• Title/Summary/Keyword: energy band

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Study on energy of valence-band splitting from photocurrent spectrum of photoconductive $CdGa_2Se_4$ thin films

  • Hong, Kwang-Joon
    • Proceedings of the Korean Institute of Electrical and Electronic Material Engineers Conference
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    • 2009.11a
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    • pp.66-66
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    • 2009
  • The photoconductive $CdGa_2Se_4$ layer was grown through the hot wall epitaxy method. From the photocurrent (PC) measurements, the three peaks in the PC spectra were associated with the band-to-band transitions. The PC intensities were observed to decrease with decreasing temperature. The valence-band splitting on $CdGa_2Se_4$ was also observed by means of the PC spectroscopy. The crystal field splitting and the spin orbit splitting turned out to be 0.1604 and 0.4179 eV at 10 K, respectively.

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A Study on the Band Structure of ZnO/CdS Heterojunction for CIGS Solar-Cell Application

  • Sim, Hana;Lee, Jeongmin;Cho, Seongjae;Cho, Eou-Sik;Kwon, Sang Jik
    • JSTS:Journal of Semiconductor Technology and Science
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    • v.15 no.2
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    • pp.267-275
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    • 2015
  • In this paper, ZnO films were prepared by atomic layer deposition (ALD) and CdS films were deposited using chemical bath deposition (CBD) to form ZnO/CdS heterojunction. More accurate mapping of band arrangement of the ZnO/CdS heterojunction has been performed by analyzing its electrical and optical characteristics in depth by various methods including transmittance, x-ray photoemission spectroscopy (XPS), and ultraviolet photoemission spectroscopy (UPS). The optical bandgap energies ($E_g$) of ZnO and CdS were 3.27 eV and 2.34 eV, respectively. UPS was capable of extracting the ionization potential energies (IPEs) of the materials, which turned out to be 8.69 eV and 7.30 eV, respectively. The electron affinity (EA) values of ZnO and CdS calculated from IPE and $E_g$ were 5.42 eV and 4.96 eV, respectively. Energy-band structures of the heterojunction could be accurately drawn from these parameters taking the conduction band offset (CBO) into account, which will substantially help acquisition of the full band structures of the thin films in the CIGS solar-cell device and contribute to the optimal device designs.

Computer-simulation with Different Types of Bandgap Profiling for Amorphous Silicon Germanium Thin Films Solar Cells

  • Jo, Jae-Hyeon;Lee, Jun-Sin
    • Proceedings of the Korean Vacuum Society Conference
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    • 2014.02a
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    • pp.320-320
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    • 2014
  • Amorphous silicon alloy (a-Si) solar cells and modules have been receiving a great deal of attention as a low-cost alternate energy source for large-scale terrestrial applications. Key to the achievement of high-efficiency solar cells using the multi-junction approach is the development of high quality, low band-gap materials which can capture the low-energy photons of the solar spectrum. Several cell designs have been reported in the past where grading or buffer layers have been incorporated at the junction interface to reduce carrier recombination near the junction. We have investigated profiling the composition of the a-SiGe alloy throughout the bulk of the intrinsic material so as to have a built-in electrical field in a substantial portion of the intrinsic material. As a result, the band gap mismatch between a-Si:H and $a-Si_{1-x}Ge_x:H$ creates a barrier for carrier transport. Previous reports have proposed a graded band gap structure in the absorber layer not only effectively increases the short wavelength absorption near the p/i interface, but also enhances the hole transport near the i-n interface. Here, we modulated the GeH4 flow rate to control the band gap to be graded from 1.75 eV (a-Si:H) to 1.55 eV ($a-Si_{1-x}Ge_x:H$). The band structure in the absorber layer thus became like a U-shape in which the lowest band gap was located in the middle of the i-layer. Incorporation of this structure in the middle and top cell of the triple-cell configuration is expected to increase the conversion efficiency further.

