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Titlebook: High Performance Computing in Science and Engineering, Garching/Munich 2007; Transactions of the Siegfried Wagner,Matthias Steinmetz,Matth

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书目名称High Performance Computing in Science and Engineering, Garching/Munich 2007
副标题Transactions of the
编辑Siegfried Wagner,Matthias Steinmetz,Matthias Brehm
视频video
概述Includes supplementary material:
图书封面Titlebook: High Performance Computing in Science and Engineering, Garching/Munich 2007; Transactions of the  Siegfried Wagner,Matthias Steinmetz,Matth
描述For the fourth time, the Leibniz Supercomputing Centre (LRZ) and the Com- tence Network for Technical, Scienti c High Performance Computing in Bavaria (KONWIHR) publishes the results from scienti c projects conducted on the c- puter systems HLRB I and II (High Performance Computer in Bavaria). This book reports the research carried out on the HLRB systems within the last three years and compiles the proceedings of the Third Joint HLRB and KONWIHR Result and Reviewing Workshop (3rd and 4th December 2007) in Garching. In 2000, HLRB I was the rst system in Europe that was capable of performing more than one Tera op/s or one billion oating point operations per second. In 2006 it was replaced by HLRB II. After a substantial upgrade it now achieves a peak performance of more than 62 Tera op/s. To install and operate this powerful system, LRZ had to move to its new facilities in Garching. However, the situation regarding the need for more computation cycles has not changed much since 2000. The demand for higher performance is still present, a trend that is likely to continue for the foreseeable future. Other resources like memory and disk space are currently in suf cient abundance on this
出版日期Conference proceedings 2009
关键词Hochleistungsrechnen; algorithms; astrophysics; computational fluid dynamics; computational physics; high
版次1
doihttps://doi.org/10.1007/978-3-540-69182-2
isbn_softcover978-3-642-08868-1
isbn_ebook978-3-540-69182-2
copyrightSpringer-Verlag Berlin Heidelberg 2009
The information of publication is updating

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Elizabeth M. Lupton,Irmgard Frank“first wave” of studies on heuristic use (Kahneman, Slovic, & Tversky, 1982). Most of this research, however, employed laboratory simulations, using college undergraduates to make judgments about fictional people and events.
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Star Formation in the Turbulent Interstellar Medium and Its Implications on Galaxy Evolutione are described by a subgrid scale model. Implementing FEARLESS into the open source AMR code Enzo, we successfully tested the new method both in hydrodynamic and self-gravitating turbulence simulations. In the next phase of the project, FEARLESS will be applied to star formation and galactic disk simulations.
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Numerical Simulations of Compact Binary Systems of our simulations. We also report on the physical results extracted from these simulations. These concern black-hole physics in general as well as the use of our numerically generated waveforms in the ongoing effort to detect gravitational waves.
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Oxidative Dehydrogenation of Simple Molecules over RuO2(110): Density Functional Theory Calculationsf NH. oxidation the desorption of NO is the rate-determining step of the reaction, due to the high adsorption energy of NO. The oxidation of HCl is characterized by gradual chlorination of the top-most layer of the surface of the catalyst.
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