Copper Indium Dis elenide (CIS) based solar cells: effect of CIS preparation conditions and thickness on performance
dc.contributor.author | Mwabora, Julius Mwakondo | |
dc.date.accessioned | 2019-08-29T09:57:21Z | |
dc.date.accessioned | 2020-01-07T15:46:34Z | |
dc.date.available | 2019-08-29T09:57:21Z | |
dc.date.available | 2020-01-07T15:46:34Z | |
dc.date.issued | 1999 | |
dc.description | Available in print form | en_US |
dc.description.abstract | The effect of CuInSe2 thin film preparation conditions and thickness on CuInSe2 based solar cells has been investigated. Prior to CuInSe2 thin films and device fabrication, metallic Cu and in resistivity changes with deposition conditions were studied. The CuInSe2 thin films were fabricated by two stage process which involved DC sputtering of metallic CuIn bilayers followed by reaction of the bilayels in H2SE gas in a chemical vapor deposition reactor. Metallic Cu and In films resistivities depend on vacuum deposition conditions as well as their thicknesses. For deposition parameters studied in this work, Cu film resistivity changes are within the order of 10' while those for In film were up to order of 10". A semi quantitative description on the formation of CuInSe2 films with respect to reaction period, reaction temperature, and precursor thickness has been given. This has helped to explain the phases observed and their effects on device performance. Low reaction temperatures require long reaction periods for complete reaction of CuIn precursors which is consistent with low reaction rate constants for low reaction temperatures. At temperatures greater than 400 °C device performance deteriorates. A kinetic model was used to predict the progressive number of moles of CuInSe2 and InSe phases in the selenized Culn bilayers and compared with experimental number of moles calculated from XRD counts. Generally, the experimental data were found to be in good qualitative agreement with those predicted. The best solar cell (efficiency was 10.6 %} in this work was obtained using an absorber layer with a trace of InSe phase. This means a good device with efficiency greater than 10 % can be obtained using an absorber layer with a trace of InSe phase provided that the number of InSe moles approaches zero. For each reaction period, there is a limiting CuInSe2 thickness which gives the highest efficiency. Similarly, for each precursor thickness, there is a limiting efficiency which can be obtained. For commercial considerations, the most interesting result is the 7.41 % efficiency obtained for a 0.6 mm thick CuInSe2 absorber layer prepared for 15 minutes at reaction temperature of 350°C. The thinner CuInSe2 saves the starting Cu and In materials while the short reaction period and the lower reaction temperature translates to low operating costs. | en_US |
dc.identifier.citation | Mwabora, J. M. (1999) Copper Indium Dis elenide (CIS) based solar cells: effect of CIS preparation conditions and thickness on performance, Masters’ dissertation, University of Dar es Salaam. Available at (http://41.86.178.3/internetserver3.1.2/detail.aspx) | en_US |
dc.identifier.uri | http://localhost:8080/xmlui/handle/123456789/1904 | |
dc.language.iso | en | en_US |
dc.publisher | University of Dar es Salaam | en_US |
dc.subject | Copper indium | en_US |
dc.subject | Copper content | en_US |
dc.subject | Copper industry and trade | en_US |
dc.subject | Tanzania | en_US |
dc.title | Copper Indium Dis elenide (CIS) based solar cells: effect of CIS preparation conditions and thickness on performance | en_US |
dc.type | Thesis | en_US |