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