Conference Record of the Twentieth IEEE Photovoltaic Specialists Conference 1988
DOI: 10.1109/pvsc.1988.105992
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CuInSe/sub 2/ films prepared by screen-printing and sintering method

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Cited by 12 publications
(4 citation statements)
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“…This facile particle growth has rarely been reported primarily because sintering of highly crystalline CIGS nanoparticles is difficult because of the high melting point of CIGS. 17,20 Interestingly, this substrate temperature of 520 °C (Figure 4d) is very close to the melting temperature of CuSe binary phase, which was found to exist in our binary mixture precursors. From this result, we claim that the significant growth of the Cu−In−Se nanoparticles by selenization at 520 °C is closely related to the presence of amorphous Cu−Se phase in the precursor particles, also supported by the fact that particle growth was not remarkable when the substrate temperature was in the range of 280 to 430 °C.…”
Section: ■ Results and Discussionsupporting
confidence: 67%
“…This facile particle growth has rarely been reported primarily because sintering of highly crystalline CIGS nanoparticles is difficult because of the high melting point of CIGS. 17,20 Interestingly, this substrate temperature of 520 °C (Figure 4d) is very close to the melting temperature of CuSe binary phase, which was found to exist in our binary mixture precursors. From this result, we claim that the significant growth of the Cu−In−Se nanoparticles by selenization at 520 °C is closely related to the presence of amorphous Cu−Se phase in the precursor particles, also supported by the fact that particle growth was not remarkable when the substrate temperature was in the range of 280 to 430 °C.…”
Section: ■ Results and Discussionsupporting
confidence: 67%
“…Attempts to use such layers without annealing have produced only limited photovoltaic response 134. However, sintering such materials is difficult as the high melting point of CIGS leads to very limited sintering at the temperatures accessible on low‐cost substrates 135. Similar difficulties are encountered when using atomically mixed ternary and quaternary precursor particles, probably due to the formation of CIGS at very low temperatures, before significant inter‐particle sintering has occurred 136,137.…”
Section: Particulate Processes For Cigs Depositionmentioning
confidence: 99%
“…N 2 H 4 , or nanoparticle routes without organic coordination of the metal cations are preferred. However, lower molecular intermixing and remaining porosity are evident downsides of the nanoparticle route . In that regard, it is imperative to find suitable fluxing agents to ensure metal diffusion and grain growth.…”
Section: Introductionmentioning
confidence: 99%