Use of the Photoelectric Absorption Measurements

There is, in principle, a simpler approach to the calculation of the dispersion terms by using the following relationship between the oscillator density functions (dg/d$\omega_s$) and the photoelectric absorption coefficient $\mu(\omega)$:⁶¹

$$\Big(\frac{\mbox{d}g}{\mbox{d}\omega}\Big) = \frac{mc}{2{\pi}^2e^2} {\mu}(\omega),$$ (23)

which indicates that the oscillator density (dg/d$\omega$) is simply proportional to $\mu(\omega)$.

Using experimental values of $\mu$($\omega$) one could obtain values for the oscillator densities from equation (23). However, accurate values for $\mu$($\omega$) are not presently available for all the elements in a useful range of $\omega$. Then, the usefulness of an empirical method to obtain (dg/d$\omega$)_s, g_s, ${\Delta}f^{\prime}$ and ${\Delta}f^{\prime\prime}$ based on the experimental values of $\mu$($\omega$) is very limited.

A semi-empirical method has been used by taking the well known approximate functional dependence of $\mu$($\omega$):

$$\mu(\omega) = \left\{ \begin{array} {ll} ({\omega}_s/{\omeg... ...} \gt {\omega}_s \\ 0 & \omega < {\omega}_s\end{array} \right.$$ (24)

where n has a value of about 3 which, however, changes with the atomic number and with the absorption edge involved. Moreover $\mu$($\omega$) is not strictly zero below $\omega_s$.

By choosing the best experimental values for n and $\mu$($\omega_s$)integration of equation (17) should provide reasonably good values of g_s. One can substitute, in the general case, equations (23) and (24) in (17) to obtain:

$$g_s = \frac{mc}{2{\pi}^2e^2}\frac{{\omega}_s}{n - 1} {\mu}({\omega}_s).$$ (25)

Analogously, we obtain from (22) the contribution ${\Delta}f^{\prime}_s$ of electrons s to ${\Delta}f^{\prime}$:

$${\Delta}f^{\prime}_s = \frac{mc}{2{\pi}^2e^2} {\mu}({\omega}... ...\omega}^2 \mbox{d}\omega}{({\omega}^2_i-{\omega}^2) {\omega}^n}$$ (26)

Equation (26) has been integrated in the general case by Parratt and Hempstead.³⁶ These authors have expressed their results in the form of `universal anomalous dispersion curves', which are essentially the representation of the integral in equation (26) with n as a parameter, as a function of ${\lambda}_i/{\lambda}_s$. When damping is neglected, these curves are independent of the atomic number and of the electronic shell involved. To obtain a particular value of ${\Delta}f^{\prime}_s$, the value on the curve with the correct value of n is multiplied by the oscillator strength calculated from equation (25). ${\Delta}f^{\prime}$ is then obtained by summation through all s = K, L, M,$\dots$ shells. The shape of the curves, reproduced in Fig. 1, is quite instructive. They are qualitatively correct and show that the dispersion contributions from the various electron shells are rarely negligible, or, in other words, as Parratt and Hempstead point out, there is practically no region of normal dispersion.

Figure 1: Universal anomalous dispersion curves according to Parratt and Hempstead. The value of Re(J_q - 1) times the oscillator strength gives the anomalous dispersion correction for any atomic shell of electrons.

Since the method used by Parratt and Hempstead is based on experimentally determined values and uses exact integrations one should expect results in better agreement with the independent measurements made of the atomic scattering factor than is the case for the values obtained using Hönl's theory based on hydrogen-like electron shells. The calculations made by Parratt and Hempstead for the K region of copper and the L region of tungsten using only one term in the oscillator distribution for each electron shell, actually showed a less satisfactory agreement than Hönl's theory. This rather discouraging result was attributed by Parratt and Hempstead to (a) the difficulties inherent in the experimental measurements and (b) neglect of parts of the calculations in previous comparisons.

In fact, the experimental differences (f - f₀) which they used to compare their calculations were presumably of a rather low precision, since they were based on values of f measured in the early 30's and presumably not very precise. The value of f₀ subtracted in the iron case was the Thomas-Fermi f₀ = 17.3 for plane (110) of Fe.

It would be interesting to remeasure the values of f using modern techniques and subtract better values of f₀ as are currently available nowadays in order to make a definite comparison.

Copyright © 1981, 1998 International Union of Crystallography