242 research outputs found
Pre-dewetting transition on a hydrophobic wall: Statics and dynamics
For one-component fluids, we predict a pre-dewetting phase transition between
a thin and thick low-density layer in liquid on a wall repelling the fluid.
This is the case of a hydrophobic wall for water. A pre-dewetting line starts
from the coexistence curve and ends at a surface critical point in the phase
diagram. We calculate this line numerically using the van der Waals model and
analytically using the free energy expansion up to the quartic order. We also
examine the pre-dewetting dynamics of a layer created on a hydrophobic spot on
a heterogeneous wall. It is from a thin to thick layer during decompression and
from a thick to thin layer during compression. Upon the transition, a liquid
region above the film is cooled for decompression and heated for compression
due to latent heat convection and a small pressure pulse is emitted from the
film into the liquid.Comment: 14 pages, 17 figure
Molecular Dynamics Study of the Nematic-Isotropic Interface
We present large-scale molecular dynamics simulations of a nematic-isotropic
interface in a system of repulsive ellipsoidal molecules, focusing in
particular on the capillary wave fluctuations of the interfacial position. The
interface anchors the nematic phase in a planar way, i.e., the director aligns
parallel to the interface. Capillary waves in the direction parallel and
perpendicular to the director are considered separately. We find that the
spectrum is anisotropic, the amplitudes of capillary waves being larger in the
direction perpendicular to the director. In the long wavelength limit, however,
the spectrum becomes isotropic and compares well with the predictions of a
simple capillary wave theory.Comment: to appear in Phys. Rev.
Surface layering of liquids: The role of surface tension
Recent measurements show that the free surfaces of liquid metals and alloys
are always layered, regardless of composition and surface tension; a result
supported by three decades of simulations and theory. Recent theoretical work
claims, however, that at low enough temperatures the free surfaces of all
liquids should become layered, unless preempted by bulk freezing. Using x-ray
reflectivity and diffuse scattering measurements we show that there is no
observable surface-induced layering in water at T=298 K, thus highlighting a
fundamental difference between dielectric and metallic liquids. The
implications of this result for the question in the title are discussed.Comment: 5 pages, 4 figures, to appear in Phys. Rev. B. 69 (2004
Acellular dermal matrix and coronally advanced flap or tunnel technique in the treatment of multiple adjacent gingival recessions. A 12-year follow-up from a randomized clinical trial
AimTo evaluate the long-term outcomes of Acellular Dermal Matrix (ADM) with Coronally Advanced Flap (CAF) or Tunnel technique (TUN) in the treatment of multiple adjacent gingival recessions (MAGRs).Material and methodsNineteen of the original 24 patients contributing to a total number of 33 sites for CAF and 34 for TUN were available for the 12 years follow-up examination. Recession depth, mean root coverage (mRC), keratinized tissue width (KTW), gingival thickness (GT) were evaluated and compared with baseline values and 6-months results. Regression analysis was performed to identify factors related to the stability of the gingival margin.ResultsA highly significant drop in mRC was observed for both groups from the 6 months timepoint to the 12 years recall (p  .05). KTW - 2 mm and GT - 1.2 mm at 6-months were two predictors for stability of the gingival margin (p = .03 and p = .01, respectively).ConclusionsA significant relapse of the gingival margin of MAGRs treated with CAF or TUN + ADM was observed after 12 years.Peer Reviewedhttps://deepblue.lib.umich.edu/bitstream/2027.42/151340/1/jcpe13163_am.pdfhttps://deepblue.lib.umich.edu/bitstream/2027.42/151340/2/jcpe13163.pd
Microscopic View on Short-Range Wetting at the Free Surface of the Binary Metallic Liquid Gallium-Bismuth: An X-ray Reflectivity and Square Gradient Theory Study
We present an x-ray reflectivity study of wetting at the free surface of the
binary liquid metal gallium-bismuth (Ga-Bi) in the region where the bulk phase
separates into Bi-rich and Ga-rich liquid phases. The measurements reveal the
evolution of the microscopic structure of wetting films of the Bi-rich,
low-surface-tension phase along different paths in the bulk phase diagram. A
balance between the surface potential preferring the Bi-rich phase and the
gravitational potential which favors the Ga-rich phase at the surface pins the
interface of the two demixed liquid metallic phases close to the free surface.
This enables us to resolve it on an Angstrom level and to apply a mean-field,
square gradient model extended by thermally activated capillary waves as
dominant thermal fluctuations. The sole free parameter of the gradient model,
i.e. the so-called influence parameter, , is determined from our
measurements. Relying on a calculation of the liquid/liquid interfacial tension
that makes it possible to distinguish between intrinsic and capillary wave
contributions to the interfacial structure we estimate that fluctuations affect
the observed short-range, complete wetting phenomena only marginally. A
critical wetting transition that should be sensitive to thermal fluctuations
seems to be absent in this binary metallic alloy.Comment: RevTex4, twocolumn, 15 pages, 10 figure
Instantaneous Liquid Interfaces
We describe and illustrate a simple procedure for identifying a liquid
interface from atomic coordinates. In particular, a coarse grained density
field is constructed, and the interface is defined as a constant density
surface for this coarse grained field. In applications to a molecular dynamics
simulation of liquid water, it is shown that this procedure provides
instructive and useful pictures of liquid-vapor interfaces and of
liquid-protein interfaces.Comment: 15 pages, 4 figure
Atomic X-ray Spectroscopy of Accreting Black Holes
Current astrophysical research suggests that the most persistently luminous
objects in the Universe are powered by the flow of matter through accretion
disks onto black holes. Accretion disk systems are observed to emit copious
radiation across the electromagnetic spectrum, each energy band providing
access to rather distinct regimes of physical conditions and geometric scale.
