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