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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
116
Indicateur d'Open Access
85 %
Evolution des dépôts
mots clés
Low-Mach correction
Data parallelism
Linear systems
HII regions
CUDA
Brown dwarfs
Planets and satellites interiors
Hydrodynamics
Methods numerical
Dynamic processes
Convection
Big data
Energy
Detection-techniques
Stars formation
Planets and satellites composition
Boosting
Epidemic
Sparse matrix
Turbulence
Interferometers-planets and satellites
Parallel computing
Water
Planets and satellites formation
Ensemble learning
Geometric multigrid
65Y05
High angular resolution
Complex and heterogeneous dynamic system
HPC
Shallow water equations
Laser
Approximate Riemann solver
Iterative methods
Infrared planetary systems
Large time steps
Calcul haute performance
Godunov-type scheme
Insider threat
Ghost Fluid method
Domain decomposition
FFT
Sharp interface
ISM molecules
Exascale
High performance computing
Planets and satellites atmospheres
Techniques spectroscopic
Well-balanced property
Accretion disks
Astrophysics - Earth and Planetary Astrophysics
Two-phase flows
Magnetohydrodynamics
Planets and satellites gaseous planets
Efficiency
Big data analysis
Solvation
OpenMP
Radiative transfer
Low Froude
Stars massive
Gravitational effects
Methods data analysis
Conservation laws
ISM kinematics and dynamics
Gas dynamics
Plasma physics
Cybersecurity
Planets and satellites fundamental parameters
Bagging
Adaptive optics-instrumentation
Unite and conquer
Schrödinger equation
Hyperbolic systems
Unite and Conquer
Methods statistical
Supercapacitors
Astrophysics - Astrophysics of Galaxies
Astrometry
Accretion
Linear algebra
Dask
ISM individual objects Orion B
Low Mach correction
High Performance Computing
AMITEXFFTP
Surface tension
Astrochemistry
Instrumentation
Aerodynamics
Asynchronous communication
GPU computing
Level-Set
MPI
Astrophysics - Solar and Stellar Astrophysics
Electron
Supernovae general
Compressible two-phase flow
ISM clouds
ISM structure