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