• 제목/요약/키워드: Metal dispersion

검색결과 267건 처리시간 0.034초

파우더, 첨가제의 종류와 함량에 따른 수상 내에서의 파우더 분산에 관한 연구 (A Research on Powder Dispersion Ability Using Several Content, Variety of Powder and Additive in Aqueous System)

  • 김선영;김일구;최승만;이상민
    • 대한화장품학회지
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    • 제38권4호
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    • pp.271-276
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    • 2012
  • 본 연구에서는 파우더와 첨가제의 종류, 함량에 따른 저점도 가용화 제형에서의 파우더 분산성을 연구하였다. 파우더는 화학 구조상 부분적 극성이 존재하여 반발력이 존재하고, 물리적인 구조상 다공성 물질로 접촉 면적이 넓고 밀도가 낮은 PMMA 파우더가 뛰어난 분산성을 보였다. 파우더가 분산되어 있는 견본에 염을 첨가한 견본의 경우 염이 첨가되지 않은 견본에 비해 우수한 분산성을 보여주었다. 이때의 분산성은 염의 농도에 의존적인 성향을 보이며, 같은 농도에서 1가 이온으로 이루어진 NaCl, KCl에 비해 2가 이온으로 이루어진 $MgSO_4$에서 더 높은 분산능을 보였다. 이는 염이 이온화되어 파우더의 주변에 존재하여 파우더간의 반발력을 높여주기 때문에 응집 현상이 줄어들고 분산능을 증가시키는 것으로 해석할 수 있다. 마지막으로 MgSO4 염이 첨가되어 있는 견본에 EDTA를 첨가제로 첨가하면 그렇지 않은 견본에 비해 더욱 뛰어난 분산능을 보여 주었다. EDTA는 금속 양이온과 결합하여 그 작용을 막으므로, EDTA가 포함된 견본은 음이온에 의한 작용이 극대화되어 파우더간의 반발력이 더욱 커지게 된다. 이는 결국 파우더의 수분산성을 향상시키고 제형의 안정화에 도움을 줄 수 있다.

ORTHO/PARA 수소의 전환에의 연구 (Study on the Conversion of Ortho to Para Hydrogen)

  • 김종팔;이광현
    • 한국수소및신에너지학회논문집
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    • 제18권3호
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    • pp.317-324
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    • 2007
  • The conversion reaction of ortho to para hydrogen was studied. The percentage of ortho and para hydrogen is mainly dependent on the equilibrium temperature. Because this reaction is known to be accelerated by the catalyst such as nickel-silicate and ruthenium on silica, we focused in the test and development of the catalysts. We studied metal-silicates because they provide high metal dispersion on support. Nickel-silicate, ruthenium-silicate and mixed-silicate were prepared by the coprecipitation method and used in the reaction at the temperature of liquid nitrogen. The conversion was measured by the difference of thermal conductivity between reference gas and sample gas. The activation condition was important and it affected the activities of the catalysts. Nickel-silicate showed high activities. Ruthenium-silicate also showed relative high activities but mixed-silicate showed poor activities.

The Development of High Contact Fatigue Strength P/M Sprocket for the Silent Chain System

  • Yamanishi, Yuuji;Tsutsui, Tadayuki;Ishii, Kei
    • 한국분말야금학회:학술대회논문집
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    • 한국분말야금학회 2006년도 Extended Abstracts of 2006 POWDER METALLURGY World Congress Part 1
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    • pp.142-143
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    • 2006
  • Recently, automotive engines have changed to the silent chain system in order to reduce noise and to improve reliability. High contact fatigue strength is needed for the sprockets of silent chain system. As a result, a high-contact-fatigue-strength P/M material was developed using the technology of surface rolling, which densifies the surface layer of sintered parts. It was established that the contact fatigue strength of the developed material was a great improvement over that of the conventionally used sintered material.

