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technology, or a related field. You have a strong background in hydrodynamics and ship manoeuvring. You should also have a good understanding of control theory and optimization. Additional requirements
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Program since 2023 and provides a passionate, supportive and personalised approach to her work. Email Kapisha News https://cms.unimelb.edu.au/central-site-management/content-templates/news-listing/v4-assets
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hydrodynamics and/or N-body simulations in the star and planet formation context Experience in the field with HPC system usage and parallel/distributed computing Knowledge in GPU-based programming would be
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support system of senior scientists, supporting their work. Your primary responsibilities will include: Apply and adapt a high-resolution coupled hydrodynamic (GETM) - biogeochemical (ERGOM) model to assess
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Dynamics , Condensed Matter Theory , Cosmology , Crystallography , Dark Matter , Data analysis , EIC , Electron Hydrodynamics , electron-positron collisions , electron-proton collisions , Electronic Detector
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: Aerodynamics and hydrodynamics, Computational fluid dynamics (CFD), Compressible flows, Environmental fluid mechanics, Flow control and optimisation, Fluid-structure interaction, Wave energy, Wind energy
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improved stability, when exposed to SAC containing wastewater streams. Here e.g., hydrodynamic shear effects can be exploited, when response to stresses of these SAC-films at the interface is known
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Cornell community. Our group has broad interests in hard and soft condensed matter physics, including (but not limited to): biophysics, cold atom physics, electronic structure theory, hydrodynamics
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, Condensed Matter Theory , Cosmology , Dark Matter , Electron Hydrodynamics , electron-positron collisions , electron-proton collisions , Electronic Detector Group , Elementary Particle Physics , Elementary
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, accretion, stellar evolution and similar phenomena. Qualifications: A Ph.D. in Physics or Astronomy. Experience with hydrodynamical, stellar evolution, or radiation-transfer simulations. Benefits: Full