The photodissociation dynamics of size-selected C-n(+) clusters with 1
9 less than or equal to n less than or equal to 29 is analysed using v
isible and UV irradiation. Both the number of absorbed photons leading
to dissociation, and the time decay of the associated internal energy
state are determined. The measured dissociation time constants indica
te an evaporative behaviour, where energy redistribution over the mode
s of vibration occurs before dissociation. The RRKM theory is therefor
e used and shown to lead to low dissociation energies. At the low leve
ls of internal energy reached in our photodissociation experiments, a
more appropriate model is proposed, which accounts for a restricted re
distribution of energy inside the cluster. This model leads to dissoci
ation energies ranging from 4.05 to 3.3 eV. One-photon dissociation is
also observed with photon energies close to 4.5 eV. On the one hand,
this suggests a dissociative process for this photo-excitation wavelen
gth. On the other hand, it allows to get upper limits for the dissocia
tion energies.