Time, temperature and concentration resolved Yb3+ luminescence study in co-sputtered Cu2-xGaxS2 (0.1 < x < 1.6) thin films with a Cu–Ga composition gradient

The broad class of Cu(Al,Ga,In) (S,Se,Te)2 solar absorber materials when doped with Yb3+ are interesting for thin film based luminescent solar concentrator (LSC's) application. In this work the strong and broad absorption properties of co-sputtered CuGaS2 (CGS) thin films combined with the lumi...

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Published inOptical materials Vol. 157; p. 116220
Main Authors Derksen, Max, Bergkamp, Sem, Kohnstamm, Olivia, van der Kolk, Erik
Format Journal Article
LanguageEnglish
Published Elsevier B.V 01.11.2024
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Online AccessGet full text
ISSN0925-3467
DOI10.1016/j.optmat.2024.116220

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Abstract The broad class of Cu(Al,Ga,In) (S,Se,Te)2 solar absorber materials when doped with Yb3+ are interesting for thin film based luminescent solar concentrator (LSC's) application. In this work the strong and broad absorption properties of co-sputtered CuGaS2 (CGS) thin films combined with the luminescent properties of Yb are reported. Energy-dispersive x-ray spectroscopy (EDS), x-ray diffraction, transmission, excitation, and temperature dependent emission as well as radiative lifetime measurements are performed on thin films with varying Cu:Ga ratios and Yb3+ concentrations. It is found that Yb3+ emission can be broadly sensitized by the host in the range of 200–600 nm. A lower Cu:Ga ratio, crystallinity and post annealing in air provides a positive impact on the sensitization of Yb3+ emission. The temperature dependent time integrated decay curves show a clear thermal energy barrier of about 0.2 eV. Because the exponential tail, with a lifetime of 110 μs, is constant with temperature, we conclude that the barrier is connected to the thermal release of electrons trapped at the Yb2+ ground state. The low energy transfer efficiency from the host to the Yb dopant is attributed to efficient non-radiative electron-hole pair recombination. The prospects and design criteria of Cu(Al,Ga,In) (S,Se,Te)2 solar absorber materials for LSC applications is the further subject of the discussion. [Display omitted] •CuGaS2 host sensitized Yb3+ emission in sputtered thin films have less than 0.01 % IQE.•Yb3+ ions excited in the 2F5/2 state are not thermally quenched up to 550 K.•Time- and temperature dependent CuGaS2 to Yb3+ energy transfer is reported.•Increased Ga/Cu ratio and O content boost Yb3+ intensity by 25 and 375, respectively.•The lifetime of Yb3+ in CuGaS2 is 110 μs.
AbstractList The broad class of Cu(Al,Ga,In) (S,Se,Te)2 solar absorber materials when doped with Yb3+ are interesting for thin film based luminescent solar concentrator (LSC's) application. In this work the strong and broad absorption properties of co-sputtered CuGaS2 (CGS) thin films combined with the luminescent properties of Yb are reported. Energy-dispersive x-ray spectroscopy (EDS), x-ray diffraction, transmission, excitation, and temperature dependent emission as well as radiative lifetime measurements are performed on thin films with varying Cu:Ga ratios and Yb3+ concentrations. It is found that Yb3+ emission can be broadly sensitized by the host in the range of 200–600 nm. A lower Cu:Ga ratio, crystallinity and post annealing in air provides a positive impact on the sensitization of Yb3+ emission. The temperature dependent time integrated decay curves show a clear thermal energy barrier of about 0.2 eV. Because the exponential tail, with a lifetime of 110 μs, is constant with temperature, we conclude that the barrier is connected to the thermal release of electrons trapped at the Yb2+ ground state. The low energy transfer efficiency from the host to the Yb dopant is attributed to efficient non-radiative electron-hole pair recombination. The prospects and design criteria of Cu(Al,Ga,In) (S,Se,Te)2 solar absorber materials for LSC applications is the further subject of the discussion. [Display omitted] •CuGaS2 host sensitized Yb3+ emission in sputtered thin films have less than 0.01 % IQE.•Yb3+ ions excited in the 2F5/2 state are not thermally quenched up to 550 K.•Time- and temperature dependent CuGaS2 to Yb3+ energy transfer is reported.•Increased Ga/Cu ratio and O content boost Yb3+ intensity by 25 and 375, respectively.•The lifetime of Yb3+ in CuGaS2 is 110 μs.
ArticleNumber 116220
Author Derksen, Max
van der Kolk, Erik
Bergkamp, Sem
Kohnstamm, Olivia
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  givenname: Max
  orcidid: 0009-0006-1917-9612
  surname: Derksen
  fullname: Derksen, Max
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  givenname: Sem
  surname: Bergkamp
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  email: sembergkamp@gmail.com
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  givenname: Olivia
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  email: oliviakohnstamm@gmail.com
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  givenname: Erik
  surname: van der Kolk
  fullname: van der Kolk, Erik
  email: E.vanderKolk@tudelft.nl
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Keywords Charge trapping mediated energy transfer
Host sensitized emission
Thin film luminescent solar concentrator
Combinatorial sputtering
CuGaS2:Yb3+ photoluminescence
Language English
License This is an open access article under the CC BY license.
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Snippet The broad class of Cu(Al,Ga,In) (S,Se,Te)2 solar absorber materials when doped with Yb3+ are interesting for thin film based luminescent solar concentrator...
SourceID crossref
elsevier
SourceType Index Database
Publisher
StartPage 116220
SubjectTerms Charge trapping mediated energy transfer
Combinatorial sputtering
CuGaS2:Yb3+ photoluminescence
Host sensitized emission
Thin film luminescent solar concentrator
Title Time, temperature and concentration resolved Yb3+ luminescence study in co-sputtered Cu2-xGaxS2 (0.1 < x < 1.6) thin films with a Cu–Ga composition gradient
URI https://dx.doi.org/10.1016/j.optmat.2024.116220
Volume 157
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