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an approach based on 3D imaging and numerical simulation. The objective is to support the development of the most "infiltrable" ex-PIP matrices by characterizing the spatial organization of these porous media
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Job related to staff position within a Research Infrastructure? No Offer Description Development of theoretical models of cell migration with memory Modeling in statistical physics and soft matter
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understanding its internal structure. Interpreting these geophysical data to model planetary structure and dynamics depends on understanding the physical properties of materials under relevant pressure and
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of very-high-energy gamma-ray sources, in the context of study of magnetic fields in the Milky Way galaxy and in the intergalactic medium. The work will include development of numerical code for modelling
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able to perform both analytical and numerical calculations. Experience with analytical or numerical modelling of active systems is desired. Experience with continuum/ hydrodynamic theories
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. ISTerre is part of the Observatory of Universe Sciences (OSU) at Grenoble Alpes University (UGA), which is responsible for numerous national observation services. This work will be carried out under
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planetary geodynamics and habitability. Experience using piston cylinder and DAC presses, high-temperature and high-pressure experiments, numerical modeling, Zr isotopes, atomic-scale and micro-scale analyses
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deformation behaviors. This will be supported by numerical simulations developed by the LEM where nanoindentation simulations at the atomic scale will be performed by Molecular Dynamic (MD) as well as finite
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extended complexes) The application to various models of MHD and flows in porous media The numerical analysis of the schemes The development of the computational kernel of the NEMESIS software library
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such as Euclid poses many modeling challenges. The COLIBRI ERC aims precisely to develop new theoretical and numerical tools to overcome one of these challenges: baryon modeling. The CDD will have two