• 한국진공학회:학술대회논문집
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• 한국진공학회 2014년도 제46회 동계 정기학술대회 초록집
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• pp.220.1-220.1
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• 2014

본 연구에서는 PECVD 공법 중에 이온화 에너지가 높은 선형이온빔 소스를 이용하여 고온에서 전도성 카본박막을 코팅하였다. 카본 박막 코팅을 위한 Precursor는 $C_2H_2$ gas를 이용하였으며, 온도에 따른 카본 박막의 전기적 특성 및 두께에 따른 카본 박막 성장 구조를 분석하였다. 카본 박막의 전기적 특성은 Interfacial contact resistance (ICR) 방법으로 측정하였으며, 접촉 저항 측정을 위한 모재는 SUS316L stainless steel을 사용하였고 카본 박막 성장 구조 분석을 위해서는 폴리싱된 Si-wafer를 사용하였다. 선형이온빔 소스를 이용하여 상온에서 증착한 카본 코팅의 접촉저항 값은 50 nm 코팅 두께에서 $660m{\Omega}cm^2@10kgf/cm^2$으로 비정질상의 특성을 나타냈으며, 고온에서는 $14.8m{\Omega}cm^2@10kgf/cm^2$으로 온도가 증가함에 따라 비정질상의 카본 박막이 전도성을 가지는 카본박막으로의 성장을 확인할 수 있었다. 또한 전도성 카본 박막의 성장 구조 분석은 FE-SEM 및 Raman spectrum 분석을 통해 확인하였으며, 그 결과 코팅 두께가 증가할수록 카본 입자들은 수nm에서 약 150 nm의 카본 cluster를 형성하며 성장하였다. 이때 전도성 카본 박막의 두께에 따른 접촉저항의 값은 고온 조건에서 카본 박막의 두께가 약 100 nm일 때, $12.1m{\Omega}cm^2@10kgf/cm^2$의 가장 낮은 값을 가졌다. 위의 결과를 경제성이 아주 우수한 대면적 전도성 나노 카본 박막의 상용화 가능성이 높아질 것으로 기대된다.

• Journal of Electrical Engineering and Technology
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• 제7권6호
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• pp.965-970
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• 2012

Structure and optical properties of cadmium sulphide-zinc oxide composite nanorods have been evaluated by suitable characterization techniques. The X-ray diffraction spectrum contains a series of peaks corresponding to reflections from various sets of lattice planes of hexagonal ZnO as well as CdS. The above observation is supported by the Micro-Raman spectroscopy result. The optical reflectance spectra of CdS-ZnO is compared with that of ZnO where we observe an enhanced absorption and hence diminished reflection from CdS-ZnO compared to that from only ZnO. A very small intensity of the visible photoluminescence peak observed at 550 nm proves that the ZnO nanorods have very low concentrations of point defects such as oxygen vacancies and zinc interstitials. The photocurrent in the visible region has been significantly enhanced due to deposition of CdS on the surface of the ZnO nanorods. CdS acts as a visible sensitizer because of its lower band gap compared to ZnO.

• 한국진공학회:학술대회논문집
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• 한국진공학회 2009년도 제38회 동계학술대회 초록집
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• pp.69-69
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• 2010

The research is the structural and optical characteristics of the Cadmium Sulfide(CdS) film, nanowires and nanobelts grown on the $Al_2O_3$ substrate using the vapor phase epitaxy method. The field-emission scanning electron microscopy(FE-SEM) were used to identify the shape of the surface of the nanostructures and x-ray diffraction(XRD) and transmission electron microscopy (TEM) were used to evaluate the structural characterisitcs. As a result, the XRD was confirmed the CdS peak and the substrate peak and TEM showed single crystals with wurtzite hexagonal structure on the nanostructures. As for the optical characteristic of the nanostructures, photoluminescence(PL) and micro-raman spectrum were measured. The PL measurements confirmed the emission peak related bound exciton to neutral donor($D^0X$) peak and free exciton(FX) peak. The micro-raman spectrum showed that the peak of the nanostructures were similar to the pure crystalline CdS peak and each peak were overtone of LO phonon of the hexagonal CdS of the longitudinal optical(LO) phonon mode. Therefore, it is confirmed that the CdS nanostructures grown in this research have superior crystallinity.

