1959
DOI: 10.1139/p59-107
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Scattering Factors for Some of the Heavier Atoms

Abstract: A program for calculating X-ray atomic scattering factors from the radial wave functions has been written for the IBM 650 installation at the University of Toronto. It has been applied to the results of self-consistent field calculations previously performed at this University on the FERUT computer. Results are given for Ne, V++, Kr, Ag+, and Pb+++. The results for Ne and V++ are compared with those calculated by Freeman using Allen's wave functions for Ne and Hartree's approximate wave functions for V++.

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Cited by 4 publications
(4 citation statements)
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“…Worsley (1959) has just published a scattering factor for V +~ and this agrees exactly with the values we have given in Table 1. Recently Piper (1959) with those of Piper's to the number of figures quoted, again giving an excellent check on the accuracy of our calculations.…”
Section: Total Atomic Scattering Factorssupporting
confidence: 89%
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“…Worsley (1959) has just published a scattering factor for V +~ and this agrees exactly with the values we have given in Table 1. Recently Piper (1959) with those of Piper's to the number of figures quoted, again giving an excellent check on the accuracy of our calculations.…”
Section: Total Atomic Scattering Factorssupporting
confidence: 89%
“…The numerical computations were carried out on Whirl-12 wind I, the MIT high speed computer, using routines and techniques described earlier (Freeman, 1959a). As 10 will be shown, the accuracy of the form factors agrees s digitally with the few other such calculations available to date (Worsley, 1959;Piper, 1959). …”
Section: Introductionsupporting
confidence: 65%
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“…In computing scattering factors for Bi-Sb alloys, the Brindley-James (1931) (James, 1948), with a dispersion correction for K electrons only, called the fl curve in what follows. Of the other sets of scattering factors for elements of high atomic number in the literature, those of Worsley (1959) for Pb +++, and Henry (1954) for Au + and Hg++, agree well with the Freeman values when correctly scaled, except at low (sin 0)/~t values where the degree of ionization becomes of importance. The Thomas & Umeda (1957) values however decrease less rapidly beyond (sin 0)/,~=1 than do those calculated from self-consistent field theory.…”
Section: Parameter Zsupporting
confidence: 67%