Table. 2 The optical ELF data used for Mo and W.
From: Influence of energy loss function to the Monte Carlo simulated electron backscattering coefficient
Element | Name | Photon energy range and the corresponding datasets | |||
|---|---|---|---|---|---|
Mo | Palik | 31–39 eV Interpolation45 | 40 eV–30 keV Henke48 | 30 keV–10 MeV EPDL9749 | |
Tanuma | |||||
Werner | 0.5–70.5 eV Werner34 | 71–80 eV Interpolation | 80 eV–30 keV Henke48 | ||
W | Palik | 0.05–33.5 eV Weaver52 | 34–39 eV Interpolation45 | 40 eV–30 keV Henke48 | |
Tanuma | |||||
Werner | 0.5–70.5 eV Werner34 | 71–80 eV Interpolation | 80 eV–30 keV Henke48 | ||
