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