Yang Zhenghai, Fujioka Kazuumi, Galimova Galiya R, Medvedkov Iakov A, Goettl Shane J, Sun Rui, Mebel Alexander M, Kaiser Ralf I
Department of Chemistry, University of Hawai'i at Manoa, Honolulu, Hawaii 96822, United States.
Department of Chemistry and Biochemistry, Florida International University, Miami, Florida 33199, United States.
ACS Cent Sci. 2025 Feb 4;11(2):322-330. doi: 10.1021/acscentsci.4c01606. eCollection 2025 Feb 26.
The azulene (CH) molecule, the simplest polycyclic aromatic hydrocarbon (PAH) carrying a fused seven- and five-membered ring, is regarded as a fundamental molecular building block of saddle-shaped carbonaceous nanostructures such as curved nanographenes in the interstellar medium. However, an understanding of the underlying gas-phase formation mechanisms of this nonbenzenoid 10π-Hückel aromatic molecule under low-temperature conditions is in its infancy. Here, by merging crossed molecular beam experiments with electronic structure calculations and molecular dynamics simulations, our investigations unravel an unconventional low-temperature, barrierless route to azulene via the reaction of the simplest organic radical, methylidyne (CH), with indene (CH) through ring expansion. This reaction might represent the initial step toward to the formation of saddle-shaped PAHs with seven-membered ring moieties in hydrocarbon-rich cold molecular clouds such as the Taurus Molecular Cloud-1 (TMC-1). These findings challenge conventional wisdom that molecular mass growth processes to nonplanar PAHs, especially those containing seven-membered rings, operate only at elevated pressure and high-temperature conditions, thus affording a versatile low-temperature route to contorted aromatics in our galaxy.
薁(CH)分子是最简单的带有稠合七元环和五元环的多环芳烃(PAH),被视为星际介质中马鞍形碳质纳米结构(如弯曲纳米石墨烯)的基本分子构建单元。然而,对于这种非苯型10π-休克尔芳香分子在低温条件下潜在的气相形成机制的理解仍处于起步阶段。在此,通过将交叉分子束实验与电子结构计算和分子动力学模拟相结合,我们的研究揭示了一条非常规的低温、无势垒途径,即通过最简单的有机自由基亚甲基(CH)与茚(CH)通过扩环反应生成薁。该反应可能是在富含烃类的冷分子云(如金牛座分子云-1(TMC-1))中形成带有七元环部分的马鞍形多环芳烃的初始步骤。这些发现挑战了传统观念,即非平面多环芳烃,尤其是那些含有七元环的分子质量增长过程仅在高压和高温条件下发生,从而为我们星系中扭曲芳烃提供了一条通用的低温途径。