A&A 458, 331-337 (2006)
DOI: 10.1051/0004-6361:20065713
F. Lique^{1} - A. Spielfiedel^{1} - G. Dhont^{2} - N. Feautrier^{1}
1 - LERMA and UMR 8112 of CNRS, Observatoire de
Paris-Meudon, 92195 Meudon Cedex, France
2 -
Université du Littoral Côte d'opale, LPCA, 189A avenue Maurice Schumann, 59140 Dunkerque, France
Received 29 May 2006 / Accepted 13 July 2006
Abstract
Context. Over the next few years, ALMA and Herschel missions will perform high spatial and spectral resolution studies at infrared and sub-millimeter wavelengths. This will provide much greater detail about the composition and evolution of molecules in space. Modeling of the spectra will require accurate radiative and collisional rates for species of astrophysical interest.
Aims. We calculate ro-vibrational excitation rate coefficients of SO by He, useful for studies of high-temperature environments.
Methods. A new accurate three dimensional (3D) potential energy surface was calculated for the SO-He system which explicitly takes into account the r-dependence of the SO vibration as well as the R-distance and
angle which describe the relative position of the collision partners. The dynamics calculations were performed according to the VCC-IOS approximation.
Results. The new rate coefficients between the ro-vibrational levels are calculated for temperatures from 300 K to 800 K.
Key words: ISM: molecules - molecular data - molecular processes
Observations of molecular emission at millimeter and infrared wavelengths, supplemented by careful and detailed modeling, are powerful tools to investigate the physical and chemical conditions of astrophysical objects. First observed by Gottlieb & Ball (1973) in the interstellar gas, SO has been used extensively to study shocked molecular gas in various environments (Turner et al. 1992; van Dishoeck & Blake 1998; Blake et al. 1987). The modeling of the line intensities requires comparison with model excitation calculations using radiative as well as collisional rates. Collisional excitation in shocked regions and in photon dominated regions involves excitation of high-rotational levels as well as vibrational excitation by the most abundant species, He and H_{2}.
Rotational excitation rate coefficients for collisions among fine structure levels of SO with He atoms, based on an accurate ab initio potential energy surface (PES), have been calculated recently (Lique et al. 2005; Lique et al. 2006). For pure rotational excitation, the SO r-distance was kept at its equilibrium geometry for the calculation of the PES. In Lique et al. (2005) the sensitivity of the cross sections to different basis sets used in the calculation of the SO-He surface has been studied. In the present paper we focus on calculations of rate coefficients for the v=0-1 vibrational excitation by He. The potential energy surface was calculated for different SO r-distances in order to account for the vibration of SO. The same strategy of calculation of the surface for each SO r-distance as in Lique et al. (2005) was adopted here.
A full close coupling approach for the dynamics calculations is prohibitively expensive in computer time for heavy molecules when transitions among highly excited rovibrational levels are involved. We therefore used the vibrational close-coupling rotational infinite order sudden (VCC-IOS) method (Parker & Pack 1978; Goldflam et al. 1977a,b) to perform the calculations. Cross-sections among the 118 first rotational levels of v=0 and v=1 have been calculated for total energies up to 5000 cm^{-1}. After Boltzmann thermal average, they give rate coefficients up to 800 K.
The paper is organized as follows: Sect. 2 describes the ab initio calculation of the potential energy surface. Section 3 provides a rapid description of the theory and of the calculations. In Sect. 4 we present and discuss our results.
The present work uses a Jacobi coordinate system, in which r is the SO distance, R is the distance from the center of mass of SO to the He atom and is the angle between the two distance vectors ( : He adjacent to oxygen atom, : He adjacent to sulfur atom). The SO-He potential energy surface was calculated in the supermolecular approach based on the single and double excitation open-shell coupled cluster method with perturbative contributions of connected triple excitations (RCCSD(T)) computed as defined by Knowles et al. (1993, 2000). To check the validity of this mono-configurational method, we have performed calculations for the first triplet electronic states with the Multi-Configuration Self-Consistent-field (MCSCF) approach. For all investigated geometries, it was found that the weight of the dominant configuration in the ground electronic state of the SO-He complex was between 0.92 and 0.94 which justifies the choice of the RCCSD(T) approach. Calculations were performed for three SO r-distances (2.4, 2.8 and 3.3 bohr) and the same grid of R and values (R was assigned values from 4.0 bohr to 16.0 bohr by steps of 0.25 bohr, the angular grid was uniform with a 15 degree spacing from 0 to 180 degree) as described in Lique et al. (2005).The three atoms were described by the standard correlation consistent polarized valence quadruple zeta set of Woon & Dunning (1994) augmented by the (3s3p2d2f1g) bond functions optimized by Cybulski & Toczylowski (1999), placed at mid-distance between the SO centre-of-mass and He. In all calculations, the basis set superposition error (BSSE) is corrected at all geometries with the Boys & Bernardi (1970) counterpoise procedure. The PES calculations were performed with the MOLPRO 2002 package (MOLPRO 2002).
