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Y.-J. Hsiao et al. / Journal of Alloys and Compounds 471 (2009) 259–262
tant role in the formation of these defect levels. In our experiment,
organic networks fiercely burnt out in a very short time, and this
process consumed a great amount of oxygen, which induced the
absence of oxygen sites and a great deal of oxygen vacancies [20].
In this way, the shifted absorption peak at 300nm may be caused by
the absorption of defect levels in nanosized CdNb2O6. The absorp-
tion edges were calculated according to the method reported by
Khan et al. [21]. Band-gap energy both was similar between 600
and 700 ◦C. The visible light absorption edge of 700 ◦C sample was
at 370 nm, which corresponded to the band-gap energy of 3.35 eV.
4. Conclusions
CdNb2O6 crystal was prepared by a sol–gel synthesis using
[Cd(NO3)2·6H2O] and NbCl5. The well-crystallized orthorhombic
CdNb2O6 can be obtained by heat-treatment at 600 ◦C from XRD.
The excitation wavelengths at a calcining temperature of 600 ◦C,
at about 272 and 330 nm, were associated with charge transfer
bands of [NbO6]7− and oxygen deficient niobate groups [NbO4]3−
.
Fig. 6. Absorption spectra of CdNb2O6 precursor powders annealed at 600 and
The PL spectra under 272 nm excitation show a broad and strong
blue emission peak at about 460 nm, originating from the niobate
octahedra group [NbO6]7−. The visible light absorption edge of the
700 ◦C sample was at 370 nm, which corresponded to the band-gap
energy of 3.35 eV.
700 ◦C for 3 h measured at room temperature.
transfer bands of [NbO6]7− and [NbO4]3− in the CdNb2O6 sys-
tem. The CdNb2O6 has an ordered columbite structure where the
pentavalent cations form pairs by face sharing of their coordina-
incomplete crystallization, and the departure of the Cd/Nb stoi-
chiometric ratio may generate various structural defects, such as
oxygen vacancies and Cd vacancies or interstitials. Therefore, the
concentration of extrinsic niobate groups (i.e., groups with an oxy-
gen deficiency or excess positive charge) [15,16] cannot be avoided.
Thus, the excitation bands at 330 nm, may be attributed to the
defects and impurities with different densities generated from
the extrinsic niobate groups (i.e., oxygen deficient niobate groups
[NbO4]3−).
The PL emission spectral wavelength distribution curves of
CdNb2O6 phosphors under 272 nm excitation at room temperature
are shown in Fig. 5b. The PL spectra show a broad and strong blue
emission peak at about 460 nm. Here, the edge-shared NbO6 groups
are efficient luminescent centers for the blue emission, which
may be ascribed to self-trapped exciton recombination [17]. This
Acknowledgement
The authors would like to thank the National Science Council of
Republic of China, Taiwan, for financially supporting this research
under contract no. NSC 96-2811-E-006-014.
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