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New Horizons of Computational Science, Softcover reprint of the original 1st ed. 2001 Proceedings of the International Symposium on Supercomputing held in Tokyo, Japan, September 1—3, 1997 Astrophysics and Space Science Library Series, Vol. 263

Langue : Anglais

Coordonnateurs : Ebisuzaki Toshikazu, Makino Junichiro

Couverture de l’ouvrage New Horizons of Computational Science
Proceedings of the International Symposium on Supercomputing held in Tokyo, Japan, September 1-3, 1997
Stellar Evolution, Stellar Dynamics and Tera-Flops Computation.- Simulation of Nature by Computer.- Supercomputing and Evolution in Close Binaries.- Stellar Dynamics of Dense Stellar Systems.- Stellar Dynamics on 200 Tflops Special-Purpose Computers.- Astrophysical N-Body Simulations: Algorithms and Challenges.- Star Cluster Simulations.- Stellar Dynamical Simulations of Galaxies and of Galaxy Systems Using the Marseille Grape-3 Systems.- Accretion of Planets and Moons.- What We Learned from Special Purpose Computers.- Reconfigurable Computing.- Special-Purpose Computer for Radio Astronomy.- Special-Purpose Computers for Classical Particle Simulations.- Molecular Dynamics Machine: Highly Parallelized Special-Purpose-Computer for Molecular Dynamics Simulations.- Molecular Simulations with the MD-Grape Special-Purpose Computer.- High Performance Computing in Biophysics: Recent Experiences and Developments of Charmm.- Massive Parallelism: The Hardware for Computational Chemistry?.- Molecular Dynamics Simulation of Ion Channels.- The QCDSP Computer: Particle Physics with 20,000 Processors.- The CP-PACS Project and Lattice QCD.- Three Generations of APE Projects: Lessons and Perspective.- Vector-Parallel Processing and Fujitsu VPP300E/700E Supercomputer System.- The Evolution of Rotating Collisional Stellar Systems.- Effects of the Alfvén Wave on the Gravitational Instability in the Interstellar Medium.- N-Body Simulation of Halo Formation Using GRAPE-4.- The PCI Interface for Grape Systems: PCI-HIB.- Fragmentation of Molecular Clouds: The Initial Phase of a Stellar Cluster.- Formation of Star Clusters in the Magellanic Clouds.- Three Dimensional MHD Simulations of Accretion Disks and Jet Formation.- Gravitational Collapse of Rotating Clouds: Bar Formation in aSelf-Similarly Contracting Disk.- The Formation and Evolution of Dwarf Galaxies: Hydrodynamics and Color Gradient.- Parallel 3D Lattice Boltzmann Simulations of Turbulent Dark Cloud Flows.- Photoionization of a Clumpy Universe.- Smoothed Particle Hydrodynamics with Parallel Virtual Machine.- Jets from Time-Dependent Accretion Flows onto a Black Hole.- Supercomputing in the Astronomical Institute of Romanian Academy.- Anisotropic Fokker-Planck Models of Globular Cluster Evolution.- An Efficient Parallel Hierarchical Algorithm for Module Placement.- The Efficient Parallel Newton-GMRES Algorithm for Computational Fluid Dynamics.- Molecular Mechanism of Homogeneous Nucleation in Vapor Phase: Lennard-Jones Fluid.- Development of Special Purpose Computer for Cosmic Hydrodynamics with SPH Method.

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Ouvrage de 312 p.

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Date de parution :

Ouvrage de 312 p.

15.5x23.5 cm

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210,99 €

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