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Exact(5)
The emission around 3.31 eV has been a controversial issue for a long time [21 23].
The emission around 430 nm is ascribed to the Mg acceptor levels in the p-GaN thin film.
In this case, the emission around 3.5 kHz would correspond to the chorus' upper band, and the one at 2 kHz to the lower band.
Similar results have been obtained for the second wafer containing the type II quantum wells grown on the InAs substrate designed for the emission around 6.2 μm.
In addition, because vacancy states lie deeper in the band gap than do the states arising from interstitial atoms in colloidal ZnS [38 40], the emission band of QD_ZnS_4 and QD_ZnS_5 identified at about 418 nm (2.97 eV) is due to transitions involving interstitial states, while the emission around 440 nm (2.82 eV) is assigned to vacancy states.
Similar(55)
It is found that the defect emission (around 490 nm) from ZnS is dramatically tailored by the presence of Au nanoparticles.
For longer excitation wavelengths, we observed a slight red shift of the emission maximum (around 520 nm at 825 nm excitation, see Fig. 9).
That would, in turn, have meant the emission of around 150m tonnes of CO2.
Therefore, it is reasonable to believe that the emission band around 370 nm arises from the ZnO clusters encapsulated in the channels of SBA-15.
As expected, the emission peaks around 550, 650, and 750 nm for samples A, B, and C closely match the peaks in the transmittance spectra in Figure 3.
In addition, it was noted that the emission peak around 465 nm also decreased gradually, revealing that the quality of AZO surface could be improved by the sensitization of CdS nanoparticles[51].
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