Isotopic substitution shifts in methane and vibrational band assignment in the 5560–6200 cm−1 region

https://doi.org/10.1016/j.jqsrt.2009年02月01日6 Get rights and content

Abstract

The absorption spectra of the 12CH4 and 13CH4 molecules have been recorded and assigned in the 5560–6200 cm−1 region. The effects of isotopic substitution for 12C by 13C on the methane vibrational energy levels have been calculated from an ab initio potential energy surface and compared with experiment. Comparison of the results obtained for two isotopic species allows us to confirm the vibrational assignment for the strongest bands of 12CH4 in this region. Good agreement of ab initio calculations with observed energy levels has been demonstrated. A list of the assigned 13CH4 lines valuable in atmospheric applications is reported.

Introduction

Numerous theoretical studies have been devoted to calculations of the methane vibrational energy levels [1], [2], [3], [4] and rovibrational energy levels [5]. The analysis of highly excited energy levels and transitions of the methane molecule is a difficult problem due to the complex structure of vibrational levels and the high dimensionality of the calculation models [6], [7], [8], [9]. Furthermore, the structure of vibrational levels for the tetradecade of methane in the 5300–6200 cm−1 region is still unclear. The results presented in Refs. [1], [2], [3] significantly differ from those obtained in Refs. [6], [8]. In present work, we compare the ab initio calculations with experiment and determine the structure of the methane vibrational energy levels more precisely. The energy levels in the 5800–6200 cm−1 region are very valuable for atmospheric applications, because this region covers the strongest band of the tetradecade 2ν3 (F2). But even the 2ν3 (F2) identification is questionable today [10]. Systematic identification of 13CH4 has been published only up to 3200 cm−1 [11], [12].
In this paper, the ab initio points calculated in Ref. [13] have been used to determine the 12CH4 and 13CH4 potential energy surface (PES) in the internal mass-dependent coordinates. The vibrational energy levels up to 6200 cm−1 have been calculated for both molecules. The technique used for calculations of energy levels is described in Ref. [13].
The 12CH4 and 13CH4 spectra have been recorded with high-resolution Fourier transform spectrometers (FTS) at the Toray Research Center Inc., Otsu, Japan. The spectra were recorded at different temperatures that allowed us to estimate the value of the lower rotational quantum number J for transitions with small J values. As a rule, the comparison of the strongest lines of 12CH4 and 13CH4 allowed us to establish a one-to-one correspondence between spectral lines of those molecules.
One of the main goals of the present research is to perform the vibrational assignment based on the calculated isotopic shifts. This is possible to realize for the strongest lines with small J values. A similar research of four lines of the 2ν3 (F2) band has been conducted in Ref. [14]. However, the complete identification of all lines in the considered region is not a goal of our research. It is questionable whether this problem can be resolved without the detailed modeling of an effective Hamiltonian.
This paper is composed of three sections. The first section provides a brief description of the technique used to calculate vibrational energy levels and isotopic shifts from an ab initio PES. The second section describes the experimental spectra. The assignments of the 12CH4 and 13CH4 spectra, as well as the comparison of the calculated isotopic shifts with experiment, are presented in the third section.

Section snippets

PES and energy level calculation

The GAUSSIAN 98 program [15] was used to perform the geometry optimization using the CCSD(T) method with the cc-pVQZ basis set. The internal electron correlation effect was not taken into account. The minimum energy −40.450888 h was reached at rithat is equal to re=1.0879031Å. Near the equilibrium geometry, the interbond angles qe=ArcCos(-13). To simplify the kinetic energy operator [16], the PES has been calculated using the internal mass-dependent coordinates [17]: ri=ri+dj=14rj,whered=-14

Experiment

The spectra of methane were recorded with two high-resolution FTS. The 12CH4 spectra were recorded with the Bruker IFS 120 HR spectrometer at the Toray Research Center Inc. The 13CH4 spectra were recorded with the Bruker IFS 125 HR spectrometer at the Toray Research Center Inc. The coolable gas cells with an 8.75 cm absorption path length and ZnSe windows were used in these measurements. In FTS, the CaF2 beam splitter, the InSb detector, and a tungsten halogen lamp as the light source were used.

Comparison of the 12CH4 and 13CH4 cold spectra (assignment of spectra)

The 2ν3 (F2) bands of the 12CH4 and 13CH4 molecules have been compared in Ref. [14]. One of the purposes of the present research is to verify the identification of the ν2+ν3+ν4 and ν1+ν3 bands. The ab initio calculations [1], [3] show a wide disagreement with assignment reported in Ref. [8]. An assumption that the identifications of the ν2+ν3+ν4 and ν1+ν3 bands reported in Ref. [8] are not correct was made in Ref. [4]. This assumption is based only on the ab initio calculations. A good

Conclusion

The spectra of the two most abundant isotopologues of the methane have been recorded and analyzed to confirm vibrational assignment of the 12CH4 energy levels. The spectral measurements were performed at different temperatures by means of high-resolution Fourier transform spectrometers. A comparison of the room and low temperature spectra allows us to make the J assignment of low rotational levels for observed lines of 12CH4 and 13CH4. The PES-based calculated vibrational energy levels of both

Acknowledgments

We are grateful for the support provided by the NIES GOSAT (Greenhouse Observing SATellite) project.
These studies were supported by the Russian Foundation for Basic Research (Russia) in the framework of the Grant no. 06-05-65010a. This investigation was made partly within the framework of the Program 2.10.1 "Optical Spectroscopy and Frequency Standards".
A.V.N. acknowledges Prof. J.-P. Champion and Drs. L.R. Brown and V. Boudon for continuous collaboration on the methane spectra studies.

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