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Field
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, the concept of "slow sound" (reduced group velocity) can be naturally achieved through the propagation of shear waves in very soft media (hydrogels, complex fluid suspensions) or via acoustic metamaterials
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stellar interiors, birth properties of black holes and neutron stars, supernova light curves and spectra, gravitational waves, neutrino astrophysics, the production of heavy elements stellar explosions, and
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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
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charge transport, such protection of propagating fluctuations of the magnetization – dubbed spin waves or magnons – has recently been gaining attention. This PhD project will focus on using femtosecond
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structure dynamics including wave transmission and reflection, overtopping, mooring loading, and motion response across a range of realistic wave conditions. Numerical modelling using OpenFOAM and Delft3D
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ecosystems. Natural vegetated coastal habitats, by contrast, support high biodiversity, sequester carbon and attenuate waves, though may not fully protect coastal assets. This PhD project investigates
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of time-varying photonic metamaterials. First-principles mathematical modeling of optic-wave physics in canonical geometries under space-time-varying polarization responses. Computer programming and
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-reciprocity of spin waves Angular Momentum of Magnons Magnetically doped Transition Metal Dichalcogenide Thin Films via Molecular Beam Epitaxy Modeling of a magnonic diode based on spin-wave non-reciprocity in
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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
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), wave propagation modeling in complex 3D geometries, development and optimization of event detection algorithms, high-precision localization methods, event magnitude as well as source characterization