Hostname: page-component-586b7cd67f-vdxz6 Total loading time: 0 Render date: 2024-11-29T21:39:28.636Z Has data issue: false hasContentIssue false

The computation of quadrupole line strengths

Published online by Cambridge University Press:  24 October 2008

R. H. Garstang
Affiliation:
University of London ObservatoryMill Hill Park London, N. W. 7

Abstract

The methods introduced into the theory of atomic spectra by Racah are applied to the problem of the computation of the strengths of electric quadrupole lines. Detailed numerical results are given for two configurations of equivalent d-electrons.

Type
Research Article
Copyright
Copyright © Cambridge Philosophical Society 1957

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

REFERENCES

(1)Condon, E. U. and Shortley, G. H.Theory of Atomic Spectra (Cambridge University Press, 1951).Google Scholar
(2)Garstang, R. H.Man. Not. R. Astr. Soc. 111 (1951), 115.Google Scholar
(3)Garstang, R. H.Vistas in Astronomy (Pergamon Press, London, 1955), vol. 1, p. 268.Google Scholar
(4)Garstang, R. H.Proc. Camb. Phil. Soc. 52 (1956), 107.CrossRefGoogle Scholar
(5)Obi, S., Ishidzu, T., Horie, H., Yanagawa, S., Tanabe, Y. and Sato, M.Ann. Obs. Astr. Tokyo, 3 (1953), no. 3, 4 (1954), no. 1 and 4 (1955), no. 2. Tables are also available in Oak Ridge National Laboratory Report, no. 1098, 1952.Google Scholar
(6)Pasternack, S.Astrophys. J. 92 (1940), 129.CrossRefGoogle Scholar
(7)Racah, G.Phys. Rev. (2), 62 (1942), 438.CrossRefGoogle Scholar
(8)Racah, G.Phys. Rev. (2), 63 (1943), 367.Google Scholar
(9)Seaton, M. J.Proc. Roy. Soc. A, 231 (1955), 37.Google Scholar
(10)Shortley, G. H.Phys. Rev. (2), 57 (1940), 225.Google Scholar