88 research outputs found
Lane reduction in driven 2d-colloidal systems through microchannels
The transport behavior of a system of gravitationally driven colloidal
particles is investigated. The particle interactions are determined by the
superparamagnetic behavior of the particles. They can thus be arranged in a
crystalline order by application of an external magnetic field. Therefore the
motion of the particles through a narrow channel occurs in well-defined lanes.
The arrangement of the particles is perturbed by diffusion and the motion
induced by gravity. Due to these combined influences a density gradient forms
along the direction of motion of the particles. A reconfiguration of the
crystal is observed leading to a reduction of the number of lanes. In the
course of the lane reduction transition a local melting of the
quasi-crystalline phase to a disordered phase and a subsequent crystallization
along the motion of the particles is observed. This transition is characterized
experimentally and using Brownian dynamics (BD) simulations.Comment: 4 pages, 4 figure
Irreversible Deposition of Line Segment Mixtures on a Square Lattice: Monte Carlo Study
We have studied kinetics of random sequential adsorption of mixtures on a
square lattice using Monte Carlo method. Mixtures of linear short segments and
long segments were deposited with the probability and , respectively.
For fixed lengths of each segment in the mixture, the jamming limits decrease
when increases. The jamming limits of mixtures always are greater than
those of the pure short- or long-segment deposition.
For fixed and fixed length of the short segments, the jamming limits have
a maximum when the length of the long segment increases. We conjectured a
kinetic equation for the jamming coverage based on the data fitting.Comment: 7 pages, latex, 5 postscript figure
Magnetic buoyancy in simulated galactic discs with a realistic circum galactic medium
We present simulations of isolated disc galaxies in a realistic environment
performed with the Tree-SPMHD-Code Gadget-3. Our simulations include a
spherical circum-galactic medium (CGM) surrounding the galactic disc, motivated
by observations and the results of cosmological simulations. We present three
galactic models with different halo masses between 10e10 Msol and 10e12 Msol,
and for each we use two different approaches to seed the magnetic field, as
well as a control simulation without a magnetic field. We find that the
amplification of the magnetic field in the centre of the disc leads to a
biconical magnetic outflow of gas that magnetizes the CGM. This biconical
magnetic outflow reduces the star formation rate (SFR) of the galaxy by roughly
40 percent compared to the simulations without magnetic fields. As the key
aspect of our simulations, we find that small scale turbulent motion of the gas
in the disc leads to the amplification of the magnetic field up to tens of
10e-6 G, as long as the magnetic field strength is low. For stronger magnetic
fields turbulent motion does not lead to significant amplification but is
replaced by an alpha-omega dynamo. The occurance of a small scale turbulent
dynamo becomes apparent through the magnetic power spectrum and analysis of the
field lines' curvature. In accordance with recent observations we find an
anti-correlation between the spiral structure in the gas density and in the
magnetic field due to a diffusion term added to the induction equation.Comment: 22 pages, 16 figures, submitted to MNRA
Thermal conductance of metallic atomic-size contacts: Phonon transport and Wiedemann-Franz law
Motivated by recent experiments [Science 355, 6330 (2017); Nat. Nanotechnol.
12, 430 (2017)], we present here an extensive theoretical analysis of the
thermal conductance of atomic-size contacts made of three different metals,
namely gold (Au), platinum (Pt) and aluminum (Al)
Kinetic Roughening in Deposition with Suppressed Screening
Models of irreversible surface deposition of k-mers on a linear lattice, with
screening suppressed by disallowing overhangs blocking large gaps, are studied
by extensive Monte Carlo simulations of the temporal and size dependence of the
growing interface width. Despite earlier finding that for such models the
deposit density tends to increase away from the substrate, our numerical
results place them clearly within the standard KPZ universality class.Comment: nine pages, plain TeX (4 figures not included
Molecular dynamics study of the thermopower of Ag, Au, and Pt nanocontacts
Using molecular dynamics simulations of many junction stretching processes we
analyze the thermopower of silver (Ag), gold (Au), and platinum (Pt) atomic
contacts. In all cases we observe that the thermopower vanishes on average
within the standard deviation and that its fluctuations increase for decreasing
minimum cross-section of the junctions. However, we find a suppression of the
fluctuations of the thermopower for the s-valent metals Ag and Au, when the
conductance originates from a single, perfectly transmitting channel. Essential
features of the experimental results for Au, Ag, and copper (Cu) of Ludoph and
van Ruitenbeek [Phys. Rev. B 59, 12290 (1999)], as yet unaddressed by atomistic
studies, can hence be explained by considering the atomic and electronic
structure at the disordered narrowest constriction of the contacts. For the
multivalent metal Pt our calculations predict the fluctuations of the
thermopower to be larger by one order of magnitude as compared to Ag and Au,
and suppressions of the fluctuations as a function of the conductance are
absent.Comment: 13 pages, 10 figure
Morphology of Fine-Particle Monolayers Deposited on Nanopatterned Substrates
We study the effect of the presence of a regular substrate pattern on the
irreversible adsorption of nanosized and colloid particles. Deposition of disks
of radius is considered, with the allowed regions for their center
attachment at the planar surface consisting of square cells arranged in a
square lattice pattern. We study the jammed state properties of a generalized
version of the random sequential adsorption model for different values of the
cell size, , and cell-cell separation, . The model shows a surprisingly
rich behavior in the space of the two dimensionless parameters
and . Extensive Monte Carlo simulations for system sizes of
square lattice unit cells were performed by utilizing an
efficient algorithm, to characterize the jammed state morphology.Comment: 11 pages, 10 figures, 3 table
Nonlocal elastic compliance for soft solids: theory, simulations, and experiments
The nonlocal elastic response function is crucial for understanding many properties of soft solids. This may be obtained by measuring strain-strain autocorrelation functions. We use computer simulations as well as video microscopy data of superparamagnetic colloids to obtain these correlations for two-dimensional triangular solids. Elastic constants and elastic correlation lengths are extracted by analyzing the correlation functions. We show that to explain our observations displacement fluctuations in a soft solid need to contain affine (strain) as well as nonaffine components
Coarse-graining microscopic strains in a harmonic, two-dimensional solid and its implications for elasticity: non-local susceptibilities and non-affine noise
In soft matter systems the local displacement field can be accessed directly
by video microscopy enabling one to compute local strain fields and hence the
elastic moduli using a coarse-graining procedure. We study this process for a
simple triangular lattice of particles connected by harmonic springs in
two-dimensions. Coarse-graining local strains obtained from particle
configurations in a Monte Carlo simulation generates non-trivial, non-local
strain correlations (susceptibilities), which may be understood within a
generalized, Landau type elastic Hamiltonian containing up to quartic terms in
strain gradients (K. Franzrahe et al., Phys. Rev. E 78, 026106 (2008)). In
order to demonstrate the versatility of the analysis of these correlations and
to make our calculations directly relevant for experiments on colloidal solids,
we systematically study various parameters such as the choice of statistical
ensemble, presence of external pressure and boundary conditions. We show that
special care needs to be taken for an accurate application of our results to
actual experiments, where the analyzed area is embedded within a larger system,
to which it is mechanically coupled. Apart from the smooth, affine strain
fields, the coarse-graining procedure also gives rise to a noise field made up
of non-affine displacements. Several properties of this noise field may be
rationalized for the harmonic solid using a simple "cell model" calculation.
Furthermore the scaling behavior of the probability distribution of the noise
field is studied and a master curve is obtained.Comment: 16 pages, 12 figure
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