Plenarvorträge - DPG-Tagungen
Plenarvorträge - DPG-Tagungen
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.