High Performance Computing in Science and Engineering ´16: by Wolfgang E. Nagel, Dietmar H. Kröner, Michael M. Resch

By Wolfgang E. Nagel, Dietmar H. Kröner, Michael M. Resch

This e-book offers the cutting-edge in supercomputer simulation. It comprises the newest findings from best researchers utilizing structures from the excessive functionality Computing middle Stuttgart (HLRS) in 2016. The reviews conceal all fields of computational technology and engineering starting from CFD to computational physics and from chemistry to machine technological know-how with a unique emphasis on industrially suitable purposes. proposing findings of 1 of Europe’s prime structures, this quantity covers a large choice of purposes that bring a excessive point of sustained performance.

The publication covers the most equipment in high-performance computing. Its impressive leads to attaining the simplest functionality for creation codes are of specific curiosity for either scientists and engineers. The ebook comes with a wealth of colour illustrations and tables of results.

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Extra resources for High Performance Computing in Science and Engineering ´16: Transactions of the High Performance Computing Center, Stuttgart (HLRS) 2016

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1 Introduction Our research efforts continue to focus on the development of computational methods to solve the Schrödinger and Dirac equations for atomic and molecular collision processes. Access to leadership-class computers such as the Cray XC40 at HLRS allows us to benchmark our theoretical solutions against dedicated collision experiments at synchrotron facilities such as the Advanced Light Source (ALS), Astrid II, BESSY II, SOLEIL and PETRA III and to provide atomic and molecular data for ongoing research in laboratory and astrophysical plasma science.

Furthermore, its abundance is expected to be enhanced in x-ray dominated regions (XDR) [58]. In their model of the Orion Bar PDR, Nagy et al. 4 % of the total destruction rate of SHC , since reactive collisions with H and dissociative recombination by electrons are more efficient. However, they adopted the estimated cross section of [55] for v 00 D 0, J 00 D 0. We point out that the adoption of the current cross sections would enhance the photodissociation contribution to greater than 10 %. We note that the photodissociation rates are not given here as they are sensitive to the local radiation field and dust properties.

Absolute state-slected measurements of the photoionization cross section of N C and OC ions. Astrophys. J. Suppl. Ser. 138, 219 (2002) 13. : K-shell photoabsorption of oxygen ions. Astrophys. J. Suppl. Ser. 158, 68 (2005) 14. : Wavelength measurements of K transitions of oxygen, neon, and magnesium with X-ray absorption lines. Astrophys. J. 774, 116 (2013) 15. : Interstellar medium composition through X-ray spectroscopy of low-mass X-ray binaries. Astron. Astrophys. 551, 25 (2013) 16. : K-shell photoionization of B-like (O3C ) oxygen ions: experiment and theory.

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