07.01.2014 Views

CHEM01200604004 Shri Sanyasinaidu Boddu - Homi Bhabha ...

CHEM01200604004 Shri Sanyasinaidu Boddu - Homi Bhabha ...

CHEM01200604004 Shri Sanyasinaidu Boddu - Homi Bhabha ...

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

onds in the GaO 6 octahedra. Based on photoluminescence studies of a variety of gallium<br />

compounds containing GaO 6 octahedra [182, 198-201] the emission around 435 nm has been<br />

attributed to recombination of electrons trapped at oxygen vacancies and hole trapped at Ga 3+<br />

vacancies present in GaOOH. Peaks around 360 and 280 nm characterize corresponding<br />

excitation spectrum. UV-visible optical absorption studies [182] have revealed that GaOOH<br />

has an optical band gap of ~ 4.4 eV (~280 nm) and hence the excitation peak around 280 nm<br />

is assigned to the excitation of electron from valence band to conduction band of GaOOH.<br />

The other excitation peak around 360 nm is attributed to excitation of electrons from valence<br />

band to defect levels (oxygen vacancies) present in the lattice. Existence of energy transfer<br />

from hosts like Ga 2 O 3 to lanthanide ions is used as criteria to confirm the lanthanide ion<br />

incorporation in host. In order to find out whether lanthanide ions are incorporated in the<br />

GaOOH lattice, detailed luminescence experiments were carried out for lanthanide ions<br />

doped GaOOH samples and are described below.<br />

1.0<br />

excitation<br />

emission<br />

Normlised intensity<br />

0.8<br />

0.6<br />

0.4<br />

0.2<br />

0.0<br />

200 300 400 500 600<br />

Wavelength (nm)<br />

Fig.26. Emission spectrum obtained after 280 nm excitation and excitation spectrum<br />

corresponding to 435 nm emission from GaOOH nanorods prepared in the absence of<br />

any Eu 3+ ions.<br />

Figure 27 (right) shows the emission spectrum of GaOOH nanorods prepared in the<br />

presence of different concentrations of Eu 3+ ions. Peaks around 590 and 615 nm, which are<br />

due to the magnetic, characterize the emission spectrum and electric dipole allowed 5 D 0 → 7 F 1<br />

and 5 D 0 → 7 F 2 transitions, respectively of Eu 3+ ions. The emission spectrum is the same for all<br />

70

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!