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