• Korean Journal of Materials Research
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• v.20 no.1
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• pp.12-18
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• 2010

$CuInSe_2$ (CIS) thin films were electrodeposited on Mo-coated glass substrates in acidic solutions containing $Cu^{2+}$, $In^{3+}$, and $Se^{4+}$ ions, depending on deposition parameters such as deposition potential (-0.4 to -0.8 V[SCE]) and pH (1.7 to 1.9). The influences of PH and deposition potential on the atomic composition of Cu, In, and Se in the deposited films were observed. The best chemical composition, approaching 1:1:2 atomic ratio for the elements, was achieved at -0.5 V (SCE) and pH 1.8. The as-deposited films showed low crystallinity and were annealed at 300 to $500^{\circ}C$ for 30 min to improve crystallization. The surface morphologies, microstructures, and crystallographic structures of the annealed films as well as the as-deposited films were analyzed with AFM, SEM, and XRD. The defects of spherical particles appeared on the surfaces of CIS thin films in the as-deposited state and decreased in size and number with increasing annealing temperatures. Additionally, the crystallization to chalcopyrite structure and surface roughness (Ra) of the as-deposited thin films were improved with the annealing process.

• Journal of the Korean Institute of Electrical and Electronic Material Engineers
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• v.15 no.12
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• pp.1070-1074
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• 2002

We have carried out two-beam interference experiments to form holographic gratings on As$_{40}$ Se$_{15}$ S$_{35}$Ge$_{10}$ single layer, Ag/As$_{40}$ Se$_{15}$ S$_{35}$Ge$_{10}$ multi-layer. In this study, holographic gratings have been formed using He-Ne laser(632.8nm) under different polarization combinations(intensity polarization holography, phase polarization holography). The diffraction efficiency was obtained by the +lst order intensity. The maximum diffraction efficiency of As$_{40}$ Se$_{15}$ S$_{35}$Ge$_{10}$ single layer, As$_{40}$ Se$_{15}$ S$_{35}$Ge$_{10}$ and MgF$_2$/As$_{40}$ Se$_{15}$ S$_{35}$Ge$_{10}$ multi-layer were 0.8%, 1.4% and 3.1% under intensity polarization holography, respectively.

• Proceedings of the Korean Institute of Electrical and Electronic Material Engineers Conference
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• 2003.07a
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• pp.331-334
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• 2003

Photovoltaics is considered as one of the most promising new energy technology, because its energy source is omni present, pollution-free and inexhaustive. It is agreed that these solar cells must be thin film type because thin film process is cost-efficive in the fact that it uses much less raw materials and can be continuous. The defect chalcopyrite material $CuIn_3Se_5$ has been identified as playing an essential role in efficient photovoltaic action in $CuInSe_2$-based devicesm It has been reported to be of n-type conductivity, forming a p-n junction with its p-type counterpart $CuInSe_2$. Because the most efficient cells consist of the $Cu(In,Ga)Se_2$ quarternary, knowledge of some physical properties of the Ga-containing defect chalcopyrite $Cu(In,Ga)_3Se_5$ may help us better understand the junction phenomena in such devices.

• Proceedings of the Korean Vacuum Society Conference
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• 2014.02a
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• pp.338.2-338.2
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• 2014

투명반도체산화물은 우수한 광학적, 전기적 특성을 가지고 있기 때문에 차세대 박막트랜지스터의 채널층으로 각광을 받고 있다. 특히, 그 중에서도 a-IGZO를 이용한 TFT는 높은 가시광선 투과율(>80%)과 큰 전하이동도(>10 cm2/Vs) 를 갖는 등 좋은 광학적, 전기적 특성을 갖기 때문에 많은 연구가 이루어졌다. 여러 연구들에 의하면, a-IGZO TFT는 소스/드레인의 전극으로 어떤 물질을 사용하는지에 따라서 동작특성에 큰 영향을 미치는 것으로 알려져 있다. 일반적으로, a-IGZO 박막은 n형 반도체로써 일함수가 작은 금속과는 ohmic contact를 형성하고, 일함수가 큰 금속과는 Schottky barrier를 형성한다고 알려져 있다. 이와 관련된 대부분의 이전의 연구들에서는 각각의 전극물질에 따라 전기적인 특성변화에 초점을 맞춰서 연구하였다. 본 연구에서는 일함수가 작은 Ag와 일함수가 큰 Au를 a-IGZO의 박막 위에 얇게 증착하면서 이에 따른 고분해능 광전자분광(high-resolution x-ray photoelectron spectroscopy) 정보의 변화를 분석함으로써, 금속의 증착에 따른 금속층과 a-IGZO 표면 및 계면에서의 화학적 상태의 변화를 연구하였다. Au 4f, Ag 3d는 metallic property를 나타내기 이전까지는 lower binding energy(BE) 쪽으로 shift하였으며, In 3d 또한 lower BE 성분이 크게 증가하였다. O 1s, Ga 3d, Zn 3d들은 상대적으로 적은 변화를 나타내었는데, 이는 Ag, Au가 In과 상대적으로 더 많이 상호작용한다는 것을 의미한다. 본 발표에서는 이들 core level의 정보들과, 가전자대의 분광정보, 그리고 band bending의 정보가 제시될 것이며, 이 정보들은 metal 증착에 따른 contact 특성을 이해하는데 기여할 것으로 기대한다.

