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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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is also a Principal Investigator at the Hylleraas Centre for Quantum Molecular Science, a Norwegian Centre of Excellence dedicated to the development and application of advanced computer simulations
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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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electrical characterization methods, material growth, device fabrication and simulations. The student will also be affiliated with the newly formed Centre for Defects in Semiconductors for Quantum Sensing
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with it the solar physics group at the University of Oslo, is known world-wide for its expertise in numerical simulations and observations of the solar atmosphere and thus offers an attractive work
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struggle to keep up. Legacy rule-based compliance systems, long the cornerstone of anti-money laundering (AML) efforts, are increasingly ineffective – often generating overwhelming false-positive alerts
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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 working with