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$In_2O_3-SnO_2$ 이성분계 소결특성에 있어서 $SnO_2$ 분산성 ($SnO_2$ Dispersion of Sintered Body in $In_2O_3-SnO_2$ Binary System)

  • 전태진;박완수;조명진;김종수;김영수
    • 한국전기전자재료학회:학술대회논문집
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    • 한국전기전자재료학회 2006년도 추계학술대회 논문집 Vol.19
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    • pp.198-198
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    • 2006
  • SnO2가 첨가된 In2O3(ITO) sputtering 타켓은 넓은 파장영역에서의 투광성과 높은 전기전도도의 특성 때문에 여러 종류의 평판형 디스플레이 제품에 사용되고 있다. 사용된 In2O3와 SnO2 분말은 높은 순도의 금속을 사용하였으며, 공질법을 이용하여 분말을 제조하였으며, 혼합된 In2O3-SnO2 분말은 하소조건과 소결조건에 따라 특성을 평가 하였다. 본 연구의 목적인 ITO sprttering 타켓의 SnO2 분산조건은 하소 온도가 증가함에 따라 분산성이 뛰어났으며, 조사된 30wt% 에서 5wt%로 SnO2의 함량이 감소함에 따라 분산성은 향상되었다. 이러한 결과들로부터 ITO 타켓 밀도와 SnO2의 분산성은 1150C 이상에서 휘발하는 SnO2의 량에 의해 크게 영향을 받는다.

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선택적 CO 산화 반응을 위한 Ru/$\alpha-Al_2O_3$ 촉매 고분산 제조 방법에 관한 연구 (Preparation of Highly Dispersed Ru/$\alpha-Al_2O_3$ Catalyst for Preferential CO Oxidation)

  • 엄현지;구기영;정운호;이영우;윤왕래
    • 한국수소및신에너지학회논문집
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    • 제21권5호
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    • pp.390-397
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    • 2010
  • 0.5wt% Ru/$\alpha-Al_2O_3$ catalysts are prepared by deposition-precipitation method for the preferential CO oxidation In order to investigate the effect of pH on the Ru dispersion and particle size, the pH of precursor solution is adjusted to between 5.5 and 9.5. 0.5wt% Ru/$\alpha-Al_2O_3$ catalyst prepared at the pH of 6.5 has high Ru dispersion of 17.9% and small particle size of 7.7nm. In addition, 0.5wt% Ru/$\alpha-Al_2O_3$ catalyst prepared at the pH 6.5 is easily reduced at low temperatures below $150^{\circ}C$ due to high dispersion of $RuO_2$ particle and shows high CO conversion over 90% in the wide temperature range between $100^{\circ}C$ and $160^{\circ}C$. Moreover, the deposition-precipitation is a feasible method to improve the Ru dispersion as compared to the impregnation method. The 0.5wt% Ru/$\alpha-Al_2O_3$ catalyst prepared by deposition-precipitation exhibits higher CO conversion than 0.5wt% Ru/$\alpha-Al_2O_3$ catalysts prepared by impregnation due to higher metal dispersion and better reducibility at low temperature.

