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" New Horizons of Computational Science : "
edited by T. Ebisuzaki, J. Makino.
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BL
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774246
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b594240
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edited by T. Ebisuzaki, J. Makino.
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New Horizons of Computational Science : : Proceedings of the International Symposium on Supercomputing held in Tokyo, Japan, September 1-3, 1997\ edited by T. Ebisuzaki, J. Makino.
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| Publication Statement
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Dordrecht : Springer Netherlands, 2001
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| Series Statement
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Astrophysics and Space Science Library, 263
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(XX, 312 Seiten)
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| ISBN
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0792370503
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: 9401008647
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: 9401038481
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: 9780792370505
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: 9789401008648
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: 9789401038485
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| Notes
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The International Symposium on Supercomputing - New Horizon of Computational Science was held on September 1-3, 1997 at the Science MuseuminTokyo, tocelebrate60-yearbirthdayofProfessorDaiichiroSug imoto, who hasbeenleadingtheoreticalandnumericalastrophysicsfor 30 years. The conference coveredexceptionally wide range ofsubjects, to follow Sugimoto'saccomplishmentsinmanyfields. Onthefirstdaywehadthree talksonstellarevolutionandsixtalksonstellardynamics. Onthesecond day, six talks on special-purpose computingand four talks on large-scale computing in MolecularDynamicswere given. Onthethirdandthelast day, threetalks on dedicatedcomputerson LatticeQCDcalculationsand sixtalksonpresentandfutureofgeneral-purposeHPCsystemsweregiven. Inaddition, some30posterswerepresentedonvarioussubjectsincompu tationalscience. Instellarevolution, D. Arnett (Univ.Of Tokyo) the 100-Tflops GRAPE-type machine for MD calculations, whichwillbefinished by 1999.OfArizona) gaveanexcellenttalk on the recent development in three-dimensionalsimulation ofSupernova, inparticularonquantitativecomparisonbetweendifferenttechniquessuch asgrid-basedmethodsandSPH (SmoothedParticleHydrodynamics). Y. Kondo (NASA) discussedresentadvanceinthemodelingoftheevolution ofbinarystars, and1. Hachisu(Univ. ofTokyo)discussedRayleigh-Taylor instabilitiesinsupernovae(contributionnotincluded). Instellardynamics, P. Hut(lAS)gaveasuperbreviewonthelong-term evolution ofstellarsystem, J. Makino (Univ. ofTokyo) described briefly theresultsobtainedonGRAPE-4special-purposecomputerandthefollow up project, GRAPE-6,whichisapprovedas ofJune 1997. GRAPE-6will be completed by year 2001 with the peak speed around 200 Tflops. R. Spurzem (Rechen-Inst.) and D. Heggie (Univ. of Edinburgh) talked on recentadvanceinthestudyofstarclusters, andE. Athanassoula(Marseille Observatory) describedthe work doneusingtheirGRAPE-3 systems. S. Ida (TokyoInst.OfTechnology) describedthe result ofthe simulationof theformationofMoon. Thefirst talkoftheseconddaywas given by F-H. Hsu oftheIBMT. J. Watson Research center, on "Deep Blue", the special-purpose computer for Chess, which, forthefirst timeinthehistory, wonthematchwiththe besthumanplayer, Mr. GaryKasparov(unfortunately, Hsu'scontribution isnot included in this volume). Then A. Bakker of Delft Inst. of Tech nology looked back his 20 years ofdevelopingspecial-purpose computers formoleculardynamicsandsimulationofspinsystems. J. Arnoldgavean overviewoftheemergingnewfieldofreconfigurablecomputing, whichfalls inbetweentraditionalgeneral-purposecomputersandspecial-purposecom puters. S. Okumura(NAO)describedthehistoryofultra-high-performance digital signalprocessors for radio astronomy. They havebuilt a machine with 20GaPS performance in early 80s, and keep improvingthe speed. M. Taiji (ISM) told on general aspects of GRAPE-type systems, and T. Narumi (Univ.
