France Atomization Methods numerical Galaxies interactions Luminescence Spectroscopy Stars formation Deep Learning Large-Eddy Simulation COVID-19 Hydrodynamics Direct numerical simulation Molecular Dynamics Molecular dynamics simulations Copper Instabilities Calcul parallèle Data assimilation Transition to turbulence Radiative transfer DFT calculations Galaxies high-redshift Climate change Aeroacoustics Neural networks Diffusion Numerical simulations Segmentation Electronic structure MPI Galaxies formation Cosmology theory Astrophysics - Astrophysics of Galaxies Ligands Modeling Direct Numerical Simulation DNS HPC Numerical simulation Density functional theory Magnetohydrodynamics MHD Modélisation Numerical modelling Quantum chemistry Density Functional Theory Adsorption Accretion 3D Combustion Large-scale structure of Universe Simulation numérique Two-phase flow Large-eddy simulation Machine learning Ab initio calculations Molecular dynamics Protoplanetary disks Computational seismology Dynamo theories and simulations DFT Deep learning Inverse theory LES Galaxies evolution Cancer Calcul haute performance Solar wind Parallel computing Large Eddy Simulation Computational fluid dynamics Machine Learning Hydrogen Dynamo Self-supervised learning Science ouverte Apprentissage profond Optimization Supernovae general Density functional calculations Ab initio Turbulence Astrochemistry Wave propagation Graphene CFD Open access Modelling Dynamique moléculaire High performance computing Heat transfer Large eddy simulation Catalysis Nanoparticles Computer vision MHD Données de la recherche Accretion disks Convection Open science Simulation