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