School of Chemistry, University of Southampton, Highfield, Southampton SO17 1BJ, UK.
Chemistry. 2012 Sep 24;18(39):12411-23. doi: 10.1002/chem.201200848. Epub 2012 Aug 21.
CH(2)OO, the simplest Criegee intermediate, and ozone are isoelectronic. They both play very important roles in atmospheric chemistry. Whilst extensive experimental studies have been made on ozone, there were no direct gas-phase studies on CH(2)OO until very recently when its photoionization spectrum was recorded and kinetics studies were made of some reactions of CH(2)OO with a number of molecules of atmospheric importance, using photoionization mass spectrometry to monitor CH(2)OO. In order to encourage more direct studies on CH(2)OO and other Criegee intermediates, the electronic and photoelectron spectra of CH(2)OO have been simulated using high level electronic structure calculations and Franck-Condon factor calculations, and the results are presented here. Adiabatic and vertical excitation energies of CH(2)OO were calculated with TDDFT, EOM-CCSD, and CASSCF methods. Also, DFT, QCISD and CASSCF calculations were performed on neutral and low-lying ionic states, with single energy calculations being carried out at higher levels to obtain more reliable ionization energies. The results show that the most intense band in the electronic spectrum of CH(2) OO corresponds to the B(1)A' ← X(1)A' absorption. It is a broad band in the region 250-450 nm showing extensive structure in vibrational modes involving O-O stretching and C-O-O bending. Evidence is presented to show that the electronic absorption spectrum of CH(2)OO has probably been recorded in earlier work, albeit at low resolution. We suggest that CH(2)OO was prepared in this earlier work from the reaction of CH(2)I with O(2) and that the assignment of the observed spectrum solely to CH(2)IOO is incorrect. The low ionization energy region of the photoelectron spectrum of CH(2)OO consists of two overlapping vibrationally structured bands corresponding to one-electron ionizations from the highest two occupied molecular orbitals of the neutral molecule. In each case, the adiabatic component is the most intense and the adiabatic ionization energies of these bands are expected to be very close, at 9.971 and 9.974 eV at the highest level of theory used.
CH(2)OO,最简单的 Criegee 中间体和臭氧是等电子体。它们在大气化学中都起着非常重要的作用。虽然对臭氧进行了广泛的实验研究,但直到最近才对 CH(2)OO 进行了直接的气相研究,当时记录了它的光致电离光谱,并使用光致电离质谱法对 CH(2)OO 与一些具有大气重要性的分子的一些反应进行了动力学研究,以监测 CH(2)OO。为了鼓励对 CH(2)OO 和其他 Criegee 中间体进行更多的直接研究,使用高水准的电子结构计算和 Franck-Condon 因子计算模拟了 CH(2)OO 的电子和光电子光谱,并在此处呈现结果。使用 TDDFT、EOM-CCSD 和 CASSCF 方法计算了 CH(2)OO 的绝热和垂直激发能。此外,还对中性和低能离子态进行了 DFT、QCISD 和 CASSCF 计算,在更高水准上进行了单点能计算,以获得更可靠的电离能。结果表明,CH(2) OO 电子光谱中最强烈的带对应于 B(1)A' ← X(1)A' 吸收。它是一个在 250-450nm 区域的宽带,显示出涉及 O-O 伸缩和 C-O-O 弯曲的振动模式中的广泛结构。有证据表明,CH(2)OO 的电子吸收光谱可能已在早期工作中记录,尽管分辨率较低。我们建议,在早期工作中,CH(2)OO 是由 CH(2)I 与 O(2) 反应制备的,并且观察到的光谱仅归因于 CH(2)IOO 是不正确的。CH(2)OO 光电子光谱的低电离能区域由两个重叠的振动结构带组成,对应于中性分子中最高两个占据分子轨道的单电子电离。在每种情况下,绝热分量是最强的,这些带的绝热电离能预计非常接近,在使用的最高水准理论上为 9.971 和 9.974eV。