The radiative and photodissociative
properties of the
dicarbon
molecule, C2, in high-lying electronic states are of utmost
importance for modeling the photochemical processes that occur in
various astronomical environments. Despite extensive spectroscopic
studies in the last two centuries, the photodissociation properties
of C2 are still largely unknown, particularly for quantum
states in the vacuum ultraviolet (VUV) region. Here, the lifetimes
of C2 for each individual rovibrational level in the recently
identified 23Σg
– state
are measured for the first time using a VUV-pump–UV-probe photoionization
scheme. The lifetimes are found to be strongly dependent on the rotational
and vibrational quantum levels in the 23Σg
– state. The strongly rotationally dependent lifetimes
observed here indicate that the 23Σg
– state may mainly undergo a predissociation process
through couplings with nearby repulsive electronic states. The current
observation could have important applications in modeling the interstellar
medium and cometary comae.