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        <identifier>oai:www.ideals.illinois.edu:2142/42271</identifier>
        <datestamp>2023-07-11</datestamp>
        <setSpec>col_2142_5131</setSpec>
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        <thesis xmlns="http://www.ndltd.org/standards/metadata/etdms/1.1/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:dc="http://purl.org/dc/elements/1.1/" xsi:schemaLocation="http://www.ndltd.org/standards/metadata/etdms/1.1/ http://www.ndltd.org/standards/metadata/etdms/1.1/etdms11.xsd http://purl.org/dc/elements/1.1/ http://www.ndltd.org/standards/metadata/etdms/1.1/etdmsdc.xsd">
          <dc:contributor>Rockett, Angus A.</dc:contributor>
          <dc:contributor>Rockett, Angus A.</dc:contributor>
          <dc:contributor>Abelson, John R.</dc:contributor>
          <dc:contributor>Bishop, Stephen G.</dc:contributor>
          <dc:contributor>Lyding, Joseph W.</dc:contributor>
          <dc:creator>Hebert, Damon</dc:creator>
          <dc:date>2013-02-03T19:29:53Z</dc:date>
          <dc:date>2013-02-03T19:29:53Z</dc:date>
          <dc:date>2012-12</dc:date>
          <dc:date>2013-02-03T19:29:53Z</dc:date>
          <dc:date>2012-12</dc:date>
          <dc:description>Cu(In,Ga)Se2 (CIGS) and its alloys are the leading choice for thin film
photovoltaic absorber layers due to their high performance in devices, low degradation,
high optical absorption coefficient and high tolerance to off-stoichiometry and intrinsic
defects. Film conductivity and recombination losses are controlled by intrinsic point
defect concentrations, especially in the near-surface space-charge region of the
heterojunction. Despite the amount of research already performed on CIGS alloys, their
optoelectronic properties, defect chemistry and recombination mechanisms are still
poorly understood. The focus of this dissertation is to optically characterize a selection
of CIGS absorber layers fabricated by various techniques in order to better understand the
radiative emission and defect physics. This work aims to identify the defects responsible
for recombination and their relation to grain boundaries and band edge fluctuations,
which limit device performance.
This study used photoluminescence (PL) spectroscopy, photoluminescence
excitation (PLE) spectroscopy, and cathodoluminescence (CL) to study radiative
emissions from a variety of Cu-poor CIGS thin films. Three general types of CIGS films
were analyzed. Polycrystalline layers deposited on Mo-coated soda lime glass,
polycrystalline layers deposited on metal foil, and epitaxial films grown on (100) and
(111) GaAs were analyzed in this work. This work concludes that the donor-acceptor
pair recombination model used in most interpretations of CIGS emission should be
replaced with a model that accounts for high compensation and band edge fluctuations,
which is shown to be undoubtedly the case in Cu-poor CIGS. Within this model, the
most commonly observed emissions were explained as free-to-bound types, specifically
iii
band-to-impurity (BI) and tail-to-impurity (TI) types. Band tail width was measured by
PLE. A correlation was established between band tail width and device efficiency. CIGS
absorber layers that produced devices of higher performance showed narrower band tails.
CL and PL showed an additional deep emission in Na-free films, not present in Nacontaining
films grown in parallel. It is concluded that most grain boundaries in CIGS
act as collection areas for point defects and point defect clusters but also are more or less
inactive with respect to recombination due to their built-in electrostatic hole barrier.
Spectral and spatial emission characteristics were studied on plan-view CIGS
surfaces that were covered with a ~50 nm thick CdS film by chemical bath deposition
(CBD). It is concluded that spectral changes that others have observed in the emission of
CdS-treated films is a result of the CBD process itself and not the resulting film or the
formation of the heterojunction. The effect of low temperature (~180°C) air annealing on
the emission characteristics of CdS/CIGS thin films was studied by cryogenic infrared
and visible PL. Spectral shape was not significantly affected by annealing for either film,
but PL intensity did show some dependence on anneal time for both films, which led to
an estimate of an optimal time window of 3-10 hours for low temperature annealing.</dc:description>
          <dc:description>Item withdrawn by Mark Zulauf (zulauf@illinois.edu) on 2012-09-04T15:09:30Z
Item was in collections:
University of Illinois Theses &amp; Dissertations (ID: 1)
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          <dc:identifier>http://hdl.handle.net/2142/42271</dc:identifier>
          <dc:language>en</dc:language>
          <dc:rights>Copyright 2012 Damon Hebert</dc:rights>
          <dc:subject>solar cell</dc:subject>
          <dc:subject>copper indium gallium diselenide (CIGS)</dc:subject>
          <dc:subject>Cu(In,Ga)Se2</dc:subject>
          <dc:subject>photoluminescence</dc:subject>
          <dc:subject>cathodoluminescence</dc:subject>
          <dc:subject>thin film</dc:subject>
          <dc:subject>electron backscatter diffraction (EBSD)</dc:subject>
          <dc:subject>band tail</dc:subject>
          <dc:subject>grain boundary</dc:subject>
          <dc:subject>emission</dc:subject>
          <dc:subject>sodium</dc:subject>
          <dc:subject>anneal</dc:subject>
          <dc:subject>Cadmium sulfied (CdS)</dc:subject>
          <dc:title>Optical characterization of copper indium gallium diselenide thin films</dc:title>
          <dc:type>text</dc:type>
          <degree>
            <department>Materials Science &amp; Engineerng</department>
            <departmentCode>1919</departmentCode>
            <discipline>Materials Science &amp; Engr</discipline>
            <disciplineCode>0130</disciplineCode>
            <grantor>University of Illinois at Urbana-Champaign</grantor>
            <level>Dissertation</level>
            <name>Ph.D.</name>
            <program>PHD:Materials Sci &amp; Engr -UIUC</program>
            <programCode>10KS0130PHD</programCode>
          </degree>
        </thesis>
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