B M McLaughlin and K L Bell 1989 J. Phys. B: At. Mol. Opt. Phys. 22 763 doi:10.1088/0953-4075/22/5/008
B M McLaughlin and K L Bell
Show affiliationsCross section calculations are carried out in the energy region 1-1024 keV to provide theoretical data on the Rydberg state formation processes H(1s)+H(1s) to H(ns,np,nd)+H( Sigma ) where n=3, 4, 5, 6, 7, 10, 12, 15, 18, 20, 22, 25, 30 and 40. The calculations are performed including electron exchange and comparisons are drawn with those carried out in the first Born approximation. Rate coefficients are evaluated from these cross sections, including those for Balmer- alpha production in the temperature range 3*102-107 K, suitable for applications in astronomy and astrophysics. At the lower temperatures, the rate coefficients should be treated with caution, because of the simplicity of the approximation used.
Issue 5 (14 March 1989)
B M McLaughlin and K L Bell 1989 J. Phys. B: At. Mol. Opt. Phys. 22 763
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