Do the interstellar molecules CCCO and CCCS rearrange when energised?
Organic & Biomolecular Chemistry Pub Date : 02/27/2004 00:00:00 , DOI:10.1039/B316867K
Abstract

Neutrals CCCO, CC13CO, CCCS and CC13CS have been prepared by one-electron vertical (Franck–Condon) oxidation of the precursor anion radicals (CCCO)˙, (CC13CO)˙, (CCCS)˙ and (CC13CS)˙ respectively in collision cells of a reverse sector mass spectrometer. Ionisation of the neutrals to decomposing cations shows the neutrals to be stable for the microsecond duration of the neutralisation–ionisation (NR+) experiment. No rearrangement of the label in energised CC13CO or CC13CS occurs during these experiments. In contrast, minor rearrangement of (CC13CO)+˙ is observed [(CC13CO)+˙ → (OCC13C)+˙], while significant rearrangement occurs for (CC13CS)+˙ [(CC13CS)+˙ → (SCC13C)+˙]. Theoretical calculations at the CCSD(T)/aug-cc-pVDZ//B3LYP/6-31G(d) level of theory show that the cationic rearrangements occur by stepwise processes via key rhombic structures. Overall, the degenerate processes result in O and S migration from C-3 to C-1. The cations (CCCO)+˙ and (CCCS)+˙ require excess energies of ≥ 516 and ≥ 226 kJ mol−1 respectively to effect rearrangement.

Graphical abstract: Do the interstellar molecules CCCO and CCCS rearrange when energised?