PhD student who is commencing research in orthopaedics and patient monitoring. Mymobility was developed by Zimmer Biomet
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ecological problems (climate change, species extinction, urbanisation) and a shift in social and political attitudes with regard to human impact on the nonhuman world call for the development of a new
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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