Abstract
The authors report a global potential energy surface for the ground electronic state of H O2 (X̃ A″2), which improves upon the XXZLG potential [Xu and, J. Chem. Phys. 122, 244305 (2005)] with additional high-level ab initio points for the long-range interaction potential in the O+OH channel. Exact J=0 quantum mechanical reaction probabilities were calculated on the new potential and the rate constant for the title reaction was obtained using a J -shifting method. The calculated rate constant is in good agreement with available experimental values and our results predict a significantly lower rate at temperature range below 30 K, offering a possible explanation for the "interstellar oxygen problem." © 2007 American Institute of Physics.
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CITATION STYLE
Xu, C., Xie, D., Honvault, P., Lin, S. Y., & Guo, H. (2007). Rate constant for OH (Π2) +O (P3) →h (S2) + O2 (g-3) reaction on an improved ab initio potential energy surface and implications for the interstellar oxygen problem. Journal of Chemical Physics, 127(2). https://doi.org/10.1063/1.2753484
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