Rovibrational transitions in OH due to collisions with He
POSTER
Abstract
In this work, we present scattering calculations for rovibrational transitions of OH(X2Π) induced by collisions with He in which fine-structure and Λ-doubling are incorporated dynamically. Rate coefficients for rotationally inelastic transitions of OH(v=0) induced by He have been computed previously for j≤11.5 [Klos et al., Chem. Phys. Lett, 445, 12 (2007)]. The present work extends previous calculations to include rates for vibrational de-excitation from OH(v=1,j). A quantum close-coupling method was used for selected j at temperatures between 1 and 500 K. The coupled-states approximation, which is less computationally intensive, was used for j=0.5-10.5 for temperatures between 1 and 3000 K; these rates were benchmarked against the close-coupling results.
The hydroxyl radical is a key species in the water chemistry of star-forming regions, and recent observations from the James Webb Space Telescope include spectra corresponding to the fundamental OH rovibrational band. The state-to-state rate coefficients presented here are needed to interpret spectra taken from non-local thermodynamic equilibrium (NLTE) environments.
The hydroxyl radical is a key species in the water chemistry of star-forming regions, and recent observations from the James Webb Space Telescope include spectra corresponding to the fundamental OH rovibrational band. The state-to-state rate coefficients presented here are needed to interpret spectra taken from non-local thermodynamic equilibrium (NLTE) environments.
*This work was supported by NASA grant 80NSSC21K1464 and NSF grant PHY-1806180.
Presenters
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T. J. Price
- Alvernia University