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