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

60Citations
Citations of this article
15Readers
Mendeley users who have this article in their library.
Get full text

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.

Cite

CITATION STYLE

APA

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

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free