• Title/Summary/Keyword: Dark I-V

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Study on Grain Boundaries in Single-layer Graphene Using Ultrahigh Resolution TEM

  • Lee, Zong-Hoon
    • Proceedings of the Korean Vacuum Society Conference
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    • 2012.08a
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    • pp.107-107
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    • 2012
  • Recently, large-area synthesis of high-quality but polycrystalline graphene has been advanced as a scalable route to applications including electronic devices. The presence of grain boundaries (GBs) may be detrimental on some electronic, thermal, and mechanical properties of graphene, including reduced electronic mobility, lower thermal conductivity, and reduced ultimate mechanical strength, yet on the other hand, GBs might be beneficially exploited via controlled GB engineering. The study of graphene grains and their boundary is therefore critical for a complete understanding of this interesting material and for enabling diverse applications. I present that scanning electron diffraction in STEM mode makes possible fast and direct identification of GBs. We also demonstrate that dark field TEM imaging techniques allow facile GB imaging for high-angle tilt GBs in graphene. GB mapping is systematically carried out on large-area graphene samples via these complementary techniques. The study of the detailed atomic structure at a GB in suspended graphene uses aberration-corrected atomic resolution TEM at a low kV.

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Enhancement of Photocurrent Generation of Solid State Dye Sensitized Solar Cells by Using MgO-coated TiO2 Photoelectrode

  • Lee, Dong-Jun;Han, Gil-Sang;Jeong, Hyeon-Seok
    • Proceedings of the Korean Vacuum Society Conference
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    • 2012.08a
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    • pp.197-197
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    • 2012
  • 염료감응형 태양전지 (DSSC)는 다양한 태양전지 중, 가장 환경친화적이고, 생산단가도 낮을 뿐만 아니라 다양한 색상과 투광성을 확보할 수 있어 많은 연구가 진행되어왔다. 하지만 액체 전해질을 사용하는 기존 염료감응형 태양전지는 높은 휘발성과 열 팽창 수축에 따른 전해질 누액의 문제점으로 인하여 최근에는 고체전해질을 이용한 염료감응형 태양전지의 개발이 활발히 이루어지고 있다. 본 연구에서는 스크린 프린팅법을 이용하여 TiO2 광전극을 코팅하고 Mg(OH)2를 솔-젤법을 이용하여 스핀 코팅 하였다. 이후에 $500^{\circ}C$에서 1시간동안 열처리를 통해 MgO 나노 코팅막을 형성하여 고체 박막 태양전지(solid state dye sensitized solar cells)을 제작하였다. MgO 나노 코팅막의 특성은 솔라시뮬레이터를 이용하여 I-V 곡선, transient Voc, dark current를 측정하였고, UV0vis spectroscopy를 이용하여 염료흡착량을 분석하여 코팅막과 효율간의 상관관계를 평가하였다.

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The Analysis of Electrical Characteristics of PV Module according to Mechanical Load Test (태양전지모듈의 기계적 하중시험에 따른 전기적 특성 분석)

  • Kim, Kyung-Soo;Kang, Gi-Hwan;Yu, Gwon-Jong
    • 한국태양에너지학회:학술대회논문집
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    • 2008.04a
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    • pp.247-251
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    • 2008
  • In this paper. we analyze electrical characteristics of photovoltaic module according to mechanical load test. Using the equipment for giving load on the surface of module, dark current-voltage is measured. By varying load from 0kg to 206kg, slight different I-V curve is detected. From this, reduced shunt resistance is roughly calculated and micro crack is assumed to be happened. system Through this experiment, periodic external force on PV module might give an negative effect. The detailed analysis is described in the following paper.

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태양전지모듈용 EVA의 가속 열화 메카니즘

  • Jeong, Jae-Seong;U, Dong-Jin;Park, No-Chang;Han, Chang-Un;Hong, Won-Sik
    • Proceedings of the Materials Research Society of Korea Conference
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    • 2011.05a
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    • pp.49.1-49.1
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    • 2011
  • 태양전지 모듈의 25년 이상 보증을 위해 태양전지 모듈을 구성하는 부품 소재의 신뢰성이 부각되고 있다. 현재까지 알려진 태양전지 모듈용 에틸렌 아세테이트 비닐(ethylene Vinyl Acetate, EVA)의 주요 열화 메카니즘은 황변(yellowing)과 박리(delaminaation)이다. 따라서 본 연구에서는 태양전지 모듈을 구성하는 재료 중 EVA 소재의 열화 메커니즘을 도출하기 위해 이미 알려진 스트레스 인자를 이용한 가속 열화시험을 설계한 후 가속열화시험을 실시하였으며, 이로부터 EVA의 열화 메카니즘을 규명하였다. 열화모드 재현을 위해 소형 태양광 모듈을 제작하였으며, Weather-Ometer를 이용하여 열화시험을 수행하였다. 시험조건은 4종 Phase가 1 사이클이 되도록 실험하였으며, Dark 조건 1 Phase 및 Light 조건 3 Phase 조건으로 실시하였다. 태양전지 모듈의 열화량은 매 500 사이클 마다 Light I-V 변화량을 측정하여 분석하였다. EVA의 물리 화학적 열화분석을 위해 단면분석, 적외선분광기(Fourier Transform-Infra Red, FT-IR) 및 주사전자현미경을 이용하여 열화 특성에 대한 분석을 실시하였고, 이를 근거로 EVA의 열화 메커니즘을 규명하였다.

