Collision-induced dissociation of molecular hydrogen in a rarefied gas

Details Collision-induced dissociation of molecular hydrogen in a rarefied gas Collision-induced dissociation of molecular hydrogen in a rarefied gas

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983sval....9..233i&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 9, July-Aug. 1983, p. 441-444) Soviet Astronomy Letters (ISSN 0360-0327), vol. 9, July-

Astronomy and Astrophysics

Astronomy

Gas Dissociation, Hydrogen Clouds, Interstellar Chemistry, Interstellar Gas, Molecular Collisions, Gas Cooling, Gas Density, High Temperature Gases, Reaction Kinetics, Vibrational Spectra

Scientific paper

The rate coefficient of the H2 + H to H + H + H reaction, including
dissociation from all the H2 vibrational levels, is calculated for
temperatures 1000-15000 K and particle densities n(H) = from 1 to 10 to
the 7th/cu cm. In rarefied gas with n(H) less than about 10,000/cu cm,
the low H2 vibrational levels will dominate the dissociation rate.

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