Zhao Long, Prendergast Matthew B, Kaiser Ralf I, Xu Bo, Ablikim Utuq, Ahmed Musahid, Sun Bing-Jian, Chen Yue-Lin, Chang Agnes H H, Mohamed Rana K, Fischer Felix R
Department of Chemistry, University of Hawaii at Manoa, Honolulu, Hawaii, 96822, USA.
Chemical Sciences Division, Lawrence Berkeley National Laboratory, Berkeley, CA, 94720, USA.
Angew Chem Int Ed Engl. 2019 Nov 25;58(48):17442-17450. doi: 10.1002/anie.201909876. Epub 2019 Oct 16.
Polycyclic aromatic hydrocarbons (PAHs) represent the link between resonance-stabilized free radicals and carbonaceous nanoparticles generated in incomplete combustion processes and in circumstellar envelopes of carbon rich asymptotic giant branch (AGB) stars. Although these PAHs resemble building blocks of complex carbonaceous nanostructures, their fundamental formation mechanisms have remained elusive. By exploring these reaction mechanisms of the phenyl radical with biphenyl/naphthalene theoretically and experimentally, we provide compelling evidence on a novel phenyl-addition/dehydrocyclization (PAC) pathway leading to prototype PAHs: triphenylene and fluoranthene. PAC operates efficiently at high temperatures leading through rapid molecular mass growth processes to complex aromatic structures, which are difficult to synthesize by traditional pathways such as hydrogen-abstraction/acetylene-addition. The elucidation of the fundamental reactions leading to PAHs is necessary to facilitate an understanding of the origin and evolution of the molecular universe and of carbon in our galaxy.
多环芳烃(PAHs)是共振稳定自由基与不完全燃烧过程以及富含碳的渐近巨星分支(AGB)恒星的星周包层中产生的碳质纳米颗粒之间的联系。尽管这些多环芳烃类似于复杂碳质纳米结构的构建块,但其基本形成机制仍然难以捉摸。通过理论和实验探索苯基自由基与联苯/萘的这些反应机制,我们为通向原型多环芳烃:三亚苯和荧蒽的新型苯基加成/脱氢环化(PAC)途径提供了令人信服的证据。PAC在高温下高效运行,通过快速的分子质量增长过程形成复杂的芳香结构,而这些结构很难通过传统途径如氢提取/乙炔加成来合成。阐明导致多环芳烃的基本反应对于促进理解分子宇宙和我们星系中碳的起源与演化是必要 的。