room 1.40, Pasteura 5 at 09:30

Krzysztof Mizerski (IGF PAN)
It is well known that a field of random waves in a fluid of non-zero resistivity is capable of exciting a large-scale magnetic field through creation of an electromotive force (EMF) which leads to exponential growth of magnetic energy until the growing Lorentz force reacts back upon the wave field, leading to a saturated state. For highly conducting plasma it is generally found that kinematic fast-dynamos with finite growth rate in the limit of vanishing resistivity, have a pathological structure, non-differentiable wherever they are non-zero; the applicability of fast-dynamo theory to natural physical systems is then questionable.
Here we relax the standard simplifying assumptions of stationarity and homogeneity of the background turbulence and introduce new fast-dynamo mechanisms, fully dynamic, that is incorporating the back reaction of the Lorentz force on the flow (hitherto scarcely considered), for which the growing magnetic field remains smooth during the whole dynamo process. This results from a random superposition of waves, perturbed by the magnetic field. Particularly effective are the interactions of ‘beating’ waves (close-frequency waves) and nonlinear effects in the mean electromotive force leading to very fast amplification of the mean magnetic field. The renormalization approach is udertaken to obtain final mean-field equations and saturation of the large-scale field.
The theory has the potential to be applied to the dynamo generation of magnetic fields in the ionised gas of the early universe, both before and during the process of galaxy formation. In such a plasma, the resistivity is extremely low, giving characteristic diffusion times many orders of magnitude greater than the age of the entire universe and hence negligible. Nevertheless the large-scale galactic magnetic fields and fields of galaxy clusters are observed, thus non-resistive dynamo mechanisms are strongly desirable in this context.
It is well known that a field of random waves in a fluid of non-zero resistivity is capable of exciting a large-scale magnetic field through creation of an electromotive force (EMF) which leads to exponential growth of magnetic energy until the growing Lorentz force reacts back upon the wave field, leading to a saturated state. For highly conducting plasma it is generally found that kinematic fast-dynamos with finite growth rate in the limit of vanishing resistivity, have a pathological structure, non-differentiable wherever they are non-zero; the applicability of fast-dynamo theory to natural physical systems is then questionable.
Here we relax the standard simplifying assumptions of stationarity and homogeneity of the background turbulence and introduce new fast-dynamo mechanisms, fully dynamic, that is incorporating the back reaction of the Lorentz force on the flow (hitherto scarcely considered), for which the growing magnetic field remains smooth during the whole dynamo process. This results from a random superposition of waves, perturbed by the magnetic field. Particularly effective are the interactions of ‘beating’ waves (close-frequency waves) and nonlinear effects in the mean electromotive force leading to very fast amplification of the mean magnetic field. The renormalization approach is udertaken to obtain final mean-field equations and saturation of the large-scale field.
The theory has the potential to be applied to the dynamo generation of magnetic fields in the ionised gas of the early universe, both before and during the process of galaxy formation. In such a plasma, the resistivity is extremely low, giving characteristic diffusion times many orders of magnitude greater than the age of the entire universe and hence negligible. Nevertheless the large-scale galactic magnetic fields and fields of galaxy clusters are observed, thus non-resistive dynamo mechanisms are strongly desirable in this context. room 1.40, Pasteura 5 at 09:30

Paweł Żuk (IPPT PAN)
Two oppositely charged surfaces separated by a dielectric medium attract each other. In contrast, using the Surface Force Apparatus, we observe a strong repulsion between two plates of a capacitor that is filled with an aqueous electrolyte upon application of an alternating potential difference between the plates. This long-range force is observed on the distances two orders of magnitude larger than Debye length, the typical length scale for the extension of electrostatic effects. It increases with the ratio of diffusion coefficients of the ions in the medium and reaches steady state after a few minutes, which is much larger than the millisecond time scale of diffusion across the narrow gap. The repulsive force is an order of magnitude stronger than the electrostatic attraction observed in the same setup in air. We find that it results from the increase in osmotic pressure as a consequence of the field-induced excess of cations and anions due to lateral transport from adjacent reservoirs. Oppositely to what is observed with DC fields the ion concentration is elevated across the whole narrow gap instead of in the double layer region only. The unexpected distribution of ions in the thin electrolyte film under AC voltage points to the new design principles for fine control of local ionic concentration.
room 1.40, Pasteura 5 at 09:30

Paweł Sznajder (IPPT PAN)
In this short talk I will present the problem of diverging expressions for velocity fluctuations in a stationary state of uniform sedimenting suspension. Those divergencies, as suggested by Koch and Shaqfeh, can be eliminated by plasma like screening conditions for correlation functions. Unfortunately BBGKY hierarchy for that system derived by Cichocki and Sadlej can not have solutions which obey those conditions.