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, non-invasive device to monitor dehydration in a clinical and non-clinical setting. The aim of this project is to pursue research and development in a sensor system for continuous monitoring
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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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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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possess translational symmetry, the role of structure and symmetry in glasses is not established. This research programme involves the development of new x-ray and electron diffraction-based methods
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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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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
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beach rocks, a bio-inspired cementation technology will be developed. A novel bio-sintering process is proposed through successive dissolution and remineralization of limestone utilizing the microbes
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and assessment of CVI in children with cerebral palsy. Objectives 1. Develop protocol for screening for CVI in young children with cerebral palsy 2. Evaluate the efficacy of CVI assessments in
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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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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