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

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nti 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 proc

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Miroslav Mocák,Ewald Müllercertain matrices which can be understood as the skew symmetric counterpart of the corresponding Gramians. Based on this representation we calculate the .th Clifford power . of a vector . ∈ .. which enables the extension of an analytical function . : . → . to their corresponding Clifford function .:.. → ..(.).

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Modeling of Turbulent Flows Applied to?Numerical Simulations of Galaxy Clusterslso affect the level of turbulence in the cluster core, according to the first results of our cosmological simulations. Especially in the latter problem, a significant improvement in the modeling is expected from the use of the full . implementation.

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Redox Catalysis and Reactivity of?Metalloporphyrinesations with Fe, Co and Ni show two-state reactivity, while those with Cu and Zn proceed on a single potential energy surface. For metalation with Zn, we calculated a barrier of the first hydrogen transfer step of 32.6?kcal?mol., in a good agreement with the overall experimental activation energy of 31?kcal?mol..

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Formation of the First Supermassive Black Holes in the Early Universe contributions at the temperatures found in our simulation. Understanding black hole formation in the early universe will help to predict the evolution of the black hole population and lead to more accurate predictions for the gravitational wave interferometer LISA.