Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/1336
Title: Dual-Mode Photoluminescence of Er<sup>3+</sup> -Doped Ta<inf>2</inf>O<inf>5</inf> Coatings Formed by Plasma Electrolytic Oxidation of Tantalum
Authors: Stojadinović, Stevan 
Ćirić, Aleksandar 
Keywords: Down-conversion;Er 3+;Er /Yb 3+ 3+;Photoluminescence;Plasma electrolytic oxidation;Up-conversion
Issue Date: 1-Jan-2023
Journal: Journal of Electronic Materials
Abstract: 
Orthorhombic Ta2O5:Er3+ coatings were obtained by plasma electrolytic oxidation (PEO) of tantalum in an alkaline electrolyte with the addition of Er2O3 particles in various concentrations. Down-conversion photoluminescence (PL) emission spectra is featured by sharp bands attributed to 4f–4f transitions of Er3+. The most intense green PL emission band centered at 544 nm is attributed to the 4S3/2 → 4I15/2 emission of Er3+. Population paths of the Er3+ down-conversion PL happen under resonant excitation conditions of the Er3+ from ground state 4I15/2 to higher levels, and via a broad violet charge transfer excitation band. Both excitation energy and Er content have an impact on the PL emission response in Ta2O5:Er3+ coatings. The 4I15/2 → 4G11/2 transition is the dominant excitation pathway for the PL emission of Er3+. Up-conversion PL spectra created after 980 nm irradiation of Ta2O5:Er3+ coatings have characteristic 4f–4f transitions of Er3+. The intensity of the green 4S3/2 → 4I15/2 is much higher compared to the red 4F9/2 → 4I15/2 emission of Er3+. Co-doping Ta2O5:Er3+ coatings with sensitizer Yb3+ ions increased the up-conversion emission PL intensity of Er3+ thanks to the efficient energy transfer from Yb3+ to Er3+. The red up-conversion PL intensity of 4F9/2 → 4I15/2 transition increases more rapidly with respect to green emission 4S3/2 → 4I15/2. A phonon-assisted energy back transfer process from Er3+ ions (4S3/2 → 4I13/2) to the neighboring Yb3+ ions (2F7/2 → 2F5/2) leads to enhanced red emission 4F9/2 → 4I15 and decreased green emission 4S3/2 → 4I15/2.
URI: https://physrep.ff.bg.ac.rs/handle/123456789/1336
ISSN: 03615235
DOI: 10.1007/s11664-023-10658-6
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