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of advanced ab-initio computational methods for modeling electronic and magnetic properties of low-dimensional systems; - documented organizational activities (supervision of students and PhD candidates
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-body contributions. Tasks: Independent scientific collaboration on the above-mentioned project Data analysis and interpretation, numerical modeling, and preparation of scientific publications
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trips, plus an elective course. Examples of elective courses could include aqueous geochemistry, geomorphology, soils, glaciology, GIS, or numerical modeling. We are seeking candidates who can demonstrate
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. Advanced knowledge of the ISO standards and the CMMI (Compatibility Maturity Model Integration) model. Thorough knowledge of other areas of IT. Thorough knowledge of department and University processes and
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staff position within a Research Infrastructure? No Offer Description Numerical simulations of community dynamics: 1. Simulation of the dynamics of a local community of two species in the presence of time
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at the start of your appointment. You have already conducted research within the field of numerical modelling of wind in your master thesis. You have preferentially have experience with CFD tools using URANS
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University of North Carolina at Chapel Hill | Chapel Hill, North Carolina | United States | about 23 hours ago
opportunities for career growth, skill development and lifelong learning and enjoy exclusive perks for numerous retail, restaurant and performing arts discounts, savings on local child care centers and special
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sustainable resources, smart and resilient cyber-infrastructure, and data science and numerical modeling. This research advances technology and innovation and offers students hands-on opportunities to address
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trips, plus an elective course. Examples of elective courses could include aqueous geochemistry, geomorphology, soils, glaciology, GIS, or numerical modeling. We are seeking candidates who can demonstrate
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Statistics. The UCD Relativity group invites applications for an ERC-funded Research Scientist position in gravitational-wave source modelling, with a focus on small mass-ratio binaries and second-order