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| Contents
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Preface; T. Ebisuzaki, J. Makino. List of Participants. Stellar Evolution, Stellor Dynamics and Tera-Flops Computation; D. Sugimoto. Simulation of Nature by Computer; D. Arnett. Supercomputing and Evolution in Close Binaries; Y. Kondo. Stellar Dynamics of Dense Stellar Systems; P. Hut. Stellar Dynamics on 200 Tflops Special-Purpose Computers; J. Makino. Astrophysical N-Body Simulations: Algorithms and Challenges; R. Spurzem. Star Cluster Simulations; D.C. Heggie. Stellar Dynamical Simulations of Galaxies and of Galaxy System Using the Marselle Grape-3 Systems; E. Athanassoula. Accretion of Planets and Moons; S. Ida. What We Learned from Special Purpose Computers; A.F. Bakker, F. Berwald. Reconfigurable Computing; J.M. Arnold. Special-Purpose Computer for Radio Astronomy; S.K. Okumura. Special-Purpose Computers for Classical Particle Simulations; M. Taiji. Molecular Dynamics Machine: Highly Parallelized Special-Purpose-Computer for Molecular Dynamics Simulations; T. Narumi, et al. Molecular Simulations with the MD-Grape Special-Purpose Computer; M.J. Field. High Performance Computing in Biophysics: Recent Experiences and Developments of Charmm; M. Hodoscek, et al. Massive Parallelism: The Hardware for Computational Chemistry? M.F. Guest, et al. Molecular Dynamics Simulation of Ion Channels; Q. Zhong, et al. The QCDSP Computer: Particle Physics with 20,000 Processors; R.D. Mawhinney. The CP-PACS Project and Lattice QCD; Y. Iwasaki. Three Generations of APE Projects: Lessons and Perspective; R. Tripiccione. Vector-Parallel Processing and Fujitsu VPP300E/700E Supercomputer System; K. Miura. The Evolution of Rotating Collisional Stellar Systems; C.R.W. Einsel. Effects of the Alfven Wave on the GravitationalInstability in the Interstellar Medium; N. Fukuda, T. Hanawa. N-Body Simulation of Halo Formation Using GRAPE-4; T. Fukushige, J. Makino. The PCI Interface for Grape Systems: PCI-HIB; A. Kawai, et al. Fragmentation of Molecular Clouds: The Initial Phase of a Stellar Cluster; R.S. Klessen, A. Burkert. Formation of Star Clusters in the Magellanic Clouds; M. Kontizas, et al. Three Dimensional MHD Simulations of Accretion Disks and Jet Formation; R. Matsumoto, et al. Gravitational Collapse of Rotating Clouds: Bar Formation in a Self-Similarly Contracting Disk; T. Matsumoto, T. Hanawa. The Formation and Evolution of Dwarf Galaxies: Hydrodynamics and Color Gradient; M. Mori, et al. Parallel 3D Lattice Boltzmann Simulations of Turbulent Dark Cloud Flows; D. Muders. Photoionization of a Clumpy Universe; T. Nakamoto, et al. Smoothed Particle Hybrodynamics with Parallel Virtual Machine; N. Nakasato, et al. Jets from Time-Dependent Accretion Flows onto a Black Hole; K. Nobuta, T. Hanawa. Supercomputing in the Astronomical Institute of Romanian Academy; M.D. Suran, N.A. Popescu. Anisotropic Fokker-Planck Models of Globular Cluster Evolution; K. Takahashi. An Efficient Parallel Hierarchical Algorithm for Module Placement; T. Yang. The Efficient Parallel Newton-GMRES Algorithm for Computational Fluid Dynamics; T. Yang. Molecular Mechanism of Homogeneous Nucleation in Vapor Phase: Lennard-Jones Fluid; K. Yasuoka, M. Matsumoto. Development of Special Purpose Computer for Cosmic Hydrodynamics with SPH Method; Y. Yokono, et al. Index.
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Astrophysics and Astroparticles.
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Atomic, Molecular, Optical and Plasma Physics.
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Biochemistry.
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| LC Classification
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QB462.2E358 2001
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| Added Entry
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J Makino
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T Ebisuzaki
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| Parallel Title
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Proceedings of the International Symposium on Supercomputing held in Tokyo, Japan, September 1-3, 1997
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