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Defect Formatìon and Annealìng Behavìor in MeV Si Self-Implanted Silicon (MeV Si 자기 이온주입된 단결정 Silicon내의 결함 거동)

  • Cho, Nam-Hoon;Jang, Ki-Wan;Suh, Kyung-Soo;Lee, Jeoung-Yong;Ro, Jae-Sang
    • Korean Journal of Materials Research
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    • v.6 no.7
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    • pp.733-741
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    • 1996
  • In this study MeV Si self ion implantations were done to reveal the intrinsic behavior of defect formation by excluding the possibility of chemical interactions between substrate atoms and dopant ones. Self implantations were conducted using Tandem Accelerator with energy ranges from 1 to 3 MeV. Defect formation by high energy ion implantation has a significant characteristics in that the lattice damage is concentrated near Rp and isolated from the surface. In order to investigate the energy dependence on defect formation, implantation energies were varied from 1 to 3 MeV under a constant dose of $1{\times}10^{15}/cm^2$. RBS channe!ed spectra showed that the depth at which as-implanted damaged layer formed increases as energy increases and that near surface region maintains better crystallinity as energy increases. Cross sectional TEM results agree well with RBS ones. In a TEM image as-implanted damaged layer appears as a dark band, where secondary defects are formed upon annealing. In the case of 2 MeV $Si^+$ self implantation a critical dose for the secondary defect formation was found to be between $3{\times}10^{14}/cm^24$ and $5{\times}10^{14}/cm^2$. Upon annealing the upper layer of the dark band was removed while the bottom part of the dark band did not move. The observed defect behavior by TEM was interpreted by Monte Carlo computer simulations using TRIM-code. SIMS analyses indicated that the secondary defect formed after annealing gettered oxygen impurities existed in silicon.

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SnS (tin monosulfide) thin films obtained by atomic layer deposition (ALD)

  • Hu, Weiguang;Cho, Young Joon;Chang, Hyo Sik
    • Proceedings of the Korean Vacuum Society Conference
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    • 2016.02a
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    • pp.305.2-305.2
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    • 2016
  • Tin monosulfide (SnS) is one promising candidate absorber material which replace the current technology based on cadmium telluride (CdTe) and copper indium gallium sulfide selenide (CIGS) for its suitable optical band gap, high absorption coefficient, earth-abundant, non-toxic and cost-effective. During past years work, thin film solar cells based on SnS films had been improved to 4.36% certified efficiency. In this study, Tin monosul fide was obtained by atomic layer deposition (ALD) using the reaction of Tetrakis (dimethylamino) tin (TDMASn, [(CH3)2N]4Sn) and hydrogen sulfide (H2S) at low temperatures (100 to 200 oC). The direct optical band gap and strong optical absorption of SnS films were observed throughout the Ultraviolet visible spectroscopy (UV VIS), and the properties of SnS films were analyzed by sanning Electron Microscope (SEM) and X-Ray Diffraction (XRD).

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Excitation Energy Induced S-shaped PL behavior in Graphene Quantum Dots

  • Jang, Min-Ho;Jo, Yong-Hun
    • Proceedings of the Korean Vacuum Society Conference
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    • 2016.02a
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    • pp.351.2-351.2
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    • 2016
  • Graphene quantum dots (GQDs) have attracted much attention because of various advantages such as cost-effectiveness of synthesis, low toxicity, and photostability. The origins of photoluminescence (PL) in GQDs were suggested as the intrinsic states for localized sp2 carbon domains and the extrinsic states formed by oxygen-functional groups.[1,2] Nevertheless, it is still unclear to understand the information of electric band structure in GQD. Here, we observed excitation energy induced S-shaped PL behavior. The PL peak energy position shows an S-shaped shift (redshift-blueshift-redshift) as function of the excitation wavelengths. From various samples, we only observed S-shaped PL shift in the GQDs with both luminescent origins of intrinsic and extrinsic states. Therefore, this S-shaped PL shift is related to different weight of intrinsic and extrinsic states in PL spectrum depending on the excitation wavelengths. This would be the key result to understand the electric band structure of the GQDs and its derivatives.

