Fine structure on inner-shell ionization edges (ELNES/ EXELFS)

2020 ◽  
pp. 79-96
Author(s):  
Rik Brydson
Author(s):  
Raynald Gauvin ◽  
Gilles L'Espérance

Values of cross sections for ionization of inner-shell electrons by electron impact are required for electron probe microanalysis, Auger-electron spectroscopy and electron energy-loss spectroscopy. In this work, the results of the measurement of inner-shell ionization cross-sections by electron impact, Q, in a TEM are presented for the K shell.The measurement of QNi has been performed at 120 KeV in a TEM by measuring the net X-ray intensity of the Kα line of Ni, INi, which is related to QNi by the relation :(1)where i is the total electron dose, (Ω/4π)is the fractional solid angle, ω is the fluorescence yield, α is the relative intensity factor, ε is the Si (Li) detector efficiency, A is the atomic weight, ρ is the sample density, No is Avogadro's number, t' is the distance traveled by the electrons in the specimen which is equal to τ sec θ neglecting beam broadening where τ is the specimen thickness and θ is the angle between the electron beam and the normal of the thin foil and CNi is the weight fraction of Ni.


1982 ◽  
Vol 92 (3) ◽  
pp. 127-130 ◽  
Author(s):  
J.N. Das ◽  
S. Chakraborty

2014 ◽  
Vol 43 (1) ◽  
pp. 013102 ◽  
Author(s):  
Xavier Llovet ◽  
Cedric J. Powell ◽  
Francesc Salvat ◽  
Aleksander Jablonski

2003 ◽  
Vol 36 (3) ◽  
pp. 940-943 ◽  
Author(s):  
M. P. Oxley ◽  
L. J. Allen

A computer program which calculates inner-shell ionization and backscattering cross sections for fast electrons incident on a crystal is presented. The program calculates the inelastic scattering coefficients for inner-shell ionization, pertinent to electron energy loss spectroscopy and energy dispersive X-ray analysis, using recently presented parameterizations of the atomic scattering factors. Orientation-dependent cross sections, suitable for atom location by channelling enhanced microanalysis, may be calculated. Inelastic scattering coefficients that allow the calculation of orientation-dependent annular dark-field and Rutherford backscattering maps are calculated using an Einstein model. In all cases, absorption due to thermal diffuse scattering, also calculated using an Einstein model, can be included.


1997 ◽  
Vol 42 (3) ◽  
pp. 157-160 ◽  
Author(s):  
B. Nath ◽  
R. Biswas ◽  
C. Sinha

1980 ◽  
Vol 22 (2) ◽  
pp. 407-412 ◽  
Author(s):  
Shin Ito ◽  
Sakae Shimizu ◽  
Tatsumi Kawaratani ◽  
Ken-ichi Kubota

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