Abstract
8 pags., 4 figs., 4 tabs.
Spectroscopic and structural properties of methoxymethyl radical (CH3OCH2, RDME) are determined using explicitly correlated ab initio methods. This radical of astrophysical and atmospheric relevance has not been fully characterized at low temperatures, which has delayed astrophysical research. We provide rovibrational parameters, excitations to the low energy electronic states, torsional and inversion barriers, and low vibrational energy levels. In the electronic ground state (X2A), which appears “clean” from nonadiabatic effects, the minimum energy structure is an asymmetric geometry whose rotational constants and dipole moment have been determined to be A0 = 46 718.67 MHz, B0 = 10 748.42 MHz, and C0 = 9272.51 MHz, and 1.432D (μA = 0.695D, µB = 1.215D, µC = 0.302D), respectively. A variational procedure has been applied to determine torsion-inversion energy levels. Each level splits into 3 subcomponents (A1/A2 and E) corresponding to the three methyl torsion minima. Although the potential energy surface presents 12 minima, at low temperatures, the infrared band shapes correspond to a surface with only three minima because the top of the inversion Vα barrier at α = 0° (109 cm−1) stands below the zero point vibrational energy and the CH2 torsional barrier is relatively high (∼2000 cm−1). The methyl torsion barrier was computed to be ∼500 cm−1 and produces a splitting of 0.01 cm−1 of the ground vibrational state.
This research was supported by the FIS2016-76418-P project
of the “Ministerio de Ciencia, Innovación y Universidades” of
Spain and the CSIC i-coop 2018 programme No COOPB20364.
The authors acknowledge the COST Actions CM1401 “Our Astrochemical History” and CM1405 “MOLIM.” The calculations have
been performed in the CESGA and CTI-CSIC computer centers. M.C. also acknowledges the financial support from the Consejería de Conocimiento, Investigación y Universidad, Junta de
Andalucía, and European Regional Development Fund (ERDF), ref. SOMM17/6105/UGR.