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The Growth and Optical Properties of $MgGa_2Se_4$ Single Crystal ($MgGa_2Se_4$ 단결정의 성장과 광학적 특성)

  • 김형곤;이광석;이기형
    • Journal of the Korean Institute of Telematics and Electronics
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    • v.25 no.4
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    • pp.402-406
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    • 1988
  • The MgGa2Se4 single crystal for study of optical properties is for the first time grown by Bridgmna method. The crystal structure of grown MgGa2Se4 single crystal has the Rhomobohedral structure (R3m) and its lattice constant are a=3.950\ulcorner c=38.893\ulcornerin Hexagonal structure. The energy band structure of grown MgGa2Se4 single crystal structure has direct band gap and the optical energy gap measured from optical absorption in this crystal is 2.20eV at 290K. The temperature dependence of energy gap was given Eg(T)=Eg(O)-aT\ulcorner)B+T), from varshni equation, where Eg(O)=2.34eV, a=8.79x10**-4eV/and b=250K.

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졸-겔법에 의한 CdS 분산$SiO_2$ Glass 박막의 비선형광학특성

  • 문종수;강종봉;김경문
    • Journal of the Korean Ceramic Society
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    • v.33 no.12
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    • pp.1353-1364
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    • 1996
  • Recently semiconductor doped glasses have attracted attention as nonlinear optical materials because of their large third order nonlinear optical properties. The transparent and homogeneous CdS-doped SiO2 glass thin films were obtained by the dip=coating process of the sol-gel method. Thin films were consisted of glasses containing CdS microcrystallites which were formed by dissolved Cd2+ and S2- ions in a SiO2 matrix solutions. A subsequent thermal treatment of this samples led the formation of colloidal agglomerates and finally of microcrystallites. The size of CdS microcrystallites was about 4 to 15 nm after thermal treatments at various heating conditions. From the optical absorption spectra of the CdS-doped SiO2 glass films it was found that the absorption edge was blue-shifted compared with that of the bulk CdS crystal(~2, 4 eV) and that the amount of energy shift was inversely proportional to the crystal size. And the band gap energy increased with the decrease in crystallite size indicating that the quantum size effects occured.

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Binding energy study from photocurrent signal in HgCdTe layers

  • Hong, Kwang-Joon
    • Proceedings of the Korean Institute of Electrical and Electronic Material Engineers Conference
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    • 2010.06a
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    • pp.379-379
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    • 2010
  • $Hg_{1_x}Cd_xTe$ (MCT) was grown by hot wall epitaxy. Prior to the MCT growth, the CdTe (111) buffer layer was grown on the GaAs substrate at the temperature of $590^{\circ}C$ for 15 min. When the thickness of the CdTe buffer layer was $5\;{\mu}m$ or thicker, the full width at half maximum values obtained from the x-ray rocking curves were found to significantly decrease. After a good quality CdTe buffer layer was grown, the MCT epilayers were grown on the CdTe (111) /GaAs substrate at various temperatures in situ. The crystal quality for those epilayers was investigated by means of the x-ray rocking curves and the photocurrent experiment. The photoconductor characterization for the epilayers was also measured. The energy band gap of MCT was determined from the photocurrent measurement and the x composition rates from the temperature dependence of the energy band gap were turned out.

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Simulation of Radiative Property Effects on Radiant Cooling of Opaque Surface (비 투과면 복사 냉각에 대한 복사 물성의 영향 예측)

  • Byun, Ki-Hong
    • Journal of the Korean Solar Energy Society
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    • v.29 no.6
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    • pp.32-38
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    • 2009
  • The effects of surface radiative properties on the radiant cooling of opaque surfaces under clear sky condition are studied. Two types of surfaces, one gray and the other selective, are compared. For the nighttime cooling, black surface gives the lowest plate temperature and on the other hand the ideal selective surface gives the highest temperature. The reverse is true when there is an insolation. Equivalent radiative heat transfer coefficient of radiant cooling without convection is about $1{\sim}7\;W/m^2-K$ for the range of values studied. The surface with black within the $6{\sim}13\;{\mu}m$ band else zero emissivity could be regarded as a black surface for the nighttime radiant cooling purposes. However, lower band limit of $4\;{\mu}m$ is preferred to $6\;{\mu}m$ for small insolation situations.