Glycine has been identified in several extraterrestrial environments, however, its detection in the interstellar medium remains elusive. Here, the authors investigate a catalytic pathway for glycine formation on silicate grains during relatively warm (> 150 K) stages of star formation using atomistic simulations, proposing a mechanism involving low-energy surface-stabilized intermediates that lead to spontaneous formation of glycine in a single-barrier exoergic process.
- Eric Mates-Torres
- Albert Rimola