3,713 research outputs found

    Characterization of CoTiO3 Nanocrystallites Prepared by Homogeneous Precipitation Method

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    Nanocrystalline cobalt titanate (CoTiO3) has been synthesized from a well-mixed precursor. The precursor was prepared by a homogeneous precipitation method, in which urea was used as the precipitator. The as-synthesized sample is a mixture of CoTiO3 and rutile nanocrystallites with mean sizes of around 50 nm. It strongly absorbs visible light in the wavelength range of 500-690 nm besides ultraviolet light (wavelength < 370 nm). We found the synthetic CoTiO3 is a semiconducting material with a direct band gap of 2.53 eV. The green CoTiO3 has two absorbance peaks at the wavelengths of 537 and 606 nm, which correspond to the photon energies of 2.31 and 2.05 eV, respectively. When you are citing the document, use the following link http://essuir.sumdu.edu.ua/handle/123456789/3195

    Fabrication Process Simulation of a PEM Fuel Cell Catalyst Layer and Its Microscopic Structure Characteristics

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    The catalyst layers (CLs) in proton exchange membrane fuel cells (PEMFCs) are porous composites of complex microstructures of the building blocks, i.e., Pt nano-particles, carbonaceous substrates and Nafion ionomers. It is important to understand the factors that control the microstructure formation in the fabrication process. A coarse-grained molecular dynamics (CG-MD) method is employed to investigate the fabrication process of CLs, which depends on the type and amount of components and also the type of the dispersion medium (ethylene glycol, isopropanol or hexanol) used during ink preparation of the catalyst-coated membranes (CCMs). The dynamical behaviors of all the components are outlined and analyzed following the fabrication steps. In addition, the Pt nano-particle size distribution is evaluated and compared with the labor testing. Furthermore, the primary pore size distributions in the final formations of three cases are shown and compared with the experiments. The sizes of the reconstructed agglomerates are also considered on the effect of solvent polarity. (C) 2012 The Electrochemical Society. [DOI: 10.1149/2.064203jes] All rights reserved

    GluA3 subunits are required for appropriate assembly of AMPAR GluA2 and GluA4 subunits on cochlear afferent synapses and for presynaptic ribbon modiolar-pillar morphology

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    Cochlear sound encoding depends on α-amino-3-hydroxy-5-methyl-4-isoxazole propionic acid receptors (AMPARs), but reliance on specific pore-forming subunits is unknown. With 5-week-old male C57BL/6

    Experimental study on mechanical behavior of RPC circular columns confined by high-strength stirrups under axial compression

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    The axial compression mechanical behavior of Reactive Power Concrete (RPC) circular columns which confined by the spiral hoop of yield strength 600MPa are tested, and the tie spacing and volume tie ratio were used to evaluate the RPC columns failure modes, load-displacement relationship and yield characteristics of high-strength stirrups. The results show that the peak stress of the 250mm diameter circular column with no reinforcement can be up to 144.4MPa but with brittle failure mode, and the large volume tie ratio can increase the peak stress to 180MPa and failure by ductility; also, the high-strength spiral stirrups do not yield at the peak axial load, and the effective confined stress should be calculated according to the measured stirrups strain , and the remaining strength can be ensured the good ductility of the RPC specimens before reaching the ultimate failure mode; the peak strength and strain of RPC are proportional to linearly increase with effective confinement stress, but the proportion coefficient is smaller than that of ordinary concrete. The decline section of RPC stress-strain curve becomes smooth with the increase of effective binding stress, and the ductility coefficient of displacement gradually satisfies the ductility design requirements. The measured RPC stress-strain curve agrees well with the confined concrete Mander model and can be used conservatively. According to the test results, the calculation formula and the construction measurements of the axial compression capacity of the RPC with the spiral stirrup confined are put forward, which is convenient for the popularization and application of the confined RPC columns in the practical engineering

    Galactic Disk Bulk Motions as Revealed by the LSS-GAC DR2

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    We report a detailed investigation of the bulk motions of the nearby Galactic stellar disk, based on three samples selected from the LSS-GAC DR2: a global sample containing 0.57 million FGK dwarfs out to \sim 2 kpc, a local subset of the global sample consisting \sim 5,400 stars within 150 pc, and an anti-center sample containing \sim 4,400 AFGK dwarfs and red clump stars within windows of a few degree wide centered on the Galactic anti-center. The global sample is used to construct a three-dimensional map of bulk motions of the Galactic disk from the solar vicinity out to \sim 2 kpc with a spatial resolution of \sim 250 pc. Typical values of the radial and vertical components of bulk motion range from -15 km s1^{-1} to 15 km s1^{-1}, while the lag behind the circular speed dominates the azimuthal component by up to \sim 15 km s1^{-1}. The map reveals spatially coherent, kpc-scale stellar flows in the disk, with typical velocities of a few tens km s1^{-1}. Bending- and breathing-mode perturbations are clearly visible, and vary smoothly across the disk plane. Our data also reveal higher-order perturbations, such as breaks and ripples, in the profiles of vertical motion versus height. From the local sample, we find that stars of different populations exhibit very different patterns of bulk motion. Finally, the anti-center sample reveals a number of peaks in stellar number density in the line-of-sight velocity versus distance distribution, with the nearer ones apparently related to the known moving groups. The "velocity bifurcation" reported by Liu et al. (2012) at Galactocentric radii 10--11 kpc is confirmed. However, just beyond this distance, our data also reveal a new triple-peaked structure.Comment: 27 pages, 17 figures, Accepted for publication in a special issue of Research in Astronomy and Astrophysics on LAMOST science
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