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Titlebook: High Performance Computing in Science and Engineering ’03; Transactions of the Egon Krause,Willi Jäger,Michael Resch Conference proceeding

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Water on Marss Odyssey ([1], [2], [4]). These gamma rays are supposed to be produced during inelastic collision and/or capture of secondary neutrons which were produced in the soil by cosmic rays. The signals are indicative of the presence of a large amount (at least 35 wt %) of hydrogen below a dry layer in thi
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Formation and Propagation of Jets Around Compact Objectsblack holes in microquasar or black hole X-ray binaries (BHXBs), around young stellar objects, but also around stellar compact sources as white dwarfs in symbiotic stars and neutron stars in low mass X-ray binaries (LMXBs). In interacting binaries containing compact objects, the secondary — a main-s
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Crack Propagation in Icosahedral Model Quasicrystalstomically sharp crack and subsequently loaded by linear scaling of the displacement field. The response of the system is then monitored during the simulation. In particular, the crack surface morphology is investigated in dependence of the orientation of the fracture plane. For this purpose, fractur
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Gas-Phase Epitaxy Grown InP(001) Surfaces From Real-Space Finite-Difference Calculationsproperties of P-rich InP(001)(2x1) surfaces grown in gas-phase epitaxy. These surfaces have been reported to consist of a semiconducting monolayer of buckled phosphorus dimers. This apparent violation of the electron counting principle was explained by effects of strong electron correlation. Our cal
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