Scattering characteristics of metal and dielectric optical nano-antennas

  • Ee, Ho-Seok;Lee, Eun-Khwang;Song, Jung-Hwan;Kim, Jinhyung;Seo, Min-Kyo
    • 한국진공학회:학술대회논문집
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    • 한국진공학회 2015년도 제49회 하계 정기학술대회 초록집
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    • pp.76.1-76.1
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    • 2015
  • Optical resonances of metallic or dielectric nanoantennas enable to effectively convert free-propagating electromagnetic waves to localized electromagnetic fields and vice versa. Plasmonic resonances of metal nanoantennas extremely modify the local density of optical states beyond the optical diffraction limit and thus facilitate highly-efficient light-emitting, nonlinear signal conversion, photovoltaics, and optical trapping. The leaky-mode resonances, or termed Mie resonances, allow dielectric nanoantennas to have a compact size even less than the wavelength scale. The dielectric nanoantennas exhibiting low optical losses and supporting both electric and magnetic resonances provide an alternative to their metallic counterparts. To extend the utility of metal and dielectric nanoantennas in further applications, e.g. metasurfaces and metamaterials, it is required to understand and engineer their scattering characteristics. At first, we characterize resonant plasmonic antenna radiations of a single-crystalline Ag nanowire over a wide spectral range from visible to near infrared regions. Dark-field optical microscope and direct far-field scanning measurements successfully identify the FP resonances and mode matching conditions of the antenna radiation, and reveal the mutual relation between the SPP dispersion and the far-field antenna radiation. Secondly, we perform a systematical study on resonant scattering properties of high-refractive-index dielectric nanoantennas. In this research, we examined Si nanoblock and electron-beam induced deposition (EBID) carbonaceous nanorod structures. Scattering spectra of the transverse-electric (TE) and transverse-magnetic (TM) leaky-mode resonances are measured by dark-field microscope spectroscopy. The leaky-mode resonances result a large scattering cross section approaching the theoretical single-channel scattering limit, and their wide tuning ranges enable vivid structural color generation over the full visible spectrum range from blue to green, yellow, and red. In particular, the lowest-order TM01 mode overcomes the diffraction limit. The finite-difference time-domain method and modal dispersion model successfully reproduce the experimental results.

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THE EVOLUTION OF THE GALACTIC GLOBULAR CLUSTERS.: I. METAL ABUNDANCE CALIBRATIONS

  • Lee, See-Woo;Park, Nam-Kyu
    • 천문학회지
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    • 제17권2호
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    • pp.69-103
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    • 1984
  • Five different calibrations of metal abundances of globular clusters are examined and these are compared with metallicity ranking parameters such as $(Sp)_c$, . Q39 and IR-indices. Except for the calibration $[Fe/H]_H$ by the high dispersion echelle analysis. the other calibration scales are correlated with the morphological parameters of red giant branch. In the $[Fe/H]_H$-scale. the clusters later than ${\sim}F8$ have nearly a constant metal abundance. $[Fe/H]_H{\simeq}-1.05$, regradless of morphological characteristics of horizontal branch and red giant branch. By the two fundamental calibration scales of $[Fe/H]_L$ (derived by the low dispersion analysis) and $[Fe/H]_{{\Delta}s}$ (derived by the spectral analysis of RR Lyrae stars). the globular clusters are divided into the halo clusters with [Fe/H]<-1.0 and the disk clusters confined within the galactocentric distance ${\tau}_G=10\;kpc$ and galactic plane distance |z|=3 kpc. In this case the abundance gradient is given by d[Fe/H]/$dr_G{\approx}-0.05\;kpc^{-1}$ and d[Fe/H]/$d|z|{\simeq}-0.08\;kpc^{-1}$ within ${\tau}_G=20\;kpc$ and |z|=10 kpc, respectively. According to these characteristics of the spatial distribution of globular clusters. the chemical evolution of the galactic globular clusters can be accounted for by the two-zone (disk-halo) slow collapse model when the $[Fe/H]_L$-or $[Fe/H]_{{\Delta}s}$-scale is applied. In the case of $[Fe/H]_H$-scale, the one-zone fast collapse model is preferred for the evolution of globular clusters.

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백금 담지 촉매상에서 에탄올의 저온연소 (Low-Temperature Combustion of Ethanol over Supported Platinum Catalysts)

