Mid-Infrared (MIR) Complex Refractive Index Spectra of Polycrystalline Copper-Nitride Films by IR-VASE Ellipsometry and Their FIB-SEM Porosity
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Márquez, E.Blanco, E.
Mánuel, J.M.
Ballester, M.
García-Gurrea, M.
Rodríguez-Tapiador, M.I.
Fernández, S.M.
Willomitzer, F.
Katsaggelos, A.K.
Affiliation
Wyant College of Optical Sciences, University of ArizonaIssue Date
2023-12-19
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Márquez, E.; Blanco, E.; Mánuel, J.M.; Ballester, M.; García-Gurrea, M.; Rodríguez-Tapiador, M.I.; Fernández, S.M.; Willomitzer, F.; Katsaggelos, A.K. Mid-Infrared Complex Refractive Index Spectra of Polycrystalline Copper-Nitride Films by IR-VASE Ellipsometry and Their FIB-SEM Porosity. Coatings 2024, 14, 5. https://doi.org/10.3390/coatings14010005Journal
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© 2023 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution license.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
Copper-nitride (Cu (Formula presented.) N) semiconductor material is attracting much attention as a potential, next-generation thin-film solar light absorber in solar cells. In this communication, polycrystalline covalent Cu (Formula presented.) N thin films were prepared using reactive-RF-magnetron-sputtering deposition, at room temperature, onto glass and silicon substrates. The very-broadband optical properties of the Cu (Formula presented.) N thin film layers were studied by UV-MIR (0.2–40 (Formula presented.) m) ellipsometry and optical transmission, to be able to achieve the goal of a low-cost absorber material to replace the conventional silicon. The reactive-RF-sputtered Cu (Formula presented.) N films were also investigated by focused ion beam scanning electron microscopy and both FTIR and Raman spectroscopies. The less dense layer was found to have a value of the static refractive index of 2.304, and the denser film had a value of 2.496. The iso-absorption gap, (Formula presented.), varied between approximately 1.3 and 1.8 eV and could be considered suitable as a solar light absorber. © 2023 by the authors.Note
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2079-6412Version
Final Published Versionae974a485f413a2113503eed53cd6c53
10.3390/coatings14010005
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Except where otherwise noted, this item's license is described as © 2023 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution license.