The trivalent lanthanide ions show
optical transitions between
energy levels within the 4f shell. All these transitions are formally
forbidden according to the quantum mechanical selection rules used
in molecular photophysics. Nevertheless, highly luminescent complexes
can be achieved, and terbium(III) and europium(III) ions are particularly
efficient emitters. This report started when an apparent lack of data
in the literature led us to revisit the fundamental photophysics of
europium(III). The photophysical properties of two complexes[Eu·DOTA(MeOH-d
4)]− and [Eu(MeOH-d
4)9]3+were investigated
in deuterated methanol at five different temperatures. Absorption
spectra showed decreased absorbance as the temperature was increased.
Luminescence spectra and time-resolved emission decay profiles showed
a decrease in intensity and lifetime as the temperature was increased.
Having corrected the emission spectra for the actual number of absorbed
photons and differences in the non-radiative pathways, the relative
emission probability was revealed. These were found to increase with
increasing temperature. The transition probability for luminescence
was shown to increase with temperature, while the transition probability
for light absorption decreased. The changes in transition probabilities
were correlated with a change in the symmetry of the absorber or emitter,
with an average increase in symmetry lowering absorbance and access
to more asymmetric structures increasing the emission rate constant.
Determining luminescence quantum yields and the Einstein coefficient
for spontaneous emission allowed us to conclude that lowering symmetry
increases both. Furthermore, it was found that collisional self-quenching
is an issue for lanthanide luminescence, when high concentrations
are used. Finally, detailed analysis revealed results that show the
so-called “Werts’ method” for calculating radiative
lifetimes and intrinsic quantum yields is based on assumptions that
do not hold for the two systems investigated here. We conclude that
we are lacking a good theoretical description of the intraconfigurational
f–f transitions, and that there are still aspects of fundamental
lanthanide photophysics to be explored.