Synthesis and spectroscopic properties of Yb super(3+) and Tb super(3+) co-doped GdBO sub(3) materials showing down- and up-conversion luminescence

Gadolinium orthoborates doped with Yb super(3+) and Tb super(3+) ions were synthesised by the sol-gel Pechini method. Materials annealed at 900 degree C were composed of the monoclinic GdBO sub(3) phase with micrometre-sized crystals. The structural properties of the products were analysed by X-ray...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Dalton transactions : an international journal of inorganic chemistry 2015-02, Vol.44 (9), p.4063-4069
Hauptverfasser: Grzyb, Tomasz, Kubasiewicz, Konrad, Szczeszak, Agata, Lis, Stefan
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
Beschreibung
Zusammenfassung:Gadolinium orthoborates doped with Yb super(3+) and Tb super(3+) ions were synthesised by the sol-gel Pechini method. Materials annealed at 900 degree C were composed of the monoclinic GdBO sub(3) phase with micrometre-sized crystals. The structural properties of the products were analysed by X-ray diffraction (XRD) and transmission electron microscopy (TEM). The composition of the prepared materials was determined by inductively coupled plasma optical emission spectroscopy (ICP-OES). The materials showed intense ultraviolet (UV) or near infrared (NIR) excited green emission, which resulted from down- or up-conversion processes taking place in their structure. Spectroscopic properties were investigated on the basis of the measured excitation and emission spectra. Also, luminescence decays showing a short rise of emission with time after NIR excitation were measured. The dependence of the integral up-conversion intensity on the energy of the pumping laser was measured. The results indicated a two-photon process based on cooperative energy transfer (CET). The analysis of the synthesised series of samples allowed us to identify those with the best emission under a UV or NIR excitation source.
ISSN:1477-9226
1477-9234
DOI:10.1039/c4dt03667k