Mechanisms of Prebiotic Adenine Synthesis from HCN by Oligomerization in the Gas Phase
- Authors
- Jung, Sun Hwa; Choe, Joong Chul
- Issue Date
- May-2013
- Publisher
- MARY ANN LIEBERT, INC
- Keywords
- Prebiotic chemistry; Astrobiology; Chemical evolution; Titan; ISM chemistry
- Citation
- ASTROBIOLOGY, v.13, no.5, pp 465 - 475
- Pages
- 11
- Indexed
- SCIE
SCOPUS
- Journal Title
- ASTROBIOLOGY
- Volume
- 13
- Number
- 5
- Start Page
- 465
- End Page
- 475
- URI
- https://scholarworks.dongguk.edu/handle/sw.dongguk/23660
- DOI
- 10.1089/ast.2013.0973
- ISSN
- 1531-1074
1557-8070
- Abstract
- We explored the potential energy surfaces for adenine synthesis by oligomerizations of HCN or HNC from CBS-QB3 calculations. The pathways have been obtained for the formation of the covalently bound HCN dimer, trimer, tetramer, and pentamer (adenine) by sequential additions of HCN or HNC. The activation energies of the individual oligomerization stages are a few hundred kilojoules per mole, which prevent efficient adenine synthesis in interstellar space or in the atmosphere of Titan. On the other hand, when the oligomerizations start from HCNH+, the activation energies of sequential HCN or HNC additions are significantly reduced. Kinetic analyses results suggest that adenine synthesis by proton-catalyzed oligomerizations cannot occur efficiently in interstellar space or in the atmosphere of Titan, even though some oligomerization stages can occur under the latter condition.
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Collections - College of Natural Science > Department of Chemistry > 1. Journal Articles

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