Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...430..435k&link_type=abstract
The Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 430, no. 1, p. 435-437
Astronomy and Astrophysics
Astrophysics
16
Atomic Collisions, Atomic Excitations, Charge Exchange, Electron Transfer, Hydrogen Ions, Ionic Collisions, Lithium, Particle Collisions, Protons, Radiative Transfer, Astronomical Models, Configuration Interaction, Interstellar Matter, Molecular Orbitals, Quantum Mechanics, Temperature Effects
Scientific paper
Charge transfer resulting from collisions of H(+) with Li is studied from 1 keV/u down to 10-5 eV/u. Excitation to Li* (2p) and charge transfer to H(n = 2) are found to be dominant above 10 eV. Below 10 eV, nonradiative charge transfer to H(1s) takes over, and at much lower energies radiative charge transfer/association becomes dominant. The rate coefficient for radiative charge transfer/association is on the order of10--17 cc/s with a slowly decreasing trend as the temeprature increases, while that for non-radiative charge transfer varies drastically from 10-20 cc/s at 100 K to 10-12 cc/s at 10,000 K.
Dutta C. M.
Kimura Masahiro
Shimakura N.
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