The effects of adiabatic dust grain
charge fluctuation and inhomogeneity on the nonlinear properties of dust acoustic (DA) solitary waves are studied. The plasma under consideration is a hot magnetized dusty plasma consisting of negatively charged dust particles, Boltzmann ions, and nonextensive electrons. A modified Zakharov-Kusnetsov equation, which admits a solitary wave solution, is derived using the reductive perturbation theory. It is found that the charge fluctuation of the dust grain modifies the nature of DA solitary structures. The numerical results may be useful to understand phenomena in laboratory and astrophysical plasmas.
The properties of decaying turbulence have been studied with the help of a Generalized Hydrodynamic (GHD) fluid model in the context of strongly coupled dusty plasma medium in two dimensions. The GHD model treats the strongly coupled dusty plasma system as a visco-elastic medium. The incompressible limit of the GHD model is considered here. The studies carried out here are, however, applicable to a wider class of visco-elastic systems, and are not merely confined to the dusty plasma medium. Our simulations studies show that an initial spectrum that is confined in a limited domain of wave numbers becomes broad, even when the Reynold's number is much less than the critical value required for the onset of turbulence in Newtonian fluids. This is a signature of elastic turbulence, where Weissenberg's number also plays an important role on the onset of turbulence. This feature has been observed in several experiments. It is also shown that the existence of memory relaxation time parameter and the transverse shear wave inhibit the normal process (for 2-D systems) of inverse spectral cascade in this case. A detailed simulation study has been carried out for the understanding of this inhibition.
Author(s): Sergey A. Khrapak and Hubertus M. Thomas
Simple practical expressions that allow estimation of thermodynamic properties of Yukawa fluids in a wide range of coupling, up to the fluid-solid phase transition, are presented. These expressions demonstrate excellent agreement with the available results from numerical simulations. The approach pr...
[Phys. Rev. E 91, 023108] Published Wed Feb 25, 2015
It is demonstrated explicitly that the scattering of electromagnetic waves by dust structures can be strongly enhanced as compared to incoherent scattering by random electrons. If the size of the dust structure is much less than the wavelength of the incident radiation, the scattering is coherent. In this case, the scattering is proportional to the square of the total number of electrons in the structure. In the opposite limit, the scattering is incoherent being proportional to the total number of electrons in the structure. The factor describing the degree of coherency is calculated numerically for several models of self-organized structures. It is demonstrated in general way that for sudden heating of electrons, the factor of coherency in scattering by structures can decrease by several orders of magnitude with subsequent increase after the heating is switched off. In laboratory dusty plasmas, the coherent scattering is proposed for diagnostics of universal structuring instability and as a probe for determining the properties typical for self-organized nature of structures that are observed in recent experiments.
An ion beam propagating through a magnetized dusty plasma drives Kelvin Helmholtz Instability (KHI) via Cerenkov interaction. The frequency of the unstable wave increases with the relative density of negatively charged dust grains. It is observed that the beam has stabilizing effect on the growth rate of KHI for low shear parameter, but for high shear parameter, the instability is destabilized with relative density of negatively charged dust grains.
The nonthermal and geometric effects on the propagation of the surface dust acoustic waves are investigated in a Lorentzian dusty plasma slab. The symmetric and anti-symmetric dispersion modes of the dust acoustic waves are obtained by the plasma
dielectric function with the spectral reflection conditions the slab geometry. The variation of the nonthermal and geometric effects on the symmetric and the anti-symmetric modes of the surface plasma waves is also discussed.
Langmuir probe measurements in dusty plasmas is a challenge because particle and film deposition on
the probe leads to contamination and distortion of the current–voltage characteristics. This problem
is particularly acute while determining the electron energy probability function (EEPF) from the
second derivative of the Langmuir probe current–voltage characteristics. Here, we present reliable
EEPF measurements in a capacitively coupled argon–silane dusty plasma using a fast-scanning and
shielded Langmuir probe. A solenoid-actuated shield covered the probe and the probe was exposed to
the plasma only for short periods of time (less than 6 s) when the current–voltage characteristics
were recorded during rapid voltage scans. This approach minimized probe surface contamination. In
presence of dust (silicon nanoparticles) the electron density decreased and the electron temperature
increased in comparison to a pristine argon plasma. While the population of lower energy electrons
Transport properties of dense liquid helium under the conditions of planet's
core and cool atmosphere of white dwarfs have been investigated by using the
improved centroid path-integral simulations combined with density functional
theory. The self-diffusion is largely higher and the shear viscosity is notably
lower predicted with the quantum mechanical description of the nuclear motion
compared with the description by Newton equation. The results show that nuclear
quantum effects (NQEs), which depends on the temperature and density of the
matter via the thermal de Broglie wavelength and the ionization of electrons,
are essential for the transport properties of dense liquid helium at certain
astrophysical conditions. The Stokes-Einstein relation between diffusion and
viscosity in strongly coupled regime is also examined to display the influences
Simple practical expressions are put forward, which allow to estimate
thermodynamic properties of Yukawa fluids in a wide range of coupling, up to
the fluid-solid phase transition. These expressions demonstrate excellent
agreement with the available results from numerical simulations. The approach
provides simple and accurate tool to estimate thermodynamic properties of
Yukawa fluids and related systems in a broad range of parameters.
Author(s): Damien D. Brewer and Satish Kumar
The fast lubrication dynamics method is applied to simulate the motion and deposition of charge-stabilized 100-nm-diam particles into sediment films from aqueous dispersions. Colloidal interactions are incorporated with a Yukawa potential and the effects of the screened-Coulomb potential strength an...
[Phys. Rev. E 91, 022304] Published Fri Feb 13, 2015