Abstract

The importance of Atomic Form Factors (f) is well-known to the scientific community. Tabulated values for f are mostly used in calculating cross-sections and Monte Carlo sampling for the coherent scattering of photons. The uses of these values are subjected to different approximations and interpolation techniques because the available data points for f in the literature for specified momentum-transfer-grids are very limited. In order to make it easier to accurately use the tabulated data, a mathematical expression for f functions would be a great achievement. Therefore, the current study was designed to suggest an empirical expression for the f functions. In the results, an empirical equation for Hubbell's tabulated data for f is created in the momentum transfer range, q = 0–50 Å−1 for the elements in the range 1≤ Z ≤30. The number of applied parameters was seven. The fitting to f showed that the maximum deviation was within 3%, 4% and 5% for the element having, Z = 1–11, Z = 12–22 and Z = 23–30, respectively, while the average deviations were within 0.3–2.25% for all elements (i.e., Z = 1–30). The values generated by the analytical equation were used in the Monte Carlo code instead of Hubbell’s tabulated values. The statistical noise in the Probability Distribution Functions of coherently scattered photons was efficiently removed. Furthermore, it also reduced the dependence on different interpolation techniques and approximations, and on the use of large tabulated data for f with the specified elements.

Highlights

  • The Rayleigh scattering of photons by a bound atomic electron is one of the major modes of interaction of photons with matter for low energy x-rays and soft c-rays

  • The results shows that smax(Z) from FH are within 3%, 4% and 5% for elements having Z = 1–11, Z = 12–22 and Z = 23–30, respectively while the smean(Z) and sst(Z) are within 0.3–2.25% and 0.15–1.35% respectively for the listed elements (i.e., Z = 1– 30)

  • The results show that the density of statistical noise is significantly reduced with the application of the empirical equation for the Monte Carlo (MC) sampling of coherently scattered photons

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Summary

Introduction

The Rayleigh (elastic) scattering of photons by a bound atomic electron is one of the major modes of interaction of photons with matter for low energy x-rays and soft c-rays. Tabulated values for f are mostly used in calculating cross-sections and MC sampling for coherent scattering of photons. The F (q,Z) function was constructed from the available analytical equation for Hydrogen as stated above, depending on the value of the atomic number Z as follows: Here, qi is the momentum transfer grid values given in Hubbel and Øverbø [5], FH (q,Z) represent Hubbell’s data depending on Z and Fc(q,Z) are the calculated values of the fitted analytical functions used in the present work.

Results
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