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Cross Sections for Photoionization from Valence-Electron States

Published online by Cambridge University Press:  03 August 2017

A. Burgess  and
M. J. Seaton
A. Burgess
Affiliation:
Department of Physics, University College, University of London, London, England
M. J. Seaton
Affiliation:
Department of Physics, University College, University of London, London, England

Extract

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In order to study recombination processes in gaseous nebulae, one requires the coefficients for radiative recombination to many excited states of neutral atoms and positive ions. These may be calculated as functions of electron temperature once the corresponding photoionization cross sections are known. For photoionization from valence-electron states a general formula has been obtained using a method which is an extension of that used by Bates and Damgaard for bound-bound transition probabilities.

Type
Part II: Theoretical Considerations on the Production and Dissipation of Velocity Fields in the Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 8: Cosmical Gas Dynamics , July 1958 , pp. 992 - 993
Copyright
Copyright © American Physical Society 1958 

References

1 Seaton, M. J., Monthly Notices Roy. Astron. Soc. 111, 368 (1951).Google Scholar

2 Bates, D. R. and Damgaard, A., Phil. Trans. Roy. Soc. London A242, 101 (1949).Google Scholar

3 Seaton, M. J., Compt. rend. 240, 1317 (1955); Proc. Phys. Soc. (London) A70, 620 (1957).Google Scholar

4 Ham, F. S., Solid State Physics , edited by Seitz, F. and Turnbull, D. (Academic Press, Inc., New York, 1955), Vol. 1, p. 127.Google Scholar