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Radiative defects in CuGaS2 thin films
The radiative defects in vacuum-deposited CuGaS2 is studied by photoluminescence spectroscopy (PL). The PL of Cu-rich layers is dominated by donor–acceptor lines at 2.3 and 2.26eV attributed to a common shallow donor (the S vacancy) and two acceptors (possibly Ga vacancies and CuGa antisites). The P...
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Published in: | Physica. B, Condensed matter Condensed matter, 2003-12, Vol.340-342, p.923-927 |
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creator | Botha, J.R. Branch, M.S. Leitch, A.W.R. Weber, J. |
description | The radiative defects in vacuum-deposited CuGaS2 is studied by photoluminescence spectroscopy (PL). The PL of Cu-rich layers is dominated by donor–acceptor lines at 2.3 and 2.26eV attributed to a common shallow donor (the S vacancy) and two acceptors (possibly Ga vacancies and CuGa antisites). The PL of near-stoichiometric to Ga-rich layers is dominated by green PL in the 2.3–2.45eV range and broad yellow/red luminescence below 2.2eV. The green PL is interpreted in terms of the (0/+) and (+/2+) levels associated with the S vacancy (a double donor), and the Cu vacancy (an acceptor). The yellow/red PL is typical for highly compensated semiconductors and is ascribed to donor–acceptor transitions involving Cu vacancies and deep donor levels. |
doi_str_mv | 10.1016/j.physb.2003.09.203 |
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B, Condensed matter</title><description>The radiative defects in vacuum-deposited CuGaS2 is studied by photoluminescence spectroscopy (PL). The PL of Cu-rich layers is dominated by donor–acceptor lines at 2.3 and 2.26eV attributed to a common shallow donor (the S vacancy) and two acceptors (possibly Ga vacancies and CuGa antisites). The PL of near-stoichiometric to Ga-rich layers is dominated by green PL in the 2.3–2.45eV range and broad yellow/red luminescence below 2.2eV. The green PL is interpreted in terms of the (0/+) and (+/2+) levels associated with the S vacancy (a double donor), and the Cu vacancy (an acceptor). 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B, Condensed matter</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Botha, J.R.</au><au>Branch, M.S.</au><au>Leitch, A.W.R.</au><au>Weber, J.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Radiative defects in CuGaS2 thin films</atitle><jtitle>Physica. B, Condensed matter</jtitle><date>2003-12-31</date><risdate>2003</risdate><volume>340-342</volume><spage>923</spage><epage>927</epage><pages>923-927</pages><issn>0921-4526</issn><eissn>1873-2135</eissn><abstract>The radiative defects in vacuum-deposited CuGaS2 is studied by photoluminescence spectroscopy (PL). The PL of Cu-rich layers is dominated by donor–acceptor lines at 2.3 and 2.26eV attributed to a common shallow donor (the S vacancy) and two acceptors (possibly Ga vacancies and CuGa antisites). The PL of near-stoichiometric to Ga-rich layers is dominated by green PL in the 2.3–2.45eV range and broad yellow/red luminescence below 2.2eV. The green PL is interpreted in terms of the (0/+) and (+/2+) levels associated with the S vacancy (a double donor), and the Cu vacancy (an acceptor). The yellow/red PL is typical for highly compensated semiconductors and is ascribed to donor–acceptor transitions involving Cu vacancies and deep donor levels.</abstract><pub>Elsevier B.V</pub><doi>10.1016/j.physb.2003.09.203</doi><tpages>5</tpages></addata></record> |
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subjects | CuGaS2 Intrinsic defects Photoluminescence |
title | Radiative defects in CuGaS2 thin films |
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