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