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My area of expertise is condensed matter theory. I am interested in the interplay between interactions and unconventional electronic properties of novel materials including graphene, topological
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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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to life in breakthrough experiments—please reach out. "Quantum nanophotonic chips" "Structured-light imaging and spectroscopy” “Meta-optics and meta-waveguides" "2D materials and Lightwave valleytronics
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-matter quasiparticles" "Atomically thin materials coupled to light" "Periodically driven many-body systems" web page For further details or alternative project arrangements, please contact: meera.parish
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Petersen (MCEM)) "Frustration and complexity in glasses" (with Dr Tim Petersen (MCEM)) "Local structures in soft colloidal materials with anisotropic particles" (with Prof Rico Tabor (Chemistry)) web page
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interdisciplinary and topical, and by now 21 people from my lab hold faculty positions all over the world. Nanostructured materials for efficient solar energy conversion Optical metasurfaces for quantum optics (with
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I supervise a wide range of projects stellar astronomy. They include modelling stars in 1D or 3D, deciphering the origin of the elements (stellar nucleosynthesis), and observing using optical telescopes (high-resolution spectroscopy) and space-based telescopes (asteroseismology). The uniting...
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I supervise a wide range of projects in gravitational-wave astronomy. This work is carried out within the Centre of Excellence for Gravitational-wave Discovery: OzGrav. As a member of my team, you will have the opportunity to interact with gravitational-wave researchers throughout Australia and...
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theoretical colleagues. All research takes place within our dynamic particle physics research group with academics and postdocs, as well as graduate and undergraduate students. Some work will be purely
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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...