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