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