The fitting procedure described by Werner et al. (1988) for the CN-He system was adopted in order to obtain the
numerical expansion routine required to perform the dynamical calculations. The potential was fitted to the functional form:
(1) |
N equals the number of SO bond distances and the number of angles for which the potential has been calculated.
Table 1: Vibrational matrix elements ( ) used in the vibrational averaging of the interaction potential; was taken to be 2.8 bohr.
Figure 1: Contour plot of the matrix elements of the interaction potential for elastic scattering of He+SO as a function of R and . The energies are in cm^{-1} with a distance of 1.0 cm^{-1} between two adjacent contours, the zero of energy is taken as that of the He+SO asymptote. | |
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Figure 2: Contour plot of the matrix elements of the interaction potential for inelastic scattering of He+SO as a function of R and . The energies are in cm^{-1} with a distance of 0.1 cm^{-1} between two adjacent contours, the zero of energy is taken as that of the He+SO asymptote. | |
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Figure 3: Variation of the vibrationally elastic rotational cross sections for v=0 with the v=0 and v=1 basis set (full curve) and without vibrational coupling (diamonds). | |
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Figure 4: "Fundamental IOS cross sections'' (see Eq. (4)) for vibrationally elastic rotational excitation of SO out of the v=1, N=0 level to v=0, L level calculated including 2, 3 and 4 vibrational levels in the dynamical calculations. | |
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For a VCC-IOS calculation, matrix elements of the potential between the vibrational states of the SO molecule are required for fixed values of the Jacobi scattering angle and for all the R-values. We write these matrix elements as:
Contour plots of the and surfaces are respectively shown in Figs. 1 and 2. In these plots the value corresponds to colinear He-SO. The surface is indistinguishable from the surface. The global minimum in the V_{0,0} and V_{1,1} surfaces is found to be -34.62 cm^{-1} (R=7.35 bohr, = 180).
Table 2: Energy in cm^{-1} of the fine structure levels of SO (v=0) (E=0 cm^{-1} for v=0, N_{J}=1_{0}).
In the SO (
)
electronic ground state, the rotational levels are split by spin-rotation coupling. In the intermediate coupling scheme, the rotational wave function of SO can be written for
as:
Table 3: Energy in cm^{-1} of the fine structure levels of SO (v=1) (E=0 cm^{-1} for v=0, N_{J}=1_{0}).
The energies of the first fine structure levels pertaining to the v=0 and v=1 vibrational levels are given in Tables 2 and 3. They were computed with the experimental spectroscopic constants of Bogey et al. (1982). Due to the low rotational constant there are 118 N_{j} levels with an energy lower than the first excited vibrational level.
In the VCC-IOS method, the rotational levels are treated as degenerate. Within this approximation the problem reduces to the computation of vibrationally inelastic S-matrix elements calculated with a close coupling approach at fixed Jacobi angles for a given L-value. These fixed-angle S-matrix elements must then be mutiplied by the appropriate spherical harmonics and integrated over to give the "fundamental IOS cross sections'' out of the v, N=0 level.
In the Hund's case (b) limit, the de-excitation ro-vibrational cross sections are expressed in a reduced form in terms of the
cross sections (Corey & McCourt 1983):
Rate coefficients are obtained by averaging the appropriate cross sections over a Boltzmann distribution of velocities at a given kinetic temperature T:
(5) |
As the IOS approximation neglects the energy structure of the rotational levels, it is expected to be poor at low energies, so the results presented here refer to high temperatures. The validity of this approach was checked in Lique et al. (2006) for pure rotational excitation. It was found to be appropriate, especially for transitions involving levels with N > 5.
