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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
118
Indicateur d'Open Access
85 %
Evolution des dépôts
mots clés
ISM individual objects Orion B
Turbulence
GPU computing
Epidemic
Godunov-type scheme
Astrochemistry
Electron
Methods data analysis
OpenMP
Convection
Hydrodynamics
Ensemble learning
Accretion disks
Low Froude
Accretion
Sharp interface
HII regions
High angular resolution
Stars formation
Parallel computing
Insider threat
Techniques spectroscopic
Level-Set
Planets and satellites fundamental parameters
Planets and satellites formation
Ghost Fluid method
Radiative transfer
Supercapacitors
High Performance Computing
Stars massive
Complex and heterogeneous dynamic system
Big data analysis
HPC
Linear algebra
Schrödinger equation
ISM molecules
Big data
Brown dwarfs
Plasma physics
CUDA
Dask
Unite and conquer
Data parallelism
Solvation
Detection-techniques
Magnetohydrodynamics
Planets and satellites composition
MPI
Adaptive optics-instrumentation
65Y05
Asynchronous communication
Approximate Riemann solver
Unite and Conquer
Large time steps
Energy
Astrophysics - Astrophysics of Galaxies
Compressible two-phase flow
High performance computing
Planets and satellites atmospheres
Exascale
Infrared planetary systems
ISM clouds
Surface tension
Interferometers-planets and satellites
Calcul haute performance
Gravitational effects
Iterative methods
Shallow water equations
Water
FFT
Astrophysics - Solar and Stellar Astrophysics
Boosting
ISM structure
ISM kinematics and dynamics
Instrumentation
Low-Mach correction
Cybersecurity
Planets and satellites interiors
Methods numerical
AMITEXFFTP
Hyperbolic systems
Linear systems
Astrometry
Well-balanced property
Astrophysics - Earth and Planetary Astrophysics
Sparse matrix
Compressible flows
Methods statistical
Supernovae general
Gas dynamics
Planets and satellites gaseous planets
Two-phase flows
Efficiency
Laser
Aerodynamics
Bagging
Geometric multigrid
Conservation laws
Domain decomposition
Dynamic processes