Department of Chemistry, Dongguk University-Seoul, Seoul, Korea.
Astrobiology. 2013 May;13(5):465-75. doi: 10.1089/ast.2013.0973. Epub 2013 May 9.
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.
我们通过 CBS-QB3 计算探索了通过 HCN 或 HNC 的齐聚物合成腺嘌呤的势能面。通过连续添加 HCN 或 HNC,已经获得了形成共价键合的 HCN 二聚体、三聚体、四聚体和五聚体(腺嘌呤)的途径。各个齐聚化阶段的活化能为每摩尔几百千焦耳,这阻止了星际空间或泰坦大气中腺嘌呤的有效合成。另一方面,当齐聚物从 HCNH(+)开始时,连续 HCN 或 HNC 添加的活化能显著降低。动力学分析结果表明,即使在后者条件下一些齐聚化阶段可以发生,质子催化的齐聚化也不能有效地在星际空间或泰坦大气中合成腺嘌呤。