137 research outputs found
Critical analysis of fragment-orbital DFT schemes for the calculation of electronic coupling values
We present a critical analysis of the popular fragment-orbital
density-functional theory (FO-DFT) scheme for the calculation of electronic
coupling values. We discuss the characteristics of different possible
formulations or 'flavors' of the scheme which differ by the number of electrons
in the calculation of the fragments and the construction of the Hamiltonian. In
addition to two previously described variants based on neutral fragments, we
present a third version taking a different route to the approximate diabatic
state by explicitly considering charged fragments. In applying these FO-DFT
flavors to the two molecular test sets HAB7 (electron transfer) and HAB11 (hole
transfer) we find that our new scheme gives improved electronic couplings for
HAB7 (-6.2% decrease in mean relative signed error) and greatly improved
electronic couplings for HAB11 (-15.3% decrease in mean relative signed error).
A systematic investigation of the influence of exact exchange on the electronic
coupling values shows that the use of hybrid functionals in FO-DFT calculations
improves the electronic couplings, giving values close to or even better than
more sophisticated constrained DFT calculations. Comparing the accuracy and
computational cost of each variant we devise simple rules to choose the best
possible flavor depending on the task. For accuracy, our new scheme with
charged-fragment calculations performs best, while numerically more efficient
at reasonable accuracy is the variant with neutral fragments
The small-scale dynamo: Breaking universality at high Mach numbers
(Abridged) The small-scale dynamo may play a substantial role in magnetizing
the Universe under a large range of conditions, including subsonic turbulence
at low Mach numbers, highly supersonic turbulence at high Mach numbers and a
large range of magnetic Prandtl numbers Pm, i.e. the ratio of kinetic viscosity
to magnetic resistivity. Low Mach numbers may in particular lead to the
well-known, incompressible Kolmogorov turbulence, while for high Mach numbers,
we are in the highly compressible regime, thus close to Burgers turbulence. In
this study, we explore whether in this large range of conditions, a universal
behavior can be expected. Our starting point are previous investigations in the
kinematic regime. Here, analytic studies based on the Kazantsev model have
shown that the behavior of the dynamo depends significantly on Pm and the type
of turbulence, and numerical simulations indicate a strong dependence of the
growth rate on the Mach number of the flow. Once the magnetic field saturates
on the current amplification scale, backreactions occur and the growth is
shifted to the next-larger scale. We employ a Fokker-Planck model to calculate
the magnetic field amplification during the non-linear regime, and find a
resulting power-law growth that depends on the type of turbulence invoked. For
Kolmogorov turbulence, we confirm previous results suggesting a linear growth
of magnetic energy. For more general turbulent spectra, where the turbulent
velocity v_t scales with the characteristic length scale as u_\ell\propto
\ell^{\vartheta}, we find that the magnetic energy grows as
(t/T_{ed})^{2\vartheta/(1-\vartheta)}, with t the time-coordinate and T_{ed}
the eddy-turnover time on the forcing scale of turbulence. For Burgers
turbulence, \vartheta=1/2, a quadratic rather than linear growth may thus be
expected, and a larger timescale until saturation is reached.Comment: 10 pages, 3 figures, 2 tables. Accepted at New Journal of Physics
(NJP
Idiosyncratic risk and the cost of capital - The case of electricity networks
We analyze the treatment and impact of idiosyncratic or firm-specific risk in regulation. Regulatory authorities regularly ignore firm-specific characteristics, such as size or asset ages, implying different risk exposure in incentive regulation. In contrast, it is common to apply only a single benchmark, the weighted average cost of capital (WACC), uniformly to all firms. This will lead to implicit discrimination. We combine models of firm-specific risk, liquidity management and regulatory rate setting to investigate impacts on capital costs. We focus on the example of the impact of component failures for electricity network operators. In a simulation model for Germany, we find that capital costs increase by approximately 0.2 to 3.0 percentage points depending on the size of the firm (in the range of 3% to 40% of total cost of capital). Regulation of monopolistic bottlenecks should take these risks into account to avoid implicit discrimination
Analysis of Heating Effects and Deformations for a STAF Panel with a Coupled CFD and FEM Simulation Method
Conventional sandwich panels are one of the cheapest and easiest solutions for forming the thermal building envelope of industrial buildings. They are pre-fabricated façade elements, of which millions of square metres have been produced and mounted every year. There is great potential to reduce the consumption of fossil fuels and CO2 emissions through the solar thermal activation of such a sandwich panel. In the course of the research project ABS-Network SIAT 125, a Solar Thermal Activated Façade (STAF) panel was designed which is to be optimised both thermally and structurally. This study shows a first version of a so-called ‘one way coupled’ thermal and structural analysis of a conventional sandwich panel compared to the STAF panel. For this purpose, the numerical methods of Computational Fluid Dynamics (CFD) and Finite Element Method (FEM) are used together in one simulation environment. Furthermore, results from an outdoor test facility are presented where a first version of a STAF panel is tested under real climate conditions. The CFD model was positively evaluated by comparing measured and computed temperatures
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