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Influence of selenization pressure on the growth of Cu2ZnSnSe4 films from stacked metallic layers

dc.contributor.authorSalomé, P. M. P.
dc.contributor.authorFernandes, P. A.
dc.contributor.authorCunha, A. F. da
dc.date.accessioned2014-01-22T11:11:27Z
dc.date.available2014-01-22T11:11:27Z
dc.date.issued2010
dc.description.abstractCu2ZnSnSe4 (CZTSe) is a p-type semiconductor with a high absorption coefficient, 104 to 105 cm-1, and is being seen as a possible replacement for Cu(In,Ga)Se2 in thin film solar cells. Yet, there are some fundamental properties of CZTSe that are not well known, one of them is its band gap. In order to resolve its correct value it is necessary to improve the growth conditions to ensure that single phase crystalline thin films are obtained. One of the problems encountered when growing CZTSe is the loss of Sn through evaporation of SnSe. Stoichiometric films are then difficult to obtain and usually there are other phases present. One possible way to overcome this problem is to increase the pressure of growth of CZTSe. This can be done by introducing an atmosphere of an inert gas like Ar or N2. In this work we report the results of morphological, structural and optical studies of the properties of CZTSe thin films grown by selenization of DC magnetron sputtered metallic layers under different Ar pressures. The films are analysed by SEM/EDS, Raman scattering and XRD.por
dc.identifier.doi10.1002/pssc.200982748pt_PT
dc.identifier.issn1610-1642
dc.identifier.urihttp://hdl.handle.net/10400.22/3420
dc.language.isoengpor
dc.peerreviewedyespor
dc.publisherWiley-VCHpor
dc.relation.ispartofseriesPhysica Status Solidi (c); Vol. 7, Issue 3-4
dc.relation.publisherversionhttp://onlinelibrary.wiley.com/doi/10.1002/pssc.200982748/abstractpor
dc.titleInfluence of selenization pressure on the growth of Cu2ZnSnSe4 films from stacked metallic layerspor
dc.typejournal article
dspace.entity.typePublication
oaire.citation.endPage916por
oaire.citation.issueIssue 3-4
oaire.citation.startPage913por
oaire.citation.titlePhysica Status Solidi (c)por
oaire.citation.volumeVol. 7por
rcaap.rightsopenAccesspor
rcaap.typearticlepor

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