title: Highly accurate potential energy surface, dipole moment surface, rovibrational energy levels, and infrared line list for ³²S¹⁶O₂ up to 8000 cm⁻¹.
abstract: A purely ab initio potential energy surface (PES) was refined with selected (32)S(16)O2 HITRAN data. Compared to HITRAN, the root-mean-squares error (σ(RMS)) for all J = 0-80 rovibrational energy levels computed on the refined PES (denoted Ames-1) is 0.013 cm(-1). Combined with a CCSD(T)/aug-cc-pV(Q+d)Z dipole moment surface (DMS), an infrared (IR) line list (denoted Ames-296K) has been computed at 296 K and covers up to 8000 cm(-1). Compared to the HITRAN and CDMS databases, the intensity agreement for most vibrational bands is better than 85%-90%. Our predictions for (34)S(16)O2 band origins, higher energy (32)S(16)O2 band origins and missing (32)S(16)O2 IR bands have been verified by most recent experiments and available HITRAN data. We conclude that the Ames-1 PES is able to predict (32/34)S(16)O2 band origins below 5500 cm(-1) with 0.01-0.03 cm(-1) uncertainties, and the Ames-296K line list provides continuous, reliable and accurate IR simulations. The K(a)-dependence of both line position and line intensity errors is discussed. The line list will greatly facilitate SO2 IR spectral experimental analysis, as well as elimination of SO2 lines in high-resolution astronomical observations.
authors.affiliation: SETI Institute, 189 Bernardo Ave, Suite #100, Mountain View, California 94043, USA.
authors.forename: Xinchuan
authors.initials: X
authors.lastname: Huang
authors.affiliation: MS T27B-1, NAS Facility, NASA Ames Research Center, Moffett Field, California 94035, USA.
authors.forename: David W
authors.initials: DW
authors.lastname: Schwenke
authors.affiliation: MS 245-1, Space Science and Astrobiology Division, NASA Ames Research Center, Moffett Field, California 94035, USA.
authors.forename: Timothy J
authors.initials: TJ
authors.lastname: Lee