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