Luminescence properties of Yb-doped SrTiO: the significance of the oxygentitanium charge transfer state on photon downshifting
Ceramic powders of Sr 11.5 x Yb x TiO 3 ( x = 0.0, 0.0125, 0.025, 0.05 and 0.075) solid solutions were synthesized by the polymeric complex method. The crystal structure, microstructure and optical properties of the powders annealed at 800 C for 1 h were investigated by X-ray diffraction, scanning e...
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Veröffentlicht in: | Dalton transactions : an international journal of inorganic chemistry 2019-08, Vol.48 (31), p.11889-11896 |
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Zusammenfassung: | Ceramic powders of Sr
11.5
x
Yb
x
TiO
3
(
x
= 0.0, 0.0125, 0.025, 0.05 and 0.075) solid solutions were synthesized by the polymeric complex method. The crystal structure, microstructure and optical properties of the powders annealed at 800 C for 1 h were investigated by X-ray diffraction, scanning electron microscopy, and diffuse reflectance and photoluminescence spectroscopy, respectively. All the solid solutions exhibit a cubic perovskite-like structure. The reflectance spectra show a broadband below 400 nm ascribed to the ligand-to-metal charge transfer (LMCT) O
2
Ti
4+
fundamental state. The Yb
3+
(
em
= 980 nm) excitation spectra show a broadband being also compatible with the LMCT O
2
Ti
4+
state, indicating the energy transfer from the host to the Yb
3+
. The sample with
x
= 0.025 presents the highest emission intensity upon near UV excitation, which is further enhanced when the powder is treated under an oxygen-rich atmosphere. The luminescence quenching of Yb
3+
is explained as due to defects associated with O
2
and Sr
2+
vacancies. Finally, it is shown that the solid solutions may downshift photons from UV to wavelengths where a crystalline-silicon photovoltaic solar cell has a higher spectral responsivity.
Photon downshifting in SrTiO
3
:Yb
3+
to wavelengths where a PV cell has its higher spectral responsivity is achieved upon UV excitation through an energy transfer process from a ligand-to-metal-charge transfer O
2
Ti
4+
state to the Yb
3+
excited state. |
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ISSN: | 1477-9226 1477-9234 |
DOI: | 10.1039/c9dt01360a |