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