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of mesons and baryons and their role as indirect probes for physics beyond the standard model. I also follow searches for new physics at the large hadron collider (LHC) and use them to constrain new particles
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regime, tidal disruption events, kilonovae and gamma ray burst afterglows. Some examples include: What do the spins of merging black holes tell us about binary evolution? Where are low-mass X-ray binaries
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will have the opportunity to interact with gravitational-wave researchers throughout Australia and around the world. Students in my group use data from the Laser Interferometer Gravitational-wave
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in conventional imaging, and to access a complementary ‘dark-field’ signal that originates from tiny sample structures. We do this by designing and implementing novel experimental set-ups and
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resonance, spin-Hamiltonians and time-dependent perturbations. Our experiments require hand-on experimental use of optics (e.g. lasers, detectors, lenses, etc.), microwave, RF and DC electronics, magnetic
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. "Studying the origin of the new discovered class of weak CN stars in the Magellanic Clouds using stellar variability" "How do stars merge? Studying the merger between low and intermediate-mass main-sequence
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, comprehensible and explainable machine learning explore the use of near-time data from healthcare providers to update these models over time.
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Bachelor of Applied Data Science Advanced (Honours) Ruby I'm more flexible and reassured about my financial situation with a scholarship. It has also given me the opportunity to participate in the Access