1,990 research outputs found
Electronic band structure of novel tetragonal BiOCuS as a parent phase for novel layered superconductors
Very recently, the tetragonal BiOCuS was synthesized and declared as a new
superconducting system with Fe-oxypnictide - related structure. Here, based on
first-principle FLAPW-GGA calculations, the structural parameters, electronic
bands picture, density of states and electron density distribution for BiOCuS
are investigated for the first time. Our results show that, as distinct from
related metallic-like FeAs systems, BiOCuS phase behaves as an ionic
semiconductor with the calculated indirect band gap at about 0.48 eV. The
superconductivity for BiOCuS may be achieved exclusively by doping of this
phase. Our preliminary results demonstrate that as a result of hole doping, the
[CuS] blocks become conducting owing to mixed Cu 3d + S 3p bands located near
the Fermi level. For the hole doped BiOCuS the Fermi surface adopts a
quasi-two-dimensional character, similarly to FeAs SCs.Comment: 10 pages, 5 figure
Threshold concentration for H blistering in defect free W
Lattice distortion induced by high concentration of H is believed to be
precursor of H blistering in single crystalline W (SCW) during H isotope
irradiation. However, the critical H concentration needed to trigger
bond-breaking of metal atoms presents a challenge to measure. Using density
functional theory, we have calculated the formation energy of a vacancy and a
self-interstitial atom (SIA) in supersaturated defect-free SCW with various H
concentrations. When the ratio of H:W exceeds 1:2, the formation of both
vacancies and self-interstitials becomes exothermic, meaning that spontaneous
formation of micro-voids which can accommodate molecular H2 will occur.
Molecular H2 is not allowed to form, and it is not needed either at the very
initial stage of H blistering in SCW. With supersaturated H, the free volume at
the vacancy or SIA is greatly smeared out with severe lattice distortion and
more H can be trapped than in the dilute H case.Comment: 13 pages, 4 figure
A new triclinic modification of the pyrochlore-type KOs2O6 superconductor
A new modification of KOs2O6, the representative of a new structural type
(Pearson symbol aP18, a=5.5668(1)A, b=6.4519(2)A, c=7.2356(2)A, space group
P-1, no.2) was synthesized employing high pressure technique. Its structure was
determined by single-crystal X-ray diffraction. The structure can be described
as two OsO6 octahedral chains relating to each other through inversion and
forming big voids with K atoms inside. Quantum chemical calculations were
performed on the novel compound and structurally related cubic compound.
High-pressure X-ray study showed that cubic KOs2O6 phase was stable up to
32.5(2) GPa at room temperature.Comment: 23 pages, 9 figures,6 tables. Accepted for J. Solid State Che
Oxygen molecule dissociation on carbon nanostructures with different types of nitrogen doping
Energy barrier of oxygen molecule dissociation on carbon nanotube or graphene
with different types of nitrogen doping is investigated using density
functional theory. The results show that the energy barriers can be reduced
efficiently by all types of nitrogen doping in both carbon nanotubes and
graphene. Graphite-like nitrogen and Stone-Wales defect nitrogen decrease the
energy barrier more efficiently than pyridine-like nitrogen, and a dissociation
barrier lower than 0.2 eV can be obtained. Higher nitrogen concentration
reduces the energy barrier much more efficiently for graphite-like nitrogen.
These observations are closely related to partial occupation of {\pi}* orbitals
and change of work functions. Our results thus provide useful insights into the
oxygen reduction reactions.Comment: Accepted by Nanoscal
Functional identification of Arabidopsis ATSIP2 (At3g57520) as an alkaline α-galactosidase with a substrate specificity for raffinose and an apparent sink-specific expression patter
Arabidopsis ATSIP2 has recently been suggested to be a raffinose synthase gene. However, it has high amino acid identity to functionally characterized alkaline α-galactosidases from Cucumis melo and Zea mays. Using the Sf9 insect cell expression system, we demonstrate that recombinant ATSIP2 is a genuine alkaline α-galactosidase with a distinct substrate specificity for raffinose, and not a raffinose synthase. A β-glucuronidase reporter construct using the ATSIP2 promoter shows that ATSIP2 is strongly expressed in sink tissues of Arabidopsis, i.e. sink leaves and non-xylem parts of the root stele, suggesting a physiological function in raffinose phloem unloading
Calculation of solubility in titanium alloys from first-principles
We present an approach to calculate the atomic bulk solubility in binary
alloys based on the statistical-thermodynamic theory of dilute lattice gas. The
model considers all the appropriate ground states of the alloy and results in a
simple Arrhenius-type temperature dependence determined by a {\it
"low-solubility formation enthalpy"}. This quantity, directly obtainable from
first-principle calculations, is defined as the composition derivative of the
compound formation enthalpy with respect to nearby ground states. We apply the
framework and calculate the solubility of the A specie in A-Ti alloys
(A=Ag,Au,Cd,Co,Cr,Ir,W,Zn). In addition to determining unknown low-temperature
ground states for the eight alloys, we find qualitative agreements with
solubility experimental results. The presented formalism, correct in the
low-solubility limit, should be considered as an appropriate starting point for
determining if more computationally expensive formalisms are otherwise needed.Comment: 10 pages, 12 figure
The melting curve of iron at extreme pressures: implications for planetary cores
Exoplanets with masses similar to that of Earth have recently been discovered
in extrasolar systems. A first order question for understanding their dynamics
is to know whether they possess Earth like liquid metallic cores. However, the
iron melting curve is unknown at conditions corresponding to planets of several
times the Earth's mass (over 1500 GPa for planets with 10 times the Earth's
mass (ME)). In the density-temperature region of the cores of those
super-Earths, we calculate the iron melting curve using first principle
molecular dynamics simulations based on density functional theory. By comparing
this melting curve with the calculated thermal structure of Super Earths, we
show that planets heavier than 2ME, have solid cores, thus precluding the
existence of an internal metallic-core driven magnetic field. The iron melting
curve obtained in this study exhibits a steeper slope than any calculated
planetary adiabatic temperature profile rendering the presence of molten
metallic cores less likely as sizes of terrestrial planets increase
Spin Waves in Disordered III-V Diluted Magnetic Semiconductors
We propose a new scheme for numerically computing collective-mode spectra for
large-size systems, using a reformulation of the Random Phase Approximation. In
this study, we apply this method to investigate the spectrum and nature of the
spin-waves of a (III,Mn)V Diluted Magnetic Semiconductor. We use an impurity
band picture to describe the interaction of the charge carriers with the local
Mn spins. The spin-wave spectrum is shown to depend sensitively on the
positional disorder of the Mn atoms inside the host semiconductor. Both
localized and extended spin-wave modes are found. Unusual spin and charge
transport is implied.Comment: 14 pages, including 11 figure
Electronic structure and magnetic properties of the graphene/Fe/Ni(111) intercalation-like system
The electronic structure and magnetic properties of the graphene/Fe/Ni(111)
system were investigated via combination of the density functional theory
calculations and electron-spectroscopy methods. This system was prepared via
intercalation of thin Fe layer (1 ML) underneath graphene on Ni(111) and its
inert properties were verified by means of photoelectron spectroscopy.
Intercalation of iron in the space between graphene and Ni(111) changes
drastically the magnetic response from the graphene layer that is explained by
the formation of the highly spin-polarized  quantum-well state in the
thin iron layer.Comment: Manuscript and supplementary material
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