Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-27T00:24:14.664Z Has data issue: false hasContentIssue false
  • English
  • Français

Some Methods of Estimating the Successive Ionisation Potentials of any Element

Published online by Cambridge University Press:  24 October 2008

D. R. Hartree
D. R. Hartree
Affiliation:
St John's College
Get access Rights & Permissions [Opens in a new window]

Extract

On certain assumptions as to the quantum numbers of the normal orbits of the successive electrons captured by an atom, the successive ionisation potentials can be estimated by making use of the relations between terms of the same quantum number for different atoms of the same electronic structure. Formulae for several of the successive ionisation potentials are given, the form of the formulae being suggested by theoretical reasoning and numerical values of the constants determined from known spectra; the successive ionisation potentials of O, Fe and Ag, calculated from these formulae, are tabulated. It is pointed out how far different these ionisation potentials are from the X-ray excitation potential of the same orbit of a neutral atom.

Type
Research Article
Information
Mathematical Proceedings of the Cambridge Philosophical Society , Volume 22 , Issue 3 , 20 September 1924 , pp. 464 - 474
Copyright
Copyright © Cambridge Philosophical Society 1924

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

(1)Lyman, T., Nature, vol. 110, p. 278 (1922).CrossRefGoogle Scholar
(2)Hartree, D. R., Proc. Camb. Phil. Soc. vol. 22, p. 409 (1924).CrossRefGoogle Scholar
(3) These values are quoted from rough provisional analyses of the respective spectra by the writer, which are unpublished.Google Scholar
(4) Deduced from stellar absorption spectra, see Fowler, B. H. and Milne, E. A., Monthly Notices, R.A.S., vol. 84, p. 499 (1924). See also C. H. Payne, Harvard Coll. Obs., Circular 256 (1924).CrossRefGoogle Scholar
(5)Fowler, A., Proc. Roy. Soc., vol. 105, p. 299 (1924).Google Scholar
(6)Hopfield, J. J., Phys. Rev., vol. 22, p. 523 (1923).Google Scholar
(7)Hertz, G., Proc. Kon. Akad. Amst., vol. 25, p. 442 (1923).Google Scholar
(8)Fowler, A., Report on Series in Line Spectra.Google Scholar
(9)Paschen, F., Ann. der Phys., vol. 71, p. 537 (1923).CrossRefGoogle Scholar
(10)Fowler, A., Bakerian Lecture, 1924.Google Scholar
(11)Giesler, H. and Grotrian, W., Zeit. fur Phys., vol. 25, p. 165 (1924).CrossRefGoogle Scholar
(12) See text of this paper.Google Scholar
(13) Deduced from the lines given in Paschen-Götze, Seriengesetze der Linienspectren, assuming v = 27700 for the 44 term, which is not likely to be far different from the corresponding term of He II.Google Scholar