• Electrical & Electronic Materials
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• v.7 no.2
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• pp.100-106
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• 1994

A bilayer film consisting of a layer of a-Se$_{75}$ Ge$_{25}$ with a surface layer of silver -100[.angs.] thick and a monolayer film of a-Se$_{75}$ Ge$_{25}$ are irradiated with 9[keV] Ga$^{+}$ ion beam. The Ga$^{+}$ ion (10$^{16}$ [ions/cm$^{2}$] exposed a-Se$_{75}$ Ge$_{25}$ and Ag/a-Se$_{75}$ Ge$_{25}$ thin films show an increase in optical absorption, and the absorption edge on irradiation with shifts toward longer wavelength. The shift toward longer wavelength called a "darkening effect" is observed also in film exposure to optical radiation(4.5*10$^{20}$ [photons/cm$^{2}$]). The 0.3[eV] edge shift for ion irradiation films is about twice to that obtained on irradiation with photons. These large changes are primarily due to structural changes, which lead to high etch selectivity and high sensitivity.

• The Transactions of the Korean Institute of Electrical Engineers
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• v.43 no.2
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• pp.296-302
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• 1994

Polycrystalline CuInSeS12T thin were prepared by depositing Cu/In layer, which was sequentially sputtered varying the Cu/(Cu+In) mole ratio, on glass substrate and selenizing with selenium metal vapor in a nitrogen atmosphere. Compositional and structural, characterization was carried out by X-ray diffraction (XRD), wavelength-dispersive spectroscopy(WDS), and scanning electron microscope(SEM). Electrical characterization was carried out by the measurements of Hall effect, electrical resistivity. Large indium loss occurs in early stage of the selenization process. The selenized films which had mole ratios larger than 0.28 have chalcopyrite CuInSeS12T phase and these that had less mole ratios have sphalerite phase. The selenized films containing CuS1xTSe phase have Cu-rich CuInSeS12T phase and these that did not contain CuS1xTSe have In-rich CuInSeS12T phase. By optimizing the sputtering conditions,it is possible to fabricate CuInSeS12T thin films which have little secondary phases and an appropriate hole concentration (10S015T ~ 10S016TcmS0-3T) for solar cells.

• Proceedings of the Korean Institute of Electrical and Electronic Material Engineers Conference
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• 1994.11a
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• pp.187-189
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• 1994

The degree of the photodoping process in Ag(100 )/a-$Se_{75}Ge_{25}$(2000 ) films has been measured as a funcition of photon energy between 1.5eV and 2.9eV with the exposing time. The window of Ag occurs at 3400 (3.65eV) and Ag is almost transparent in this region. It was shown that transmitance is always constant (40∼50%) for the wavelength ranges of our experiment. It was found that the energy gap of a unexposed a-$Se_{75}Ge_{25}$ film is 1.81eV. Ag photodoping process result in the photodarkenting effect which the absorption edge shift to the large wavelength. Especially, we could obtain very large band shut ( ∼0.3eV) resulting in exposing He-Ne laser(6328[ ]). From the result of our experimental, we suggest that Ag photodoping process depends on the photon absorption in Ag.

• Progress in Superconductivity
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• v.13 no.2
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• pp.117-121
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• 2011

We have fabricated $FeSe_x$ superconducting thin films at much different substrate temperatures of 430 and $610^{\circ}C$ on $Al_2O_3$(0001) substrates by using a pulsed laser deposition (PLD) technique. Superconducting transitions for both films were shown around 10 K, but their transition width and growth directions of grains were different. We found that superconducting tetragonal FeSe phases and non-superconducting hexagonal FeSe phases were coexisted in the sample grown at the low temperature of $430^{\circ}C$, whereas the hexagonal FeSe phase was decreased with increasing fabrication temperatures.

• Applied Chemistry for Engineering
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• v.26 no.5
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• pp.526-532
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• 2015

Solar cells with other alternative energies are being importantly recognized related with post-2020 climate change regime formation. In a point of view of materials, solar cells are classified to organic and inorganic solar cells which can provide a plant-scale electricity. In particular, recent studies about compound semiconductor solar cells, such as III-V tandem solar cells, chalcopyrite-series CIGSSe solar cells, and kesterite-series CZTSSe solar cells were rapidly accelerated. In this report, we introduce a research trend and technical issues for the compound semiconductor solar cells.

• Current Photovoltaic Research
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• v.3 no.1
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• pp.21-26
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• 2015

High efficiency $Cu(In,Ga)Se_2$ solar cells are generally prepared above $500^{\circ}C$. Lowering the process temperature can allow wider selection of substrate material and process window. In this paper, the three-stage co-evaporation process widely used to grow CIGS thin film at high temperature was modified to reduce the maximum substrate temperature. Below $400^{\circ}C$ the CIGS films show poor crystal growth and lower solar cell performance, in spite of external Na doping by NaF. As a new approach, Cu source instead of Cu with Se in the second stage was applied on the $(In,Ga)_2Se_3$ precursor at $400^{\circ}C$ and achieved a better crystal growth. The distribution of Ga in the films produce by new method were investigated and solar cells were fabricated using these films.