Original ArticlesGas-phase reactivity of SO+·: a selected ion flow tube study1
Introduction
Oxygen and sulfur are members of the select group of elements which are both cosmically abundant and disposed to forming chemical bonds (chiefly H, O, C, N, Mg, Si, Fe, and S, in decreasing order of solar abundance) [1]. Although sulfur is ranked below Mg, Si, and Fe in abundance, its participation in the ion/molecule chemistry of interstellar clouds is more extensive due to its higher first ionization energy (10.36 eV relative to <8.2 eV for Si, Fe, and Mg); thus, the atomic ions of H, O, C, N, S, and ions derived from these drive the bulk of synthetic gas phase ion/molecule chemistry which directs the chemical evolution of interstellar molecular clouds (ISC) [2], [3], [4]. Whereas atomic O+ does not persist in ISC due to its rapid reaction with H2 [5], [6], ground-state atomic S+ is unreactive with both H2 and CO [5], [6], the two major molecular constituents of ISC [2], [3], [4]. S+ in its ground 4S state is also unreactive with H2O [5], [6]. Sulfur and oxygen in the gas phase in ISC are thought to combine primarily by the ion/molecule reaction which has not yet been studied in the laboratory. Reaction (1) is expected to be particularly important for the synthesis of SO+· in cold, dark interstellar clouds, such as the Taurus Molecular Cloud (TMC-1) [7]. SO+· is one of the 14 sulfur-containing compounds and one of the 13 ions which have been detected in ISC [8].
The sulfur monoxide molecular ion, SO+·, itself reacts neither with H2 nor with CO [6], and thus a consideration of its reactivity with minority species in ISC is necessary. Turner has made the most extensive astrophysical searches for SO+· to date [7], [9], and has found this species to be abundant in a wide variety of interstellar sources [7]. His studies were motivated by the potential for SO+· to be a tracer for shocked regions of ISC [7]. In his simple model of SO+· chemistry in ISC, Turner considered electron/ion dissociative recombination to be the only important process that destroys SO+· [9]. His model assumed a recombination rate coefficient of αe(SO+·) = 2 × 10−7 [T(K)/300]−0.5 cm3 molecule−1 s−1 [9]; a plausible value, albeit one that has not yet been confirmed experimentally. No other destruction pathways for SO+· were considered, which necessitated the assumption of a high electron density (the so-called “high metal” value) to make the chemical model consistent with the observed SO+· column densities in many sources [9]. It is therefore important to investigate whether SO+· can be destroyed by numerous fast ion/molecule reactions with observed and expected interstellar molecules.
From a more fundamental standpoint, the reactivity of SO+· as compared with its isovalent “sister” species, S2+· and O2+·, is of considerable interest. The most important differences in reactivity among these three species are expected to stem from the essential electronic difference between the component atoms, S and O. The valence electrons of S are better shielded from the nuclear core potential than those of O, and hence, the promotion and ionization energies of electrons in molecular orbitals arising from S atoms are lower than in those arising from O atoms; for the same reason, the electronegativity of S (2.58, Pauling) is substantially lower than that of O (3.44, Pauling) [10]. In consequence, the recombination energies of S2+·, SO+·, and O2+· are 9.36, 10.29, and 12.07 eV, respectively [11], and hence, the capacity for exothermic reaction progresses steadily in the order S2+· < SO+· < O2+·. For reactions of such ions with polyatomic molecules, the prominence of charge (electron) transfer is also strongly correlated with the charge transfer exothermicity. This is because the high density of rovibronic states available in a polyatomic molecule permits a long-range charge transfer to occur with a high probability of favorable Franck-Condon factors. Here the probability of reaction essentially depends on the volume of phase space available to the reactants, and hence, on the reaction exothermicity. Such charge-transfer mechanisms in ion/molecule reactions have recently been reviewed [12].
