Mechanisms of glycine formation from aminoacetonitrile in space
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초록

The potential energy surfaces for the formation of glycine (Gly) or its precursors, such as Gly radical cation and deprotonated Gly, starting from aminoacetonitrile (NH2CH2CN) or deprotonated aminoacetonitrile were determined by CBS-QB3 calculation. The reaction of NH2CH2CN + H2O+ + H2O gave mainly unwanted products other than Gly or its precursors. The reactions of NHCH2CN + 2H(2)O, NH2CHCN + 2H(2)O, or NH2CH2CN + OH + H2O, led to Gly or its precursors as one of the main products. The overall activation barriers were 229 kJ mol(-1), 216 kJ mol(-1), and 118 kJ mol(-1), respectively. A barrierless pathway for the formation of Gly from the reaction of NH2CH2CN + OH + H2O with a catalytic H2O was found, strongly suggesting that Gly can be formed thermally from NH2CH2CN and OH on icy grain surfaces in the interstellar medium.

키워드

Potential EnergyQuantum ChemistryActivation BarriersCbs-qb3Grain SurfaceInterstellar MediasPotential-energy SurfacesRadical CationsAmino AcidsSET MODEL CHEMISTRYAMINO ACETONITRILEACETIC-ACIDGAS-PHASEAB-INITIOINTERSTELLARHCNRADICALSOH
제목
Mechanisms of glycine formation from aminoacetonitrile in space
저자
Choe, Joong Chul
DOI
10.1039/d3cp01155k
발행일
2023-06
유형
Article
저널명
Physical Chemistry Chemical Physics
25
23
페이지
16001 ~ 16008