| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1886619 | Radiation Physics and Chemistry | 2010 | 11 Pages |
Abstract
Theoretical K-shell photoionization and K X-ray fluorescence (K XRF) cross sections have been fitted empirically in polynomials of photon energy E and atomic number Z. This has been used to develop a computer code KCSPIF to generate K-shell photo-ionization and K XRF cross-sections for any element in the range 5≤Z≤95 and for photon energies, above K-edge–1500 keV, when only the atomic number and photon energy are supplied as the input.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Radiation
Authors
Meenakshi Bansal, Raj Mittal,