Document Type
Article
Publication Date
7-31-2018
Publication Title
Astrophysical Journal
Volume
862
Issue
2
First page number:
1
Last page number:
8
Abstract
Rate coefficients for pure rotational quenching in H2(ν 1 = 0, j 1) + H2(ν 2 = 0, j 2) collisions from initial levels of j 1 = 2–31 (j 2 = 0 or 1) to all lower rotational levels are presented. We carried out extensive quantum mechanical close-coupling calculations based on a recently published H2–H2 potential energy surface (PES) developed by Patkowski et al. that has been demonstrated to be more reliable than previous work. Rotational transition cross sections with initial levels of j 1 = 2–14, 18, 19, 24, and 25 were computed for energies ranging from 10−6 to 1000 cm−1, while the coupled-states approximation was adopted from 2000 to 20,000 cm−1... See full text for full abstract.
Keywords
Molecular data; Molecular processes; Scattering
Disciplines
Astrophysics and Astronomy | Chemistry
File Format
File Size
1.197 Kb
Language
English
Repository Citation
Wan, Y.,
Yang, B. H.,
Stancil, P. C.,
Naduvalath, B.,
Parekh, N. J.,
Forrey, R. C.
(2018).
Collisional Quenching of Highly Excited H2 due to H2 Collisions.
Astrophysical Journal, 862(2),
1-8.
http://dx.doi.org/10.3847/1538-4357/aaccf8