36 postdoctoral-in-optical-communication PhD positions at Monash University in Australia
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and may include travel to one of our collaborator labs above. All the projects will make use of the world-class instruments at the Monash Centre for Electron Microscopy with unique electron-optics
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of the barriers that people with disabilities face at school, university, work and in the social sphere. Our work is guided by on-the-ground partnerships with the community to ensure we’re addressing real problems
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optoelectronics, green energy, and fundamental quantum optics. As a member of my group you will have the opportunity to work with my DECRA sub-group leader Dr. Haoran Ren, and also with my research team at Imperial
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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
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insulators and Weyl semimetals. The former favours quantum states of matter (e.g. excitonic superfluidity, quantum magnetism, superconductivity), while the latter makes their optical and transport properties
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), singular optics, using electrons, atoms and light and the exploration of complex systems using statistical field theory. "Catastrophes on order-parameter manifolds" (with Dr Alexis Bishop and Dr Timothy
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, spectroscopy, astrometry) using massive optical telescopes on Earth and in space (e.g., Hubble, Gaia, JWST, Kepler, TESS). My group develops cutting-edge models to extract the most from noisy data and to better
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Zealand and Italy. "Structuring x-ray light to investigate the macro and microscale" "Dark-field x-ray imaging without optics" "Adding time to the X-ray Fokker-Planck Equation" (with Prof David Paganin
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incorporate other data as well, from gamma-ray burst satellites to optical surveys of flaring supermassive black holes. "Probing the population properties of merging binary black holes with gravitational waves
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My primary areas of research activity are two fold: first, studing thermonuclear (X-ray) bursts from accreting neutron stars; and second, searches for optical counterparts of gravitational-wave