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