• 공업화학
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• 제19권3호
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• pp.322-325
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• 2008

3,3-Dimethyl-1-butene ($C_6H_{12}$) 모노머를 PECVD 증착하였다. 비정질 탄소막은 FT-IR 스펙트럼에서 R.F.전력/압력비가 증가할수록 수소의 함유량과 dangling bond가 감소되고 막의 기계적 특성은 밀도가 상승함으로써 비례하여 향상되었다. 또한 Raman 스펙트럼에서 D 피크가 증가하였고 고리구조의 막을 형성하였다. 따라서 경도와 모듈러스가 각각 12 GPa과 85 GPa였다. 증착된 막의 굴절률(n)과 흡광계수(k)는 전력/압력비가 상승할수록 증가하였다.

• 한국산학기술학회논문지
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• 제16권5호
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• pp.3378-3384
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• 2015

최근에 라만스펙트럼에 대한 고속 검색 방법은 많은 관심을 받아왔다. 지금까지 가장 간단하고 널리 사용되는 방법은 주어진 스펙트럼과 데이터베이스 스펙트라 사이의 유클리드 거리를 계산하고 비교하는 방법이다. 하지만 고차원 데이터의 속성으로 검색의 문제는 그리 간단하지 않다. 가장 큰 문제점중의 하나는 검색 방법에 있어서 연산량이 많아 계산 시간이 너무 오래 걸린다는 것이다. 이러한 문제점을 극복하기 위해, 코드워드의 MPS(Mean Pyramids Search)와 PDS(Partial Distortion Search)을 사용하는 알고리즘이 현재 이미지 코딩 분야에서 고속 검색 알고리즘으로 널리 사용되고 있다. 하지만 이 방법은 1차원 데이터의 경우에는 적합하지 않다. 본 논문에서 우리는 라만 스펙트럼 데이터에 적합한 3가지 새로운 방법의 고속 검색 알고리즘을 제안한다. 이 방법은 벡터의 두 개의 주요한 특징으로 평균과 분산을 사용하여 후보가 될 수 없는 많은 코드워드를 계산하지 않으므로 연산량을 줄이고 계산 시간을 줄여준다. 실험은 1DMPS+PDS와 비교하여 1DMPS Sort+PDS는 42.8%, 1DMPS Sort+PDS는 48.6%, 1DMPS Sort with Sorted Variance+PDS는 55.2%의 성능향상을 보였다. 실험결과는 제안된 알고리즘이 고속 검색에 적합함을 확인시켜 준다.

• 한국진공학회:학술대회논문집
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• 한국진공학회 2009년도 제38회 동계학술대회 초록집
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• pp.59-59
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• 2010

Graphene is a 2-D sheet of $sp^2$-bonded carbon arranged in a honeycomb lattice. This material has attracted major interest, and there are many ongoing efforts in developing graphene devices because of its high charge mobility and crystal quality. Therefore clear understanding of the substrate effect and mechanism of synthesis of graphene is important for potential applications and device fabrication of graphene. In a published paper in J. Phys. Chem. C (2008), the effect of substrate on the atomic/electronic structures of graphene is negligible for graphene made by mechanical cleavage. However, nobody shows the interaction between Ni substrate and graphene. Therefore, we have studied this interaction. In order to studying these effect between graphene and Ni substrate, We have observed graphene synthesized on Ni substrate and graphene transferred on $SiO_2$/Si substrate through Raman spectroscopy. Because Raman spectroscopy has historically been used to probe structural and electronic characteristics of graphite materials, providing useful information on the defects (D-band), in-plane vibration of sp2 carbon atoms (G-band), as well as the stacking orders (2D-band), we selected this as analysis tool. In our study, we could not observe the doping effect between graphene and Ni substrate or between graphene and $SiO_2$/Si substrate because the shift of G band in Raman spectrum was not occurred by charge transfer. We could noticed that the bonding force between graphene and Ni substrate is more strong than Van de Waals force which is the interaction between graphene and $SiO_2$/Si. Furthermore, the synthesized graphene on Ni substrate was in compressive strain. This phenomenon was observed by 2D band blue-shift in Raman spectrum. And, we consider that the graphene is incommensurate growth with Ni polycrystalline substrate.

• 한국진공학회:학술대회논문집
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• 한국진공학회 2013년도 제44회 동계 정기학술대회 초록집
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• pp.277-277
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• 2013

