“…It has often been believed that surface OH groups are responsible for the blue PL emission observed in many different types of oxides. ,,,,,,, However, the simple OH-based model cannot be accepted without reservations because of the following reasons. First, the OH groups both in free and hydrogen-bonded states do not practically absorb light in the wavelength region longer than ∼300 nm, − whereas the blue PL emission occurs most effectively by using ∼330 to ∼360 nm light for excitation. − ,− Second, the blue PL output is normally enhanced after appropriate thermal annealing at ∼300 to ∼600 °C, and annealing at higher temperatures ( T ≳ 600 °C) almost eliminates the blue PL emission. ,− However, free and/or H-bonded OH groups at the surface of oxides do not exhibit the corresponding annealing temperature dependence; − rather, a large number of residual OH groups are still present up to ∼800 °C at the surface of alumina, silica, − and magnesia . It is hence probable that the blue PL emission does not result simply from the surface OH groups as they are but from certain relevant emissive defects, although the true structural origin of the emission center is not unambiguously identified at present. ,, …”