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