The C carbon cluster is found in a large variety of environments including flames, electric discharges, and astrophysical media. Due to spin-selection rules, assessing a complete overview of the dense vibronic landscape of the C cation starting from the ground electronic state X Σg+1 of the neutral is not possible, especially since the C ground state is of X Σg-4 symmetry. In this work, a flow-tube reactor source is employed to generate the neutral C in a mixture of both the lowest singlet X Σg+1 and triplet a Π electronic states. We have investigated the vibronic transitions in the vicinity of the first adiabatic ionization potential via one-photon ionization with vacuum ultraviolet synchrotron radiation coupled with electron/ion double imaging techniques. Using ab initio calculations and Franck-Condon simulations, three electronic transitions are identified and their adiabatic ionization energy is determined E(a  Π←X Σ )=12.440(10) eV, E(X  Σ ←a Π)=11.795(10) eV, and E(aΠ ← aΠ) = 12.361(10) eV. From the three origin bands, the following energy differences are extracted: ΔE(a - X) = 0.079(10) eV and ΔE(a - X) = 0.567(10) eV. The adiabatic ionization potential corresponding to the forbidden one-photon transition X ← X is derived and amounts to 11.873(10) eV, in very good agreement with the most recent measurement by Krechkivska et al. [J. Chem. Phys. 144, 144305 (2016)]. The enthalpy of formation of the doublet ground state C cation in the gas phase is determined at 0 K, ΔH(0K)(C (Πu2))=2019.9(10) kJ mol. In addition, we report the first experimental ion yield of C for which only a simple estimate was used up to now in the photochemistry models of astrophysical media due to the lack of experimental data.

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http://dx.doi.org/10.1063/1.5139309DOI Listing

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