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Plenarvorträge - DPG-Tagungen

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Dynamik und Statistische Physik Montag<br />

amounts of liquid. We used the electrowetting effect in order to manipulate<br />

liquid droplets. The droplets were placed either on top of a single<br />

substrate with a stripe electrode, or between two substrates with stripe<br />

electrodes on each side. We studied systematically the behaviour of<br />

the liquid as a function of the applied voltage, the substrate separation,<br />

and the relative orientation of opposed stripe electrodes. The experimental<br />

results are compared to both a simple analytical model as well as<br />

numerical calculations using the Surface Evolver.<br />

DY 17.3 Mo 17:00 H3<br />

Statistische Eigenschaften eines Punktwirbelmodells für die<br />

zweidimensionale Turbulenz — •Oliver Kamps und Rudolf<br />

Friedrich — Institut für Theoretische Physik der Universität Münster,<br />

Wilhelm-Klemm-Strasse 9, 48149 Münster<br />

Ausgehend von einer Punktwirbelbeschreibung einer getriebenen zweidimensionalen<br />

Strömung werden statistische Eigenschaften der Lagrangeschen<br />

Flüssigkeitsdynamik numerisch untersucht. Im Zentrum des Interesses<br />

stehen die Lagrangeschen Wahrscheinlichkeitsverteilungen für Ort<br />

und Geschwindigkeit<br />

DY 17.4 Mo 17:15 H3<br />

Thermal noise in thin liquid films — •Markus Rauscher 1,2 ,<br />

Klaus Mecke 1,2 , and Günther Grün 1,2 — 1 Max-Planck-Institut für<br />

Metallforschung, Stuttgart — 2 ITAP, Universität Stuttgart<br />

Thermal noise becomes more and more important the smaller a system<br />

is. Recent studies of thin film evolution indicate that thermal noise<br />

might influence characteristic time-scales of film dewetting [J. Becker et<br />

at., Nature Materials Vol. 2, 59 (2003)]. Up to now, thin film flow was<br />

only studied with deterministic equations.<br />

We develop a stochastic version of the thin film equation. In the thin<br />

film approximation, the stochastic incompressible hydrodynamic equations<br />

[Landau and Lifshitz, Vol. IV] reduce to the deterministic thin film<br />

equation plus a conserved noise term. We show that the noise term is<br />

consistent with the thermodynamical equilibrium distribution of the film<br />

thickness.<br />

DY 17.5 Mo 17:30 H3<br />

Adsorption of an asymmetric binary mixture at a selective solid<br />

wall — •Dirk Woywod, Jörg Silbermann, and Martin Schoen<br />

— Stranski-Laboratorium für Physikalische und Theoretische Chemie<br />

TU Berlin<br />

Sekretariat TC 7<br />

Strasse des 17.Juni 124<br />

10623 Berlin<br />

DY 20 Fractals and Nonlinearity I<br />

We consider a binary (A-B) mixture fluid near a selective planar homogenous<br />

wall. Using a lattice-gas model and mean-field approximation<br />

to the intrinsic free-energy functional, we obtain a closed expression for<br />

the potential density in the grand canonical ensemble (V, T, µA = µB).<br />

This expression depends on the attraction strength of the fluid-fluid interactions<br />

(ǫAA > ǫBB, ǫAB), the fluid-wall interactions (ǫAW < ǫBW), and<br />

the local densities (ρA, ρB). Minimizing the potential density numerically<br />

gives us access to complete phase diagrams including wetting films [1].<br />

In this presentation, we choose bulk parameters in order to promote the<br />

formation of demixed A-rich liquid phases near coexistence with a gas<br />

phase. Introducing a preference of the wall for molecules of component B,<br />

first-order phase transitions between adsorbed mixed, A-rich and B-rich<br />

films are observed. Besides multiple surface critical points, we also find<br />

a peculiar temperature dependence of the concentration of component B<br />

within a B-rich mixed film.[2]<br />

[1] D. Woywod, M. Schoen, Phys. Rev. E 67, 026122 (2003)<br />

[2] J. Silbermann, D. Woywod, M. Schoen, Phys. Rev E, in press (2003)<br />

DY 17.6 Mo 17:45 H3<br />

Microscopic theory for interfaces of binary liquid mixtures —<br />

•Thorsten Hiester 1,2 and Klaus Mecke 1,2 — 1 Max-Planck-Institut<br />

für Metallforschung, Heisenbergstraße 3, 70569 Stuttgart — 2 Institut<br />

für Theoretische und Angewandte Physik, Pfaffenwaldring 57, 70569<br />

Stuttgart<br />

Binary liquid interfaces, in particular, their nanoscopic structure is still<br />

