Electronic structure calculations have been carried out for one of the key reactions in a Strecker synthesisroute to the a
mino acid glycine, in connection with a
mino acid production in the interstellar
mediu
m (ISM).Density functional calculations at the B3LYP/6-31+G(d,p) level have been perfor
med for the reaction between
methani
mine, CH
2NH, and the two iso
mers HNC/HCN, leading to a
minoacetonitrile-a known precursor ofglycine-in both the gas phase and on a
model icy grain surface. Three
mechanis
ms are evidenced in thereference gas-phase calculations; for CH
2NH reacting with HCN, there are two routes referred to as indirectand direct, and for CH
2NH reacting with the iso
mer HNC, a one-step
mechanis
m is found. All of thesereaction paths have quite high barriers, but on a
model interstellar grain icy surface, very considerable barrierreduction results due to a concerted proton relay
mechanis
m. Explicit water
molecules in a reaction ring areshown to participate in this relay
mechanis
m in the reactions of CH
2NH both with HCN and with the HNCiso
mer. The inclusion of two explicit H
2O
molecules leads to the strongest effect for the concerted protontransfer. With several further solvating waters included, this proton relay route to a
minoacetonitrile for theHNC iso
mer via a direct
mechanis
m is found to have a very low free-energy barrier at 50 K,
mages/gifchars/Delta.gif" BORDER=0 >
G50K < 1kcal/
mol, and thus appears to be feasible in the ISM. The corresponding reaction with HCN, however, has a
much higher barrier,
mages/gifchars/Delta.gif" BORDER=0 >
G50K = 7 kcal/
mol. The significance of these results for glycine production in the ISMis discussed.