Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...424..983s&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 424, no. 2, p. 983-987
Astronomy and Astrophysics
Astrophysics
32
Dissociation, Hydrogen Plasma, Hydrogen Recombinations, Mathematical Models, Molecular Interactions, Molecular Ions, Quantum Theory, Reaction Kinetics, Computerized Simulation, Ionization, Molecular Rotation, Plasma Temperature, Potential Energy
Scientific paper
The dissociative recombination rate coefficients of H2(+) molecular ions are calculated for temperatures up to 4000 K. Specific account has been taken of rotational effects and contribution of high dissociative molecular states within the multichannel quantum defect theory (MQDT). A large range of electronic and nuclear temperatures is considered, which allows the use of these data in a variety of astrophysical and laboratory hydrogen plasmas.
Dulieu Olivier
Giusti-Suzor Annick
Roueff Evelyne
Schneider I. F.
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