However it may not be so applicable to vibrational quenching as resonant vibrational energy transfer may occur. This type of near-resonant energy transfer has been observed experimentally (Stewart et al. 2000; McCaffery & Marsh 2000) and obtained theoretically (Stewart et al. 1988, 2000; Miklavc et al. 1992; Krems et al. 2001) for diatomic molecules with a small moment of inertia (H_{2}, HF, Li_{2}). Molecules with smaller rotational constants (CO for example) can exhibit resonant vibrational relaxation when they are initially in very high rotational levels. The role of near-resonant vibrational relaxation has been investigated systematically in CO (Krems 2002). This study shows that the contribution of this resonant process is negligible for low j levels and high energy, and only becomes important when the initial rotational state of v=1 is close in energy to high rotational states of v=0. These cases were not considered in this paper.
Figure 5: Temperature variation of the collision rates for: ( upper panel), ( medium panel), ( lower panel). | |
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In order to compute cross sections and rate coefficients for vibrational relaxation of SO, we have tested the convergence of the vibrational close-coupling expansion by including several vibrational wave functions in the basis set.
We first considered the effect of vibrational coupling on the rotational excitation cross sections. Figure 3 compares the fundamental IOS cross sections (see Eq. (4)) for vibrationally elastic rotational excitation of SO out of the v=0, N=0 level calculated with and without vibrational coupling between v=0 and v=1.
As already found for other systems like CO (Krems 2002) and HF (Krems & Nordholm 2001; Krems et al. 2001), the pure rotational transitions are unaffected by the vibrational channel included in the calculation. This result is directly the consequence of the very small non-diagonal vibrational matrix elements of the interaction potential compared to the diagonal ones. In addition, there is an excellent agreement between the cross sections calculated with the 3D PES and the one previously calculated (Lique et al. 2006) with the 2D PES. This result validates the choice of a 2D PES for pure rotational excitation.
We have also considered the convergence of the vibrational expansion on inelastic vibrational cross sections. Figure 4 shows the "fundamental IOS cross sections'' out of v=1, N=0 (see Eq. (4)) for vibrational v=0,1, v=0,1,2 and v=0,1,2, 3 basis sets.
Figure 6: Distribution of the final fine structure levels N'_{j'} in v'=0,n' identified by the number n' (given in Table 2 following vibrational relaxation of v=1, N_{j} states) at T=500 K. Upper panel is for N_{j} = 0_{1} (F_{1} level), middle panel is for N_{j} = 10_{10} (F_{2} level) and bottom panel is for N_{j} = 35_{34} (F_{3} level). | |
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It follows from this plot that the "fundamental IOS cross sections'' from v=1 can be obtained by neglecting coupling with vibrational states higher than v=1. Therefore, all the calculations presented in the following were performed with the v=0,1 basis set.
Calculations were performed for the 118 first fine structure levels of v=0 and v=1 and for energies up to 5000 cm^{-1} leading to converged rate coefficients for all the considered levels and temperatures up to 800 K. The temperature variation of the rate coefficients involving the first rotational levels are displayed in Fig. 5 for , for and for transitions.
One observes a slow variation with temperature of the vibrationally elastic rate coefficients when the variation of the vibrational excitation coefficients vary more rapidly. As found for other systems, the rate coefficients for transitions are lower than the elastic coefficients by several orders of magnitude. It would be necessary to consider much higher temperatures and/or high-j levels leading to near-resonant j-levels belonging to v=0 and v=1 to get much higher vibrational excitation rate coefficients. It is thus expected that the values obtained in the present VCC-IOS approximation for vibrational excitation and desexcitation give the correct order of magnitude of the rate coefficients.
Figure 6 presents diagrams of the distribution of the final rotational states v'=0, N'_{j'} (identified by the number n') after vibrational relaxation of various v=1, N_{j} states at a temperature of 500 K.
The vibrational relaxation of low j levels exhibits a first peak centered in the region of low j' levels and a second broad peak decreasing slowly for large j' levels. As the initial rotational excitation increases, the first peak becomes larger than the second one and shifts toward larger j' values. One can also observe in this figure a strong propensity for F-conserving transitions in the large j limit. This was already found in pure rotational cross sections and rate coefficients (Lique et al. 2005) and predicted theoretically (Alexander & Dagdigian 1988).
All the rate coefficients are available on our web site (http://amdpo.obspm.fr/basecol/).
Acknowledgements
The calculations of ab initio potential energy surfaces were performed on the parallel machine MPOPM of Paris Observatory, and the scattering calculations were performed at the IDRIS-CNRS center (Institut de Développement et des Ressources en Informatique Scientifique du Centre National de la Recherche Scientifique) under project 050883.