poorly understood. In addition to capillary waves and density fluctuations<br />

there are simultaneously fluctuations of the composition. Beginning<br />

with a density functional theory for binary mixtures of inhomogeneous<br />

fluids we derive an effective Hamiltonian for interfaces of binary liquid<br />

mixtures beyond the well-known capillary-wave model. Explicit expressions<br />

for the surface tension, the bending ridigities and especially the coupling<br />

constants of compositional capillary waves in terms of two number<br />

densities are obtained. Finally, we make predictions for grazing-incidence<br />

x-ray scattering experiments.<br />

Zeit: Dienstag 09:30–11:15 Raum: H2<br />

Hauptvortrag DY 20.1 Di 09:30 H2<br />

Statistical Physics for Complex Cosmic Structures — •Luciano<br />

Pietronero — Dipartimento di Fisica, Universita’ di Roma La<br />

Sapienza, 00185 - Roma, Italy<br />

The amount of data in the field of astrophysics is growing exponentially<br />

since a few years and it will grow even more in the future. This<br />

situation is producing a dramatic change in which many speculations and<br />

conjectures can finally be tested. This large amount of data permits the<br />

detailed application of concepts from modern statistical physics. For the<br />

galaxy distribution these led to a new general perspective and, in particular,<br />

we presented strong evidence for self-similar and fractal structures<br />

extending to the limits of the data. This led to a large debate in the<br />

field which is nicely described in the recent book: “Discovery of Cosmic<br />

Fractals” by Y. Baryshev and P. Tirikorpi (World Scientific, 2002)<br />

http://www.wspc.com/books/popsci/4896.html. Recently we have extended<br />

the applications of these methods also to the Cosmic Microwave<br />

Background Radiation (which is very smooth) and to the N-body simularions<br />

(which should link the two properties). We provide an overview<br />

of the general situation of a field which represents an ideal playground of<br />

interdisciplinary research between astrophysics and statistical physics.<br />

DY 20.2 Di 10:00 H2<br />

Generalization of Oboukhov’s Model for the Description of<br />

Turbulent Lagrangian Statistics — •Rafaela Hillerbrand and<br />

Rudolph Friedrich — Wilhelm-Klemm-Str. 9, 48149 Münster<br />

Within the Langrangian framework for the description of fluid flows<br />

a model for the stochastic evolution of a particle in a turbulent flow is<br />

introduced. As a fractional Fokker-Planck equation the considered model<br />

takes into account longtime correlations. In this model the Lagrangian<br />

probability distribution function can be stated as an integral transform<br />

of the solution of an ordinary Fokker-Planck equation, where the kernel<br />

of the transformation contains the one-sided Lévy distribution. This<br />

relates the stochastic behavior of a Lagrangian particle to the class of<br />

continuous time random walks.<br />

DY 20.3 Di 10:15 H2<br />

Theoretical and experimental study of feedback-mediated drift<br />

of spiral waves — •Vladimir Zykov and Harald Engel — Technische<br />

Universitaet Berlin, Institut fuer Theoretische Physik, Sekr. PN<br />

7-1, Hardenbergstr. 36, D-10623 Berlin<br />

An efficient method is proposed to determine a velocity field describing<br />

feedback induced drift of spiral waves. This method can be applied to<br />

quite different feedback mechanisms as, for example, the one-channel and<br />

the global feedback. It is shown that a smooth variation of eccentricity of<br />

an elliptical domain subjected to the global feedback induces a cascade<br />

of bifurcations that can drastically change the spiral wave evolution. In<br />

a square shaped domain a set of point attractors appears instead of the<br />

circular resonance attractor typical for a circular domain. These predictions<br />

are in good quantitative agreement with performed numerical integrations<br />

of an excitable reaction-diffusion system and with experimental<br />

data obtained for the light-sensitive Belousov-Zhabotinsky reaction.

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