Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981phrva..24.1331c&link_type=abstract
Physical Review A - General Physics, 3rd Series, vol. 24, Sept. 1981, p. 1331-1341.
Astronomy and Astrophysics
Astrophysics
13
Atomic Collisions, Atomic Energy Levels, Charge Exchange, Hydrogen Atoms, Hydrogen Ions, Scattering Cross Sections, Sulfur, Astrophysics, Electron Scattering, Matrices (Mathematics), Potential Energy, Transition Probabilities
Scientific paper
Ab initio molecular-orbital methods were used to obtain potential-energy curves and coupling-matrix elements to determine the cross section for the charge transfer S(2+) (3P) + H(1s) yields S(+) + H(+) at electron-volt collision energies. Results of quantal coupled-channel calculations confirm the indications from the positions of the potential-energy curves that the cross section is quite small, i.e., less than about 10 to the -20th per sq cm at 1 eV.
Christensen R. B.
Watson William D.
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