  • 김문현
    • 한국환경과학회지
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    • 제26권1호
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    • pp.67-78
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    • 2017
  • Combustion of ethanol (EtOH) at low temperatures has been studied using titania- and silica-supported platinum nanocrystallites with different sizes in a wide range of 1~25 nm, to see if EtOH can be used as a clean, alternative fuel, i.e., one that does not emit sulfur oxides, fine particulates and nitrogen oxides, and if the combustion flue gas can be used for directly heating the interior of greenhouses. The results of $H_2-N_2O$ titration on the supported Pt catalysts with no calcination indicate a metal dispersion of $0.97{\pm}0.1$, corresponding to ca. 1.2 nm, while the calcination of 0.65% $Pt/SiO_2$ at 600 and $900^{\circ}C$ gives the respective sizes of 13.7 and 24.6 nm when using X-ray diffraction technique, as expected. A comparison of EtOH combustion using $Pt/TiO_2$ and $Pt/SiO_2$ catalysts with the same metal content, dispersion and nanoparticle size discloses that the former is better at all temperatures up to $200^{\circ}C$, suggesting that some acid sites can play a role for the combustion. There is a noticeable difference in the combustion characteristics of EtOH at $80{\sim}200^{\circ}C$ between samples of 0.65% $Pt/SiO_2$ consisting of different metal particle sizes; the catalyst with larger platinum nanoparticles shows higher intrinsic activity. Besides the formation of $CO_2$, low-temperature combustion of EtOH can lead to many other pathways that generate undesired byproducts, such as formaldehyde, acetaldehyde, acetic acid, diethyl ether, and ethylene, depending strongly on the catalyst and reaction conditions. A 0.65% $Pt/SiO_2$ catalyst with a Pt crystallite size of 24.6 nm shows stable performances in EtOH combustion at $120^{\circ}C$ even for 12 h, regardless of the space velocity allowed.

급속소결에 의해 제조된 Al2O3/Fe-Ni 나노복합재료의 미세조직 및 기계적 특성 (Microstructure and Mechanical Properties of Al2O3/Fe-Ni Nanocomposite Prepared by Rapid Sintering)

  • 이영인;이근재;장대환;양재교;좌용호
    • 한국분말재료학회지
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    • 제17권3호
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    • pp.203-208
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    • 2010
  • A new High Frequency Induction Heating (HFIH) process has been developed to fabricate dense $Al_2O_3$ reinforced with Fe-Ni magnetic metal dispersion particles. The process is based on the reduction of metal oxide particles immediately prior to sintering. The synthesized $Al_2O_3$/Fe-Ni nanocomposite powders were formed directly from the selective reduction of metal oxide powders, such as NiO and $Fe_2O_3$. Dense $Al_2O_3$/Fe-Ni nanocomposite was fabricated using the HFIH method with an extremely high heating rate of $2000^{\circ}C/min$. Phase identification and microstructure of nanocomposite powders and sintered specimens were determined by X-ray diffraction and SEM and TEM, respectively. Vickers hardness experiment were performed to investigate the mechanical properties of the $Al_2O_3$/Fe-Ni nanocomposite.

High Dispersion Spectra of the Elliptical Planetary Ring Nebula NGC 6803

  • 이성재;형식
    • 천문학회보
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    • 제37권1호
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    • pp.80.1-80.1
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    • 2012
  • NGC 6803 is an elliptical ring shape planetary nebula. We analyzed the high dispersion spectra which had been observed with the Hamilton Echelle Spectrograph attached to the 3-m Shane telescope of Lick Observatory. We also investigated the low dispersion UV spectral data obtained with the 60-cm interstellar ultraviolet explorer. Diverse excitation lines were found from neutral to quadruply ionized ions. The temperature diagnostic lines indicate relatively low electron temperatures, i.e., $T_{\epsilon}{\leq}9500$ K for most lines except for [ClIV] - 11,500 K. In spite of its simplistic bi-laterally symmetrical elliptical shape, the nebula appears to be very complex of a hugh density range from 1300 to 80,000 $cm^3$. A comparison of the two epoch data suggests that the density increase occurred in the high excitation line zone near the inner boundary. We derived the chemical abundances of He, C, N, O, Ne, S, Ar, Cl, and K. The chemical abundances of NGC 6803 are enhanced compared with the average Galactic planetary nebula. Our self-consistent photo-ionization model study implies that the effective temperature of the central star is 90,000 K and its luminosity is 2400 $L_{\odot}$. The evolutionary track suggests that the progenitor of NGC 6803 was about 0.9 -- 1.0 $M_{\odot}$ star, which might be born from a metal-rich zone near the galactic disk, but now relocated into the present high Galactic latitude.

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