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Merging Galaxy Cluster Abell 115: Weak Lensing with Subaru Observation

  • Kim, Mincheol;Jee, Myungkook J.
    • The Bulletin of The Korean Astronomical Society
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    • v.42 no.2
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    • pp.41.1-41.1
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    • 2017
  • We present weak-lensing analysis of the merging galaxy cluster Abell 115 at z=0.197 based on Subaru i and V band images. As merging clusters often show, Abell 115's merging signatures include radio relics, double X-ray peaks, and large offsets between the cluster member galaxies and the X-ray distributions. A weak-lensing study provides underlying dark matter distribution, the key information to determine the complex merging scenario of the cluster. In this work, we present 2D mass reconstruction of the cluster, which reveals two distinct mass peaks consistent with galaxy distributions. We measure the first weak-lensing mass of each subcluster. Our weak-lensing total mass estimate is a few factors lower than the published dynamical mass obtained from velocity dispersion. This large mass discrepancy may be attributed to a significant departure from dynamical equilibrium. We also re-analyze the archival chandra data and find that the result is consistent with weak-lensing mass.

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Constraints on dark radiation from cosmological probes

  • Rossi, Graziano;Yeche, Christophe;Palanque-Delabrouille, Nathalie;Lesgourgues, Julien
    • The Bulletin of The Korean Astronomical Society
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    • v.40 no.1
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    • pp.44.1-44.1
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    • 2015
  • We present joint constraints on the number of effective neutrino species $N_{eff}$ and the sum of neutrino masses ${\Sigma}m_{\nu}$, based on a technique which exploits the full information contained in the one-dimensional Lyman-${\alpha}$ forest flux power spectrum, complemented by additional cosmological probes. In particular, we obtain $N_{eff}=2.91{\pm}0.22$ (95% CL) and ${\Sigma}m_{\nu}$ < 0.15 eV (95% CL) when we combine BOSS Lyman-${\alpha}$ forest data with CMB (Planck+ACT+SPT+WMAP polarization) measurements, and $N_{eff}=2.88{\pm}0.20$ (95% CL) and ${Sigma}m_{\nu}$ < 0.14 eV (95% CL) when we further add baryon acoustic oscillations. Our results tend to favor the normal hierarchy scenario for the masses of the active neutrino species, provide strong evidence for the Cosmic Neutrino Background from $N_{eff}{\approx}3$($N_{eff}=0$ is rejected at more than $14{\sigma}$), and rule out the possibility of a sterile neutrino thermalized with active neutrinos (i.e., $N_{eff}=4$) - or more generally any decoupled relativistic relic with $${\Delta}N_{eff}{\sim_=}1$$ - at a significance of over $5{\sigma}$, the strongest bound to date, implying that there is no need for exotic neutrino physics in the concordance ${\Lambda}CDM$ model.

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입자침전법을 이용한 광도전체 필름의 X선 반응 특성에 관한 연구

  • Choe, Chi-Won;Gang, Sang-Sik;Jo, Seong-Ho;Gwon, Cheol;Nam, Sang-Hui
    • Proceedings of the Korean Institute of Electrical and Electronic Material Engineers Conference
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    • 2007.06a
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    • pp.176-176
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    • 2007
  • Flat-panel direct conversion detectors used in compound substance of semiconductor are being studied for digital x-ray imaging. Recently, such detectors are deposited by physical vapor deposition(PVD) generally. But, most of materials (HgI2, PbI2, TlBr, PbO) deposited by PVD have shown difficult fabrication and instability for large area x-ray imaging. Consequently, in this paper, we propose applicable potentialities for screen printing method that is coated on a substrate easily. It is compared to electrical properties among semiconductors such as $HgI_2$, $PbI_2$, PbO, HgBrI, InI, and $TlPbI_3$ under investigation for direct conversion detectors. Each film detector consists of an ~25 to $35\;{\mu}m$ thick layer of semiconductor and was coated onto the substrate. Substrates of $2cm{\times}2cm$ have been used to evaluate performance of semiconductor radiation detectors. Dark current, sensitivity and physics properties were measured. Leakage current of $HgI_2$ as low as $9pA/mm^2$ at the operation bias voltage of ${\sim}1V/{\mu}m$ was observed. Such a value is not better than PVD process, but it is easy to be fabricated in high quality for large area x-ray Imaging. Our future efforts will concentrate on optimization of growth of film thickness that is coated onto a-Si TFT array.

