81 research outputs found
Pressure-induced amorphization and polyamorphism in one-dimensional single crystal TiO2 nanomaterials
The structural phase transitions of single crystal TiO2-B nanoribbons were
investigated in-situ at high-pressure using the synchrotron X-ray diffraction
and the Raman scattering. Our results have shown a pressure-induced
amorphization (PIA) occurred in TiO2-B nanoribbons upon compression, resulting
in a high density amorphous (HDA) form related to the baddeleyite structure.
Upon decompression, the HDA form transforms to a low density amorphous (LDA)
form while the samples still maintain their pristine nanoribbon shape. HRTEM
imaging reveals that the LDA phase has an {\alpha}-PbO2 structure with short
range order. We propose a homogeneous nucleation mechanism to explain the
pressure-induced amorphous phase transitions in the TiO2-B nanoribbons. Our
study demonstrates for the first time that PIA and polyamorphism occurred in
the one-dimensional (1D) TiO2 nanomaterials and provides a new method for
preparing 1D amorphous nanomaterials from crystalline nanomaterials.Comment: 4 figure
Chemodynamical Properties and Ages of Metal-Poor Stars in S-PLUS
Metal-poor stars are key to our understanding of the early stages of chemical
evolution in the Universe. New multi-filter surveys, such as the Southern
Photometric Local Universe Survey (S-PLUS), are greatly advancing our ability
to select low-metallicity stars. In this work, we analyse the chemodynamical
properties and ages of 522 metal-poor candidates selected from the S-PLUS data
release 3. About 92% of these stars were confirmed to be metal-poor ([Fe/H]
) based on previous medium-resolution spectroscopy. We calculated the
dynamical properties of a subsample containing 241 stars, using the astrometry
from Gaia Data Release 3. Stellar ages are estimated by a Bayesian isochronal
method formalized in this work. We analyse the metallicity distribution of
these metal-poor candidates separated into different subgroups of total
velocity, dynamical properties, and ages. Our results are used to propose
further restrictions to optimize the selection of metal-poor candidates in
S-PLUS. The proposed astrometric selection ( mas) is
the one that returns the highest fraction of extremely metal-poor stars (16.3%
have [Fe/H] ); the combined selection provides the highest fraction of
very metal-poor stars (91.0% have [Fe/H] ), whereas the dynamical
selection (eccentricity > 0.35 and diskness < 0.75) is better for targetting
metal-poor (99.5% have [Fe/H] ). Using only S-PLUS photometric
selections, it is possible to achieve selection fractions of 15.6%, 88.5% and
98.3% for metallicities below 3, 2 and 1, respectively. We also show
that it is possible to use S-PLUS to target metal-poor stars in halo
substructures such as Gaia-Sausage/Enceladus, Sequoia, Thamnos and the Helmi
stream.Comment: 18 pages, 13 figures. To be published in MNRAS main journal (accepted
15-may-2023
Elastic properties of mono- and polycrystalline hexagonal AlB2-like diborides of s, p and d metals from first-principles calculations
We have performed accurate ab initio total energy calculations using the
full-potential linearized augmented plane wave (FP-LAPW) method with the
generalized gradient approximation (GGA) for the exchange-correlation potential
to systematically investigate elastic properties of 18 stable, meta-stable and
hypothetical hexagonal (AlB2-like) metal diborides MB2, where M = Na, Be, Mg,
Ca, Al, Sc, Y, Ti, Zr, Hf, V, Nb, Ta, Cr, Mo, W, Ag and Au. For monocrystalline
MB2 the optimized lattice parameters, independent elastic constants (Cij), bulk
modules (B), shear modules (G) are obtained and analyzed in comparison with the
available theoretical and experimental data. For the first time numerical
estimates of a set of elastic parameters of the polycrystalline MB2 ceramics
(in the framework of the Voigt-Reuss-Hill approximation), namely bulk and shear
modules, compressibility, Young's modules, Poisson's ratio, Lame's coefficients
are performed.Comment: 24 pages, 3 figure
Natural Resources for Therapeutic Use: Evidence from Brazil.
Identify plants used for insect stings in selfcare practices in the situation of suffering by people living in a rural location of Santa Maria municipality, Southern Brazil
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