Tokmachev Andrei M, Boggio-Pasqua Martial, Bearpark Michael J, Robb Michael A
Department of Chemistry, Imperial College London, London SW7 2AZ, United Kingdom.
J Phys Chem A. 2008 Oct 30;112(43):10881-6. doi: 10.1021/jp8044109. Epub 2008 Oct 3.
The photophysics of the pyrene radical cation, a polycyclic aromatic hydrocarbon (PAH) and a possible source of diffuse interstellar bands (DIBs), is investigated by means of hybrid molecular mechanics-valence bond (MMVB) force field and multiconfigurational CASSCF and CASPT2 ab initio methods. Potential energy surfaces of the first three electronic states D 0, D 1, and D 2 are calculated. MMVB geometry optimizations are carried out for the first time on a cationic system; the results show good agreement with CASSCF optimized structures, for minima and conical intersections, and errors in the energy gaps are no larger than those found in our previous studies of neutral systems. The presence of two easily accessible sloped D 1/D 2 and D 0/D 1 conical intersections suggests the pyrene radical cation is highly photostable, with ultrafast nonradiative decay back to the initial ground state geometry predicted via a mechanism similar to the one found in the naphthalene radical cation.
通过混合分子力学-价键(MMVB)力场以及多组态CASSCF和CASPT2从头算方法,研究了芘自由基阳离子(一种多环芳烃(PAH),可能是漫射星际带(DIBs)的来源)的光物理性质。计算了前三个电子态D0、D1和D2的势能面。首次对阳离子体系进行了MMVB几何优化;结果表明,对于极小值和锥形交叉点,其与CASSCF优化结构吻合良好,且能隙误差不大于我们之前对中性体系研究中发现的误差。两个易于接近的倾斜D1/D2和D0/D1锥形交叉点的存在表明芘自由基阳离子具有高度光稳定性,通过类似于萘自由基阳离子中发现的机制,预测其会通过超快非辐射衰变回到初始基态几何结构。