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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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. 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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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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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
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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 Jobbnorge. It is therefore
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circuit-level simulation, system modeling, and in-silicon hardware prototyping to evaluate approaches against performance metrics such as energy efficiency, inference accuracy and computational latency
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join our team at the forefront of the field. You will work with observational and simulated data, with the balance between the two adaptable to your skills and affinities. You will also contribute