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