-
Notifications
You must be signed in to change notification settings - Fork 0
praxes/henke_physical_reference
Folders and files
Name | Name | Last commit message | Last commit date | |
---|---|---|---|---|
Repository files navigation
Low-Energy X-ray Interaction Coefficients: Photoabsorption, Scattering, and Reflection E = 30-30,000 eV, Z = 1-92 B. L. Henke, E. M. Gullikson, and J. C. Davis Center for X-Ray Optics, 2-400 Lawrence Berkeley Laboratory Berkeley, California 94720 These files were used to generate the tables published in reference [1]. The files contain three columns of data: Energy(eV), f_1, f_2, where f_1 and f_2 are the atomic (forward) scattering factors. There are 500+ points on a uniform logarithmic mesh with points added 0.1 eV above and below "sharp" absorption edges. (Note: below 29 eV f_1 is set equal to -9999.) The tabulated values of f_1 contain a relativistic, energy independent, correction given by, Z* = Z - (Z/82.5)^(2.37). The atomic photoabsorption cross section, mu_a, may be readily obtained from the values of f_2 using the relation, mu_a = 2*r_0*lambda*f_2 where r_0 is the classical electron radius, and lambda is the wavelength. The index of refraction for a material with N atoms per unit volume is calculated by, n = 1 - N*r_0*(lambda)^2*(f_1+if_2)/(2*pi). These (semi-empirical) atomic scattering factors are based upon photoabsorption measurements of elements in their elemental state. The basic assumption is that condensed matter may be modeled as a collection of non-interacting atoms. This assumption is in general a good one for energies sufficiently far from absorption thresholds. In the threshold regions, the specific chemical state is important and direct experimental measurements must be made. These tables are based on a compilation of the available experimental measurements and theoretical calculations. For many elements there is little or no published data and in such cases it was necessary to rely on theoretical calculations and interpolations across Z. In order to improve the accuracy in the future considerably more experimental measurements are needed. Please send any comments to EMGullikson@lbl.gov. Note that the following elements have been updated since the publication of Ref. [1] in July 1993. Element Updated Energy Range Mg 1/15/94 30-50 eV Al 1/15/94 30-73 eV Si 1/15/94 30-100 eV Au 11/7/94 2000-6500 eV Li 11/15/94 2000-30000 eV [1] B. L. Henke, E. M. Gullikson, and J. C. Davis, Atomic Data and Nuclear Data Tables Vol. 54 No. 2 (July 1993).
About
Atomic scattering factors as compiled by Henke, Gullikson, and Davis
Resources
Stars
Watchers
Forks
Packages 0
No packages published