Mahajan Tania B, Elsila Jamie E, Deamer David W, Zare Richard N
Department of Chemistry, Stanford University, Stanford, CA 94305-5080, USA.
Orig Life Evol Biosph. 2003 Feb;33(1):17-35. doi: 10.1023/a:1023996314942.
The reaction of polycyclic aromatic hydrocarbons (PAHs) with alkanes was examined in the presence of ultraviolet (UV) light under model prebiotic Earth and interstellar medium (ISM) conditions. We observed the formation of alkylated PAHs from a variety of PAHs and alkanes, which was caused by the absorption of UV light by the PAH molecule. Photoalkylation occurred in PAHs and alkanes in solution, in thin films in contact with simulated ocean water, and in matrices simulating ISM conditions. Photoalkylation occurred readily, with significant product yields within 5 h of irradiation. Because alkanes and PAHs are presumed to be part of the organic inventory in the ISM and on the early Earth, we propose that this photoalkylation reaction is a plausible pathway for the formation of carbon-carbon bonds in both these environments.
在模拟前生物地球和星际介质(ISM)条件下,于紫外线(UV)光照存在的情况下,对多环芳烃(PAHs)与烷烃的反应进行了研究。我们观察到多种PAHs和烷烃生成了烷基化PAHs,这是由PAH分子吸收紫外线所致。光烷基化反应发生在溶液中的PAHs和烷烃、与模拟海水接触的薄膜以及模拟ISM条件的基质中。光烷基化反应很容易发生,在照射5小时内就有可观的产物产率。由于烷烃和PAHs被认为是ISM和早期地球上有机物质存量的一部分,我们提出这种光烷基化反应是在这两种环境中形成碳 - 碳键的一种合理途径。