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Bienvenue sur la collection HAL de la Maison de la Simulation, laboratoire commun au CEA, au CNRS, à l'Université Paris-Saclay et à l'Université Versailles Saint-Quentin. Elle est spécialisée dans le calcul haute performance et les simulations numériques en lien étroit avec les applications physiques, le génie logiciel parallèle, les modèles de programmation, les techniques de visualisation, l'intelligence artificielle et l'informatique quantique.

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Pour toute question : hal@cea.fr

Nombre de documents

275

Nombre de notices

117

Indicateur d'Open Access

85 %

Evolution des dépôts

mots clés

Laser Low-Mach correction Hyperbolic systems Interferometers-planets and satellites Epidemic Cybersecurity Low Mach correction Methods numerical Hydrodynamics Well-balanced property Geometric multigrid Astrophysics - Earth and Planetary Astrophysics Brown dwarfs MPI CUDA Convection Dynamic processes Linear systems Instrumentation Calcul haute performance Sparse matrix Techniques spectroscopic ISM kinematics and dynamics Asynchronous communication Surface tension High performance computing Big data analysis Electron Level-Set Planets and satellites atmospheres Planets and satellites gaseous planets Astrophysics - Astrophysics of Galaxies Plasma physics Godunov-type scheme Boosting Astrophysics - Solar and Stellar Astrophysics Shallow water equations Stars formation Planets and satellites composition ISM molecules Water Supercapacitors Methods statistical High Performance Computing Sharp interface Insider threat Detection-techniques Turbulence Large time steps Energy Planets and satellites formation Accretion Low Froude Linear algebra Planets and satellites fundamental parameters Exascale Ghost Fluid method Data parallelism Stars massive Supernovae general Astrochemistry Aerodynamics Astrometry High angular resolution Complex and heterogeneous dynamic system Gas dynamics ISM clouds Iterative methods Magnetohydrodynamics OpenMP Accretion disks Radiative transfer ISM structure ISM individual objects Orion B Compressible two-phase flow Big data Methods data analysis Planets and satellites interiors Solvation Adaptive optics-instrumentation Gravitational effects HPC Conservation laws Two-phase flows HII regions Schrödinger equation Dask Parallel computing Approximate Riemann solver Bagging Unite and Conquer FFT GPU computing 65Y05 Ensemble learning Unite and conquer AMITEXFFTP Infrared planetary systems Efficiency Domain decomposition