Momoh Paul O, Abrash Samuel A, Mabrouki Ridha, El-Shall M Samy
Department of Chemistry, Virginia Commonwealth University, Richmond, Virginia 23284-2006, USA.
J Am Chem Soc. 2006 Sep 27;128(38):12408-9. doi: 10.1021/ja064405g.
Since the discovery of acetylene and benzene in protoplanetary nebulae under powerful ultraviolet ionizing radiation, efforts have been made to investigate the polymerization of ionized acetylene. Here we report the efficient formation of benzene ions within gas-phase ionized acetylene clusters (C2H2)n+ with n = 3-60. The results from experiments, which use mass-selected ion mobility techniques, indicate that the (C2H2)3+ ion has unusual stability similar to that of the benzene cation; its primary fragment ions are similar to those reported from the benzene cation, and it has a collision cross section of 47.4 A2 in helium at 300 K, similar to the value of 47.9 A2 reported for the benzene cation. In other words, (C2H2)3+ structurally looks like benzene, it has stability similar to that of benzene, it fragments such as benzene, therefore, it must be benzene!
自从在强大的紫外线电离辐射下的原行星状星云里发现乙炔和苯以来,人们一直致力于研究电离乙炔的聚合反应。在此我们报告在气相电离乙炔簇(C2H2)n+(n = 3 - 60)中高效形成苯离子的情况。使用质量选择离子迁移技术的实验结果表明,(C2H2)3+离子具有与苯阳离子相似的异常稳定性;其主要碎片离子与苯阳离子所报道的相似,并且在300 K的氦气中它的碰撞截面为47.4 Å2,与报道的苯阳离子的47.9 Å2的值相似。换句话说,(C2H2)3+在结构上看起来像苯,它具有与苯相似的稳定性,它像苯一样碎片化,因此,它一定就是苯!