The epitaxial graphene on the 4H- or 6H-SiC(0001) surface has been intensively studied due to the possibility of wafer-scale growt. However the existence of interface layer (zero layer graphene) and its influence on the upper graphene layer have been considered as one of the main obstarcles for the industrial application. Among various methods tried to overcome the strong interaction with the substrate through the interface layer, it has been proved that the hydrogen intercalation successfully passivate the Si dangling bond of the substrate and can produce the quasi-free standing epitaxial graphene (QFEG) layers on the siC(0001) surface. In this study, we report the results of the angle-resolved photoemission spectroscopy (ARPES) and Raman spectroscopy for the QFEG layers produced by ex-situ and in-situ hydrogen intercalation.From the ARPES measurement, we confirmed that the Dirac points of QFEG layers exactly coincide with the Fermi level. The band structure of QFEG layer are sustainable upon thermal heating up to 1100 K and robust against the deposition of several metals andmolecular deposition. We also investigated the strain of the QFEG layers by using Raman spectroscopy measurement. From the change of the 2D peak position of graphene Raman spectrum, we found out that unlike the strong compressive strain in the normal epitaxial graphene on the SiC(0001) surface, the strain of the QFEG layer are significantly released and almost similar to that of the mechanically exfoliated graphene on the silicon oxide substrate. These results indicated that various ideas proposed for the ideal free-standing graphene can be tested based on the QFEG graphene layers grown on the SiC(0001) surface.

• 한국표면공학회지
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• 제51권2호
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• pp.126-132
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• 2018

SnS thin films with different substrate temperatures ($150 {\sim}300^{\circ}C$) as process parameters were grown on soda-lime glass substrates by RF magnetron sputtering. The effects of substrate temperature on the structural and optical properties of SnS thin films were investigated by X-ray diffraction (XRD), Raman spectroscopy (Raman), field-emission scanning electron microscopy (FESEM), energy dispersive X-ray spectroscopy (EDS), and Ultraviolet-visible-near infrared spectrophotometer (UV-Vis-NIR). All of the SnS thin films prepared at various substrate temperatures were polycrystalline orthorhombic structures with (111) planes preferentially oriented. The diffraction intensity of the (111) plane and the crystallite size were improved with increasing substrate temperature. The three major peaks (189, 222, $289cm^{-1}$) identified in Raman were exactly the same as the Raman spectra of monocrystalline SnS. From the XRD and Raman results, it was confirmed that all of the SnS thin films were formed into a single SnS phase without impurity phases such as $SnS_2$ and $Sn_2S_3$. In the optical transmittance spectrum, the critical wavelength of the absorption edge shifted to the long wavelength region as the substrate temperature increased. The optical bandgap was 1.67 eV at the substrate temperature of $150^{\circ}C$, 1.57 eV at $200^{\circ}C$, 1.50 eV at $250^{\circ}C$, and 1.44 eV at $300^{\circ}C$.

• 천문학회지
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• 제48권2호
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• pp.105-112
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• 2015

The symbiotic star V1016 Cygni, a detached binary system consisting of a hot white dwarf and a mass-losing Mira variable, shows very broad emission features at around 6825 Å and 7082 Å, which are Raman scattered O vi λλ 1032, 1038 by atomic hydrogen. In the high resolution spectrum of V1016 Cyg obtained with the Bohyunsan Optical Echelle Spectrograph these broad features exhibit double peak profiles with the red peak stronger than the blue counterpart. However, their profiles differ in such a way that the blue peak of the 7082 feature is relatively weaker than the 6825 counterpart when the two Raman features are normalized to exhibit an equal red peak strength in the Doppler factor space. Assuming that an accretion flow around the white dwarf is responsible for the double peak profiles, we attribute this disparity in the profiles to the local variation of the flux ratio of O vi λλ 1032, 1038 in the accretion flow. A Monte Carlo technique is adopted to provide emissivity maps showing the local emissivity of O vi λ1032 and O vi λ1038 in the vicinity of the white dwarf. We also present a map indicating the differing flux ratios of O vi λλ 1032 and 1038. Our result shows that the flux ratio reaches its maximum of 2 in the emission region responsible for the central trough of the Raman feature and that the flux ratio in the inner red emission region is almost 1. The blue emission region and the outer red emission region exhibit an intermediate ratio around 1.5. We conclude that the disparity in the profiles of the two Raman O vi features strongly implies accretion flow around the white dwarf, which is azimuthally asymmetric.

• BMB Reports
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• 제42권4호
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• pp.223-226
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• 2009

We measured the pH-induced spectral changes of yeast iso-1-cytochrome c on silver nanoparticle surfaces using surface-enhanced resonance Raman scattering (SERRS) at 457.9 nm. At a pH of ~3, the Met80 ligand in yeast iso-1-cytochrome c is assumed to dissociate, leading to a marked conformational change as evidenced by the vibrational spectral shifts. The Soret band at ~410 nm in the UV-Vis spectrum shifted to ~396 nm at pH~3, indicating a transition from a low spin state to a high spin state from a weak interaction with a water molecule. Thus, SERRS spectroscopy can measure the pH-induced denaturalization of cyt c adsorbed on metal nanoparticle surfaces at a lower concentration with a better sensitivity than ordinary resonance Raman spectroscopy.