Download High Performance Computing in Science and Engineering '09: by Volker Gaibler, Max Camenzind (auth.), Wolfgang E. Nagel, PDF
By Volker Gaibler, Max Camenzind (auth.), Wolfgang E. Nagel, Dietmar B. Kröner, Michael M. Resch (eds.)
Aus den Rezensionen: “Obwohl auch aus finanziellen Gründen eigentlich auf einen engen Kreis von Forschern beschränkt, ist die Simulation mit Supercomputern bzw. deren Resultate kaum mehr aus unserem Alltag wegzudenken - Stichwort numerische Wettervorhersage. ... Ein wissenschaftliches Buch, das den aktuellen Stand des vielfältigen Einsatzes von Supercomputing in Deutschland präsentiert.“ (in: Bulletin SEV/VSE, February/2010, S. 87)
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The abstracts and papers during this quantity have been provided on the 5th Annual overseas Computing and Combinatorics convention (COCOON ’99), which used to be held in Tokyo, Japan from July 26 to twenty-eight, 1999. the themes conceal so much facets of theoretical laptop technological know-how and combinatorics bearing on computing.
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Extra info for High Performance Computing in Science and Engineering '09: Transactions of the High Performance Computing Center, Stuttgart (HLRS) 2009
Example text
Future Generation Computer Systems, 15:485–495, 1999. 46. J. F. Richardson and W. N. Zaki. Sedimentation and fluidisation: Part 1. Trans. Instn. Chem. , 32:35–53, 1954. 47. S. Richter and G. Huber. Resonant column experiments with fine-grained model material - evidence of particle surface forces. Granular Matter, 5:121–128, 2003. 48. M. Ripoll, K. Mussawisade, R. G. Winkler, and G. Gompper. Low-Reynoldsnumber hydrodynamics of complex fluids by multi-particle-collision dynamics. Europhys. , 68:106–112, 2004.
Astron. Astrophys. 457 (2006) 281–308 25. : Delayed Neutrino-Driven Supernova Explosions Aided by the Standing Accretion-Shock Instability. Astrophys. J. 694 (2009) 664–696 26. : Explosions of O–Ne–Mg cores, the Crab supernova, and subluminous type II–P supernovae. Astron. Astrophys. 450 (2006) 345–350 32 B. M¨ uller, A. -Th. Janka 27. : Toward Gravitational Wave Signals from Realistic Core-Collapse Supernova Models. Astrophys. J. 603 (2004) 221–230 28. : Equation-of-state dependent features in shock-oscillation modulated neutrino and gravitational-wave signals from supernovae.
17, 19, 21]. For the simulation of a fluid solvent, many different simulation methods have been proposed: direct Navier Stokes solvers [28, 29, 52, 61], Stokesian Dynamics (SD) [4, 5, 44], Accelerated Stokesian Dynamics (ASD) [55, 56], pair drag simulations [31], Brownian Dynamics (BD) [22, 23], Lattice Boltzmann (LB) [30, 32–34], and Stochastic Rotation Dynamics (SRD) [21, 27, 42]. These mesoscopic fluid simulation methods have in common that they impose certain approximations to reduce the computational effort.