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I supervise a wide range of projects in stellar astrophysics, with a focus on low and intermediate-mass stars, which have masses similar to or slightly larger than our Sun. This work is carried out
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of neutron stars); stellar rotation of misaligned systems (internal rotation evolution, binary and multiple stars dynamics and interaction). Please feel free to come by my office or drop me an email if you
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University as the new Head of School of Physics and Astronomy. In addition to my research at Monash, I hold the Lee-Lucas Chair in Experimental Physics at Imperial College London. Our research work is highly
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I am interested in all aspects of theoretical astrophysics, with a particular focus on strong gravitational fields, compact objects, and gravitational-wave astronomy. I am currently exploring the evolution of massive binary stars into compact binaries as sources of gravitational-waves and...
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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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), 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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? What is the origin of potassium in globular clusters? Is thermohaline mixing the mechanism that determines abundances of red giants? "Thermohaline mixing in red giants" "Carbon production in the Galaxy
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Conventional x-ray imaging is firmly established as an invaluable tool in medicine, security, research and manufacturing. However, conventional methods extract only a fraction of the sample
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dissipation along the edges of the material. It is hoped that these sorts of materials will one day replace conventional silicon based electronics. This work is carried out within the Centre of Excellence
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the detailed interaction between matter and light in the extreme conditions of stellar interiors is still poorly understood. Despite this, stars remain the ideal laboratories to understand how galaxies form