As a consequence of the difference in electronegativity between S and O, SO+· is a highly polar species, with an electric dipole moment in the ground X 2Πr state of about 2.2 D [13]; the homonuclear S2+· and O2+· clearly lack permanent electric dipole moments. Although the overall collisional capture rates for the reactions of all three ions with neutral molecules will be dominated by the charge/permanent electric dipole and the charge/induced electric dipole interactions [14], the strong dipole of SO+· is likely to distinguish that ion from S2+· and O2+· with regard to the intimate reaction mechanisms and the kinds of products formed from the activated complex. Therefore, a comparative study of the reactivities of S2+·, SO+·, and O2+· will investigate the effects of recombination energy and charge separation on the rates and mechanisms of ion/molecule reactions.
Very few reactions of SO+· have been studied previously in the laboratory. The standard ion/molecule reaction databases [5], [6] list only eight such reactions, i.e., with H2, N, NH3, O2, H2S, CO, SO2, and SF6. Four of these, i.e., with H2, O2, CO, and SO2, do not proceed under standard conditions [6]. In contrast, many ion/molecule reactions of S2+· [5], [6], [15], [16], [17], [18] and O2+· [5], [6], [19], [20], [21], [22], [23], [24], [25] have been investigated, and hence are available for direct comparison with those of SO+·. In the present work, a selected ion flow tube (SIFT) has been used in the first systematic study of the ion/molecule reactions of SO+· with 16 organic molecules identified or likely to be present in ISC [8]: CH4, C2H6, C3H8, C2H2, C2H4, C3H4 (allene), n-C3H6, CH3OH, C2H5OH, CH3OCH3, OCS, CH2O, CH3CHO, CH3C(O)CH3, HCO2H, and HCO2CH3. For completeness of comparison, the reactions of S2+· with C2H2 and O2+· with CH4, C2H2, C3H4 (allene), n-C3H6, CH3OCH3, and HCO2H have also been investigated (of these, only the reactions of O2+ with CH4 and HCO2H have been studied previously under thermal conditions [5], [6], [20]). Rate coefficients and product distributions are presented for the reactions of all three ions with the 16 molecules, and the relative reactivities of S2+·, SO+·, and O2+· are discussed in light of these results. For SO+·, the reaction mechanisms, nature of the products formed, and implications for chemistry in ISC are also discussed.
Section snippets
Experimental
The SIFT technique has been described at length elsewhere [26]; the essentials are presented here, with emphasis on details particular to the present experiments. The SO+· ions were efficiently generated by two methods: (a) directly by impact of 70 eV electrons on SO2 in a low-pressure ion source (LPIS); and (b) by generation of S+ from 70 eV electron impact on CS2 in the same source, followed in the flow tube by where k2(2) = 1.8 × 10−11
Results and discussion
Rate coefficients, kexp(2), and fractional product distributions, f, for the reactions of SO+· and the supplementary reactions of S2+· and O2+· measured in the present study are presented in Table 1. Capture rate coefficients, kth(2), calculated from the parameterized variational “transition state” theory of Su and Chesnavich [37] are presented for comparison with the experimentally-determined rate coefficients. Electric dipole polarizabilities and electric dipole moments for these
Summary and conclusions
The reactions of the diatomic π-radical cation SO+· with 16 molecules representing examples of several classes of organic compound have been studied with a SIFT and compared with the reactions of S2+· and O2+· with the same species.
Reactions of SO+· are generally characterized by heterogenic bonding to form π-radical abstraction products such as HSO·/SOH·, HOSO·, CH3SO·, and CH3OSO·. Such products frequently appear in the ion product spectra in their protonated forms when the leaving partner
Acknowledgements
The National Science Foundation, Division of Astronomical Sciences, is gratefully acknowledged for funding this work under grant no. AST-9415485. The authors are extremely grateful to T. Daniel Crawford of the Center for Computational Quantum Chemistry at The University of Georgia for computing the dipole moment and Mulliken population of SO+·, as well as the enthalpies of formation of the various isomeric forms of H2SO+· using coupled cluster ab initio methods.
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Dedicated to the memory of Robert R. Squires.