X-ray emission probes the innermost regions of the accretion disk, where
relativistic effects prevail. While this has been known for decades, it also
has been acknowledged that inferring physical conditions in the relativistic
regime from the behavior of the X-ray continuum is problematic and not
satisfactorily constraining. With the discovery in the 1990s of iron X-ray
lines bearing signatures of relativistic distortion came the hope that such
emission would more firmly constrain models of disk accretion near black holes,
as well as provide observational criteria by which to test general relativity
in the strong field limit. Here we provide an introduction to this phenomenon.
While the presentation is intended to be primarily tutorial in nature, we aim
also to acquaint the reader with trends in current research. To achieve these
ends, we present the basic applications of general relativity that pertain to
X-ray spectroscopic observations of black hole accretion disk systems, focusing
on the Schwarzschild and Kerr solutions to the Einstein field equations. To
this we add treatments of the fundamental concepts associated with the
theoretical and modeling aspects of accretion disks, as well as relevant topics
from observational and theoretical X-ray spectroscopy.Comment: 63 pages, 21 figures, Einstein Centennial Review Article, Canadian
Journal of Physics, in pres
A critical assessment of methods for the intrinsic analysis of liquid interfaces: 2. density profiles
Substantial improvements in the molecular level understanding of fluid interfaces have recently been achieved by recognizing the importance of detecting the intrinsic surface of the coexisting condensed phases in computer simulations (i.e., after the removal of corrugations caused by capillary waves) and by developing several methods for identifying the molecules that are indeed located at the boundary of the two phases. In our previous paper [J. Phys. Chem. C 2010, 114, 11169], we critically compared those methods in terms of reliability, robustness, and computation speed. Once the intrinsic surface of a given phase is detected, various profiles, such as the density profiles of the components, can be calculated relative to this intrinsic surface rather than to the macroscopically planar Gibbs dividing surface. As a continuation of our previous study, here we present a detailed and critical comparison of various methods that can be used to calculate intrinsic density profiles once the full set of truly interfacial molecules has been identified. Two of the methods, the Fourier function and the Voronoi tessellation, are already described in the literature; two other methods, the covering surface and the triangular interpolation, are newly proposed algorithms; one method, the modified grid-based intrinsic profile (GIP) method, is an improvement over an existing procedure. The different methods are again compared in terms of accuracy and computational cost. On the basis of this comparison, we propose a fast and accurate protocol to be routinely used for intrinsic surface analyses in computer simulations
A critical assessment of methods for the intrinsic analysis of liquid interfaces. 1. surface site distributions
Substantial progress in our understanding of interfacial structure and dynamics has stemmed from the recent development of algorithms that allow for an intrinsic analysis of fluid interfaces. These work by identifying the instantaneous location of the interface, at the atomic level, for each molecular configuration and then computing properties relative to this location. Such a procedure eliminates the broadening of the interface caused by capillary waves and reveals the underlying features of the system. However, a precise definition of which molecules actually belong to the interfacial layer is difficult to achieve in practice. Furthermore, it is not known if the different intrinsic analysis methods are consistent with each other and yield similar results for the interfacial properties. In this paper, we carry out a systematic and detailed comparison of the available methods for intrinsic analysis of fluid interfaces, based on a molecular dynamics simulation of the interface between liquid water and carbon tetrachloride. We critically assess the advantages and shortcomings of each method, based on reliability, robustness, and speed of computation, and establish consistent criteria for determining which molecules belong to the surface layer. We believe this will significantly contribute to make intrinsic analysis methods widely and routinely applicable to interfacial systems
Flare-induced fountains and buried flares in AGN
We discuss the local physical changes at the surface of an AGN accretion disk
after the onset of a magnetic flare. The X-ray irradiation by a flare creates a
hot spot at the disk surface where the plasma both heats up and expands in the
vertical direction in order to regain the hydrostatic equilibrium. Assuming
that the magnetic loop causing the flare is anchored deeply within the disk
interior, we derive analytical estimates for the vertical dimension H_hot and
the optical depth tau_es of the heated atmosphere as a function of the position
within the spot. We perform computations for various values of the accretion
rate dm/dt, the fraction f_cor of radiation dissipated within the disk corona,
and the covering factor f_cover of the disk surface with flare-illuminated
patches. It turns out that generally we can distinguish three characteristic
radial zones within the disk showing a qualitatively different behavior of the
heated material. In the innermost regions of the disk (inner zone) the
expansion of the disk material is restricted by strong gravitational forces.
Further out, the flare source, initially above the disk, soon becomes embedded
by the expanding disk atmosphere. At these intermediate disk radii (middle
zone) the material is optically thick thus greatly modifying the observed
radiation by multiple Compton scattering. We show exemplary spectra models
obtained from Monte Carlo simulations illustrating the trends. In the outermost
regions of the disk (outer zone) the expanding material is optically thin and
its influence on the observed spectra is smaller but pressure gradients in
radial directions should cause the development of a fountain-like dynamical
structure around the flare source. We discuss the observational consequences of
our results.Comment: 12 pages, 14 figures, accepted by Astronomy & Astrophysic
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