Published July 1, 2013 | Version v1
Journal article

QUANTUM CALCULATION OF INELASTIC CO COLLISIONS WITH H. I. ROTATIONAL QUENCHING OF LOW-LYING ROTATIONAL LEVELS

  • 1. Department of Physics and Astronomy and the Center for Simulational Physics, The University of Georgia, Athens, GA 30602 (United States)
  • 2. Department of Chemistry, University of Nevada Las Vegas, Las Vegas, NV 89154 (United States)
  • 3. Department of Physics, Penn State University, Berks Campus, Reading, PA 19610 (United States)
  • 4. Department of Chemistry, Emory University, Atlanta, GA 30322 (United States)

Description

New quantum scattering calculations for rotational deexcitation transitions of CO induced by H collisions using two CO-H potential energy surfaces (PESs) from Shepler et al. are reported. State-to-state rate coefficients are computed for temperatures ranging from 1 to 3000 K for CO(v = 0, j) deexcitation from j = 1 to 5 to all lower j' levels, with j being the rotational quantum number. Different resonance structures in the cross sections are attributed to the differences in the anisotropy and the long-range van der Waals well depths of the two PESs. These differences affect rate coefficients at low temperatures and give an indication of the uncertainty of the results. Significant discrepancies are found between the current rate coefficients and previous results computed using earlier potentials, while the current results satisfy expected propensity rules. Astrophysical applications to modeling far infrared and submillimeter observations are briefly discussed.

Availability note (English)

Available from http://dx.doi.org/10.1088/0004-637X/771/1/49

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
771
Journal Issue
1
Journal Page Range
[7 p.]
ISSN
0004-637X
CODEN
ASJOAB