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THE HST COSMOS PROJECT: CONTRIBUTION FROM THE SUBARU TELESCOPE

  • TANIGUCHI YOSHIAKI;SCOVILLE N. Z.;SANDERS D. B.;MOBASHER B.;AUSSEL H.;CAPAK P.;AJIKI M.;MURAYAMA T.;MIYAZAK S.;KOMIYAMA Y.;SHIOYA Y.;NAGAO T.
    • Journal of The Korean Astronomical Society
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    • v.38 no.2
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    • pp.187-190
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    • 2005
  • The Cosmic Evolution Survey (COSMOS) is a Hubble Space Telescope (HST) treasury project. The COSMOS aims to perform a 2 square degree imaging survey of an equatorial field in I(F814W) band, using the Advanced Camera for Surveys (ACS). Such a wide field survey, combined with ground-based photometric and spectroscopic data, is essential to understand the interplay between large scale structure, evolution and formation of galaxies and dark matter. In 2004, we have obtained high-quality, broad band images of the COSMOS field (B, V, r', i', and z') using Suprime-Cam on the Subaru Telescope, and we have started our new optical multi-band program, COSMOS-21 in 2005. Here, we present a brief summary of the current status of the COSMOS project together with contributions from the Subaru Telescope. Our future Subaru program, COSMOS-21, is also discussed briefly.

Phenolic Compounds from the Fruits of Paulownia coreana Uyeki (오동나무 열매 추출물의 페놀성 화합물)

  • Si, Chuan-Ling;Kim, Jin-Kyu;Kwon, Dong-Joo;Bae, Young-Soo
    • Journal of the Korean Wood Science and Technology
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    • v.34 no.1
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    • pp.79-85
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    • 2006
  • Paulownia coreana Uyeki fruits were collected, extracted with acetone-$H_2O$ (7:3, v /v), fractionated with n-hexane, methylene chloride, and ethyl acetate, then freeze dried to give some dark brown powder. The ethyl acetate soluble mixture was chromatographed on a Sephadex LH-20 column using a series of aqueous methanol and ethanol-hexane mixture as eluents. Spectrometric analysis such as NMR and MS including TLC were performed to establish the structures of the isolated compounds. From the ethyl acetate fraction, one phenolic acid (I) and five flavonoids (II~VI) and were isolated and elucidated. The antioxidative activities were tested on the isolated compounds, crude and fractionated extractives by DPPH radical scavenging method. The result showed that caffeic acid, kaempferol, luteolin, quercetin and the EtOAc soluble fraction exhibited higher activities than those of ${\alpha}$-tocopherol and BHT.

Photoelectric Properties of PbTe/CuPc Bilayer Thin Films (PbTe/CuPc 이층박막의 광전 특성)

  • Lee, Hea-Yeon;Kang, Young-Soo;Park, Jong-Man;Lee, Jong-Kyu;Jeong, Jung-Hyun
    • Journal of Sensor Science and Technology
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    • v.7 no.1
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    • pp.67-72
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    • 1998
  • The crystallized CuPc and PbTe films are formed by thermal evaporation and pulsed ArF excimer laser ablation. Structural and electrical properties of thin film is observed by XRD and current-voltage(I-V) curves. From XRD analysis, both PbTe and CuPc thin films show a-axis oriented structure. For the measurement of photovoltaic effect, the transverse current-voltage curve of CuPc/Si, PbTe/Si and PbTe/CuPc/Si junctions have been analyzed in the dark and under illumination. The PbTe/CuPc/Si junction exthibits a strong photovoltaic characteristics with short circuit current($J_{sc}$) of $25.46\;mA/cm^{2}$ and open-circuit voltage($V_{oc}$) of 170 mV. Quantum efficiency and power conversion efficiency are calculated to be 15.4% and $3.46{\times}10^{-2}$, respectively. Based on the results of QE and ${\eta}$, the photocurrent process of PbTe/CuPc/Si junction can be explained as following three effective steps; photocarrier generation in the CuPc layer, carrier separation at PbTe/CuPc interface, and finally a transportation of electrons through the PbTe layer.

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