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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
275
Nombre de notices
117
Indicateur d'Open Access
85 %
Evolution des dépôts
mots clés
ISM clouds
Sparse matrix
Convection
65Y05
MPI
Hyperbolic systems
High Performance Computing
Radiative transfer
Level-Set
Big data analysis
Methods statistical
Low Froude
Large time steps
Accretion disks
Ghost Fluid method
Sharp interface
Schrödinger equation
CUDA
Exascale
Water
Methods numerical
Gravitational effects
Supercapacitors
Insider threat
Planets and satellites gaseous planets
Iterative methods
Techniques spectroscopic
Geometric multigrid
GPU computing
Dask
Bagging
Accretion
Dynamic processes
Godunov-type scheme
Well-balanced property
Unite and conquer
High angular resolution
Parallel computing
Complex and heterogeneous dynamic system
Linear algebra
Surface tension
Stars massive
Efficiency
Adaptive optics-instrumentation
AMITEXFFTP
Methods data analysis
Brown dwarfs
Solvation
Unite and Conquer
OpenMP
Gas dynamics
Planets and satellites fundamental parameters
Electron
Ensemble learning
Low Mach correction
Interferometers-planets and satellites
Planets and satellites composition
Stars formation
Instrumentation
Hydrodynamics
HPC
Infrared planetary systems
Planets and satellites atmospheres
Shallow water equations
Astrophysics - Earth and Planetary Astrophysics
Turbulence
Compressible two-phase flow
Energy
ISM kinematics and dynamics
Magnetohydrodynamics
Low-Mach correction
Conservation laws
Astrophysics - Astrophysics of Galaxies
Calcul haute performance
Domain decomposition
Approximate Riemann solver
ISM structure
Data parallelism
HII regions
ISM individual objects Orion B
Astrochemistry
Planets and satellites formation
Planets and satellites interiors
High performance computing
Aerodynamics
Astrophysics - Solar and Stellar Astrophysics
Supernovae general
Epidemic
Plasma physics
Big data
Boosting
Linear systems
ISM molecules
FFT
Asynchronous communication
Cybersecurity
Laser
Two-phase flows
Detection-techniques
Astrometry