30 coding-"https:"-"FEMTO-ST"-"CSIC"-"L2CM"-"Inserm"-"RAEGE-Az" "https:" Postdoctoral positions at CNRS
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modeling - Coalescent modeling - Coding - Tests with simulations - Data analyses - Paper writing - Presenting results -Integration within the BioDiv team at IBENS - Availability of work station, computer
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(M/F) will work within the LUPM. The research fellow (M/F) recruited will be eligible for training and support when taking up their duties. Where to apply Website https://emploi.cnrs.fr/Candidat/Offre
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; apply the developed methodology to complex heterostructures The postdoctoral researcher will be recruited within the Chemical Theory and Modelling team (http://www.quanthic.org ) of the Institute
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the AliceVision library. Activity 3: Critical Code Optimization (C++/CUDA) - Adapt the code to drastically reduce computation times (target: < 1h). - Replace proprietary dependencies (InstantNGP) with a flexible
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deep neural activity, using methods that combine physics (waves in complex media) and computational approaches. Where to apply Website https://emploi.cnrs.fr/Candidat/Offre/UMR8552-SYLGIG-011
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Interatomic Potentials) code for ternary compounds with variable composition with crystal structure optimization algorithms (evolutionary, random, etc.); - Application of the CSP DFT/MLIP methodology to various
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Two-year postdoc position (M/F) in signal processing and Monte Carlo methods applied to epidemiology
, easy to handle codes to make available the proposed methodologies to nonspecialists. He/she will work in contact with epidemiologists and will be provided real epidemiological data. An interest in
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to the main plasma physics conferences. Where to apply Website https://emploi.cnrs.fr/Candidat/Offre/UMR7345-YANCAM-002/Candidater.aspx Requirements Research FieldPhysicsEducation LevelPhD or equivalent
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twenty years have required the development of more generic codes capable of accounting for certain specificities such as continuous fuel recycling or the modeling of effects associated with the migration
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= 30) and high-resolution (R = 100,000) spectra of exoplanets using precomputed grids of models. The code can estimate global properties (effective temperature, pressure–temperature profiles) as