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, strength and geological equations of state, to simulate hypothesized giant impacts, and especially, to establish their systemwide consequences and corollaries. For example, a giant impact on Venus would have
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computational predictions with experimental validation. At the computational stage, the candidate will establish molecular docking and molecular dynamics simulation workflows to predict receptor–ligand
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. The long-standing solar convective conundrum is the mismatch between convective flows inferred from helioseismology and flows predicted by state-of-the-art simulations. ReCon² addresses this by advancing
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stellar tidal streams) around disk galaxies. The successful candidate will design, perform and analyse idealized and cosmological hydrodynamical galaxy formation simulations, develop or improve models
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trained to work on both galaxy clustering and weak gravitational lensing, using N-body simulations to simulate structure formation and connecting the simulations to observables. The candidate will also be
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associated with research group of Professor Abhik Ghosh (https://en.uit.no/project/softmatter ). The Ghosh group is renowned for its fundamental discoveries on corroles and is currently exploring a variety of
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for offshore engineering, ship design, and coastal safety, but their occurrence is highly uncertain due to natural variability in wave conditions. Computational tools for simulating waves and quantifying
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be responsible for developing, automating and optimizing data acquisition and analysis workflows for experimental datasets. The candidate will work on the following tasks: Simulation and modeling
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tomography, with numerical simulations informed by microstructural data. The successful candidate will work at the interface between experiments, modelling, and data-driven methods. Particular emphasis will be
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living in Norway can be found here: https://uit.no/staffmobility Application Please note that the application will only be assessed based on the information submitted by the application deadline via