Large energy barriers prohibit the rearrangement of solitary acrylonitrile ions, CH 2 CHC N•+ , into their more stable hydrogen-shift isomers CH 2 C C NH•+ or CH CH-C NH •+ . This prompted us to examine if these isomerizations occur by self-catalysis in acrylonitrile dimer ions. Such ions, generated by chemical ionization experiments of acrylonitrile with an excess of carbon dioxide, undergo five dissociations in the s time frame, as witnessed by peaks at m/z 53, 54, 79, 80 and 105 in their metastable ion mass spectrum. Collision experiments on these product ions, deuterium labeling, and a detailed computational analysis using the CBS-QB3 model chemistry lead to the following conclusions: (i) the m/z 54 ions are ions CH 2 CHC NH + generated by self-protonation in ion-dipole stabilized hydrogen-bridged dimer ions [CH 2 CHC N· · ·H-C(C N)CH 2 ]•+
and [CH 2 CHC N· · ·H-C(H)C(H)C N]•+ ; the proton shifts in these ions are associated with a small reverse barrier; (ii) dissociation of the Hbridged ions into CH 2 C C NH•+ or CH CH-C NH •+ by self-catalysis is energetically feasible but kinetically improbable: experiment shows that the m/z 53 ions are CH 2 CHC N•+ ions, generated by back dissociation; (iii) the peaks at m/z 79, 80 and 105 correspond with the losses of HCN, C 2 H 2 and H• , respectively. The calculations indicate that these ions are generated from dimer ions that have adopted the (much more stable) covalently bound "head-to-tail" structure [CH 2 CHC N-C(H 2 )C(H)C N]•+ ; experiments indicate that the m/z 79 (C 5 H 5 N) and m/z 105 (C 6 H 6 N 2 ) ions have linear structures but the m/z 80 (C 4 H 4 N 2 ) ions consist of ionized pyrimidine in admixture with its stable pyrimidine-2-ylidene isomer. Acrylonitrile is a confirmed species in interstellar space and our study provides experimental and computational evidence that its dimer radical cation yields the ionized prebiotic pyrimidine molecule.