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