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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.
Dépôts récents
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Sara Moukir, Miwako Tsuji, Nahid Emad, Mitsuhisa Sato, Stephane Baudelocq. Advancements in traffic simulations with multiMATSim’s distributed framework. ICAART 2024 - the 16th International Conference on Agents and Artificial Intelligence, Feb 2024, rome, Italy. pp.374-385, ⟨10.5220/0012452600003636⟩. ⟨hal-04496277⟩
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Sara Moukir, Nahid Emad, Stéphane Baudelocq. A high performance algorithmic variant of MATSim road traffic simulator. IPDPSW 2023 - IEEE International Parallel and Distributed Processing Symposium Workshops, May 2023, St petersburg, United States. pp.914-922, ⟨10.1109/IPDPSW59300.2023.00149⟩. ⟨hal-04496008⟩
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Thomas Padioleau, Pascal Tremblin, Edouard Audit, Pierre Kestener, Samuel Kokh. A High-performance and Portable All-Mach Regime Flow Solver Code with Well-balanced Gravity. Application to Compressible Convection. The Astrophysical Journal, 2019, 875 (2), pp.128. ⟨10.3847/1538-4357/ab0f2c⟩. ⟨cea-04381512⟩
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Sohvi Luukkonen, Luc Belloni, Daniel Borgis, Maximilien Levesque. Predicting hydration free energies of the freesolv database of drug-like molecules with molecular density functional theory. Journal of Chemical Information and Modeling, 2020, 60 (7), pp.3558-3565. ⟨10.1021/acs.jcim.0c00526⟩. ⟨cea-02909000⟩
Pour toute question : hal@cea.fr
Nombre de documents
Nombre de notices
Indicateur d'Open Access
85 %
Evolution des dépôts
mots clés
MPI
Gas dynamics
OpenMP
Insider threat
Well-balanced property
CUDA
Turbulence
Schrödinger equation
Cybersecurity
Infrared planetary systems
High performance computing
Brown dwarfs
Complex and heterogeneous dynamic system
Astrometry
Ghost Fluid method
FFT
Radiative transfer
Big data analysis
Methods data analysis
Compressible two-phase flow
Gravitational effects
Interferometers-planets and satellites
ISM molecules
Low Mach correction
Electron
Astrophysics - Solar and Stellar Astrophysics
Linear algebra
Solvation
Ensemble learning
Geometric multigrid
Energy
High angular resolution
Astrophysics - Earth and Planetary Astrophysics
Asynchronous communication
Surface tension
Planets and satellites atmospheres
Data parallelism
Methods numerical
Planets and satellites formation
Dask
65Y05
Level-Set
Convection
Domain decomposition
Water
Accretion
Astrophysics - Astrophysics of Galaxies
Low Froude
Parallel computing
Dynamic processes
Methods statistical
Boosting
Planets and satellites gaseous planets
Shallow water equations
Two-phase flows
Magnetohydrodynamics
Sharp interface
Planets and satellites fundamental parameters
Supernovae general
Stars massive
Unite and Conquer
Accretion disks
Laser
Exascale
Instrumentation
Sparse matrix
ISM individual objects Orion B
Epidemic
Plasma physics
Supercapacitors
ISM structure
Big data
Efficiency
Large time steps
Adaptive optics-instrumentation
Planets and satellites composition
Detection-techniques
HPC
Conservation laws
Hydrodynamics
AMITEXFFTP
Hyperbolic systems
Low-Mach correction
Planets and satellites interiors
HII regions
High Performance Computing
Aerodynamics
Bagging
Godunov-type scheme
ISM clouds
Techniques spectroscopic
Linear systems
ISM kinematics and dynamics
Astrochemistry
Calcul haute performance
Unite and conquer
Approximate Riemann solver
Stars formation
GPU computing
Iterative methods