Titlebook: Numerical Modelling of Astrophysical Turbulence; Wolfram Schmidt Book 2014 The Author(s) 2014 Astrophysical Turbulence.Astrophysical Turbu

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d structure. The metallic edge or surface states are immune to weak disorder or impurities, and robust against the deformation of the system geometry. This book, the first of its kind on topological insulators, presents a unified description of topological insulators from one to three dimensions bas

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Wolfram Schmidtthe modified Dirac equation.A starting point to enter the ne.Topological insulators are insulating in the bulk, but process metallic states present around its boundary owing to the topological origin of the band structure. The metallic edge or surface states are immune to weak disorder or impurities

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Wolfram Schmidtlations resulting in strongly predictive quantitative resultRing polymers are one of the last big mysteries in polymer physics, and this thesis tackles the problem of describing their behaviour when interacting in dense solutions and with complex environments and reports key findings that help shed

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Wolfram Schmidtthen this duality can be established by associating to a s- plex its dual block in the barycentric subdivision. In a manifold, the dual block is a cell, so the chain complex based on the dual blocks computes the homology of the manifold. Poincaré duality then serves as a cornerstone of manifold clas

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then this duality can be established by associating to a s- plex its dual block in the barycentric subdivision. In a manifold, the dual block is a cell, so the chain complex based on the dual blocks computes the homology of the manifold. Poincaré duality then serves as a cornerstone of manifold clas

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CBC471

Turbulent Velocity Statistics, coefficients are calibrated. The resulting SGS model is applied in explicit large eddy simulations (LES) to investigate the dependence of the energy fraction below a given length scale (the grid resolution), which not only verifies the consistency of the model, but can be regarded as an alternative