7,779 research outputs found
Near-surface stellar magneto-convection: simulations for the Sun and a metal-poor solar analog
We present 2D local box simulations of near-surface radiative
magneto-convection with prescribed magnetic flux, carried out with the MHD
version of the CO5BOLD code for the Sun and a solar-like star with a metal-poor
chemical composition (metal abundances reduced by a factor 100, [M/H]=-2). The
resulting magneto-hydrodynamical models can be used to study the influence of
the metallicity on the properties of magnetized stellar atmospheres. A
preliminary analysis indicates that the horizontal magnetic field component
tends to be significantly stronger in the optically thin layers of metal-poor
stellar atmospheres.Comment: Proc. IAU Symposium 259, Cosmic Magnetic Fields: from Planets, to
Stars and Galaxies, K.G. Strassmeier, A.G. Kosovichev and J.E. Beckman, eds.
(2009) p.23
Interaction effects and transport properties of Pt capped Co nanoparticles
We studied the magnetic and transport properties of Co nanoparticles (NPs)
being capped with varying amounts of Pt. Beside field and temperature dependent
magnetization measurements we performed delta-M measurements to study the
magnetic interactions between the Co NPs. We observe a transition from
demagnetizing towards magnetizing interactions between the particles for an
increasing amount of Pt capping. Resistivity measurements show a crossover from
giant magnetoresistance towards anisotropic magnetoresistance
Electrochemical characterization of nonaqueous systems for secondary battery application
Electrochemical evaluation of electrode organic electrolyte combinations for rechargeable battery system
Microtubule dynamics depart from wormlike chain model
Thermal shape fluctuations of grafted microtubules were studied using high
resolution particle tracking of attached fluorescent beads. First mode
relaxation times were extracted from the mean square displacement in the
transverse coordinate. For microtubules shorter than 10 um, the relaxation
times were found to follow an L^2 dependence instead of L^4 as expected from
the standard wormlike chain model. This length dependence is shown to result
from a complex length dependence of the bending stiffness which can be
understood as a result of the molecular architecture of microtubules. For
microtubules shorter than 5 um, high drag coefficients indicate contributions
from internal friction to the fluctuation dynamics.Comment: 4 pages, 4 figures. Updated content, added reference, corrected typo
Quantum revival patterns from classical phase-space trajectories
A general semiclassical method in phase space based on the final value
representation of the Wigner function is considered that bypasses caustics and
the need to root-search for classical trajectories. We demonstrate its
potential by applying the method to the Kerr Hamiltonian, for which the exact
quantum evolution is punctuated by a sequence of intricate revival patterns.
The structure of such revival patterns, lying far beyond the Ehrenfest time, is
semiclassically reproduced and revealed as a consequence of constructive and
destructive interferences of classical trajectories.Comment: 7 pages, 6 figure
Monte Carlo Study of Short-Range Order and Displacement Effects in Disordered CuAu
The correlation between local chemical environment and atomic displacements
in disordered CuAu alloy has been studied using Monte Carlo simulations based
on the effective medium theory (EMT) of metallic cohesion. These simulations
correctly reproduce the chemically-specific nearest-neighbor distances in the
random alloy across the entire Cu\$_x\$Au\$_{1-x}\$ concentration range. In the
random equiatomic CuAu alloy, the chemically specific pair distances depend
strongly on the local atomic environment (i.e. fraction of like/unlike nearest
neighbors). In CuAu alloy with short-range order, the relationship between
local environment and displacements remains qualitatively similar. However the
increase in short-range order causes the average Cu-Au distance to decrease
below the average Cu-Cu distance, as it does in the ordered CuAuI phase. Many
of these trends can be understood qualitatively from the different neutral
sphere radii and compressibilities of the Cu and Au atoms.Comment: 9 pages, 5 figures, 2 table
On The Evolution of Magnetic White Dwarfs
We present the first radiation magnetohydrodynamics simulations of the
atmosphere of white dwarf stars. We demonstrate that convective energy transfer
is seriously impeded by magnetic fields when the plasma-beta parameter, the
thermal to magnetic pressure ratio, becomes smaller than unity. The critical
field strength that inhibits convection in the photosphere of white dwarfs is
in the range B = 1-50 kG, which is much smaller than the typical 1-1000 MG
field strengths observed in magnetic white dwarfs, implying that these objects
have radiative atmospheres. We have then employed evolutionary models to study
the cooling process of high-field magnetic white dwarfs, where convection is
entirely suppressed during the full evolution (B > 10 MG). We find that the
inhibition of convection has no effect on cooling rates until the effective
temperature (Teff) reaches a value of around 5500 K. In this regime, the
standard convective sequences start to deviate from the ones without convection
owing to the convective coupling between the outer layers and the degenerate
reservoir of thermal energy. Since no magnetic white dwarfs are currently known
at the low temperatures where this coupling significantly changes the
evolution, effects of magnetism on cooling rates are not expected to be
observed. This result contrasts with a recent suggestion that magnetic white
dwarfs with Teff < 10,000 K cool significantly slower than non-magnetic
degenerates.Comment: 11 pages, 12 figures, accepted for publication in the Astrophysical
Journa
Physics of a microsystem starting from non-equilibrium quantum statistical mechanics
In this paper we address the problem to give a concrete support to the idea,
originally stemming from Niels Bohr, that quantum mechanics must be rooted
inside the physics of macroscopic systems. It is shown that, starting from the
formalism of the non-equilibrium statistical operator, which is now a
consolidated part of quantum statistical mechanics, particular correlations
between two isolated systems can be singled out and interpreted as
microsystems. In this way also a new framework is established in which
questions of decoherence can be naturally addressed.Comment: 14 pages, latex, no figures, contribution to the Proceedings of the
XXXIII Symposium on Mathematical Physics (Torun, Poland
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