Measurement of Free-Atom K-Shell Binding Energies of Light Elements

1978 ◽  
Vol 17 (2) ◽  
pp. 49-52 ◽  
Author(s):  
P Bisgaard ◽  
R Bruch ◽  
P Dahl ◽  
B Fastrup ◽  
M Rødbro

In a recent paper, an account was given of new measurements on the excitation potentials of lithium metal. Here we shall describe the corresponding results for the next element, beryllium, attention being again mainly focussed on the excitation of the K-radiation. The purpose of these investigations may be defined as an attempt to determine the effect of the metallic binding on the atomic constants of these light elements. Thus, in Paper I, it was shown that the minimum energy needed for the excitation of the K-radiation of lithium metal is considerably less than the K-ionization potential of the free atom. This low value seemed at first sight inconsistent with the facts of the excitation of X-rays in heavier elements. But, if we adopt a more direct comparison, it is easy to see that the observation that this minimum excitation potential agrees numerically with the energy required for a K→L switch in the free atom implies simply that the effect of the binding here is small. We shall show that for beryllium the effect of the binding is definitely observable; its magnitude, about 20 volts, is considerable compared with the absolute K-excitation energy, about 100 volts. In the attempt to correlate these observations, it became apparent that the theory of Paper I is incomplete. We shall therefore give a corrected treatment in its application to lithium and beryllium metals, and it will be seen that, on certain assumptions, the new theory seems capable of accounting in detail for the observed break-potentials. It has also been found that there is an appreciable difference between the minimum K-excitation potentials of beryllium in the form of a metal and of a polar compound. These problems are closely related to work done on the influence of chemical binding on the absorption-edges and lines in the region of harder X-rays. Thus Bäcklin† studied the K α line of sulphur, and other elements when used in the form of various compounds, and found shifts of the order of 10 volts. Such investigations open up the question of how far the spectroscopic data of X-rays from solid targets are representative of atomic constants.


2009 ◽  
Vol 5 (S268) ◽  
pp. 469-471
Author(s):  
Hubert Reeves

AbstractMy aim is to show how the abundance ratios of the light elements (6 to 11) are related to the properties of the strong nuclear interaction and, in particular, to the major influence of closed shells of neutrons and protons, (the magic numbers : 2, 8, etc) on the binding energies of the nuclei.


1978 ◽  
Vol 68 (2) ◽  
pp. 696-699 ◽  
Author(s):  
M. S. Banna ◽  
D. C. Frost ◽  
C. A. McDowell ◽  
B. Wallbank

1965 ◽  
Vol 14 (5) ◽  
pp. 127-129 ◽  
Author(s):  
A. Fahlman ◽  
K. Hamrin ◽  
R. Nordberg ◽  
C. Nordling ◽  
K. Siegbahn

1978 ◽  
Vol 68 (12) ◽  
pp. 5459-5466 ◽  
Author(s):  
M. S. Banna ◽  
B. Wallbank ◽  
D. C. Frost ◽  
C. A. McDowell ◽  
J. S. H. Q. Perera

Author(s):  
T. Oikawa ◽  
M. Inoue ◽  
T. Honda ◽  
Y. Kokubo

EELS allows us to make analysis of light elements such as hydrogen to heavy elements of microareas on the specimen. In energy loss spectra, however, elemental signals ride on a high background; therefore, the signal/background (S/B) ratio is very low in EELS. A technique which collects the center beam axial-symmetrically in the scattering angle is generally used to obtain high total intensity. However, the technique collects high background intensity together with elemental signals; therefore, the technique does not improve the S/B ratio. This report presents the experimental results of the S/B ratio measured as a function of the scattering angle and shows the possibility of the S/B ratio being improved in the high scattering angle range.Energy loss spectra have been measured using a JEM-200CX TEM with an energy analyzer ASEA3 at 200 kV.Fig.l shows a typical K-shell electron excitation edge riding on background in an energy loss spectrum.


Author(s):  
G.F. Bastin ◽  
H.J.M. Heijligers

Among the ultra-light elements B, C, N, and O nitrogen is the most difficult element to deal with in the electron probe microanalyzer. This is mainly caused by the severe absorption that N-Kα radiation suffers in carbon which is abundantly present in the detection system (lead-stearate crystal, carbonaceous counter window). As a result the peak-to-background ratios for N-Kα measured with a conventional lead-stearate crystal can attain values well below unity in many binary nitrides . An additional complication can be caused by the presence of interfering higher-order reflections from the metal partner in the nitride specimen; notorious examples are elements such as Zr and Nb. In nitrides containing these elements is is virtually impossible to carry out an accurate background subtraction which becomes increasingly important with lower and lower peak-to-background ratios. The use of a synthetic multilayer crystal such as W/Si (2d-spacing 59.8 Å) can bring significant improvements in terms of both higher peak count rates as well as a strong suppression of higher-order reflections.


1991 ◽  
Vol 161 (5) ◽  
pp. 171-175 ◽  
Author(s):  
Yu.B. Khariton ◽  
Ya.B. Zeldovich ◽  
I.I. Gurevich ◽  
I.Ya. Pomeranchuk

1986 ◽  
Vol 1 (6) ◽  
pp. 765-773 ◽  
Author(s):  
E. Batalla ◽  
J.O. Strom-Olsen ◽  
Z. Altounian ◽  
D. Boothroyd ◽  
R. Harris

2002 ◽  
Vol 719 ◽  
Author(s):  
K. Thonke ◽  
N. Kerwien ◽  
A. Wysmolek ◽  
M. Potemski ◽  
A. Waag ◽  
...  

AbstractWe investigate by photoluminescence (PL) nominally undoped, commercially available Zinc Oxide substrates (from Eagle Picher) grown by seeded chemical vapor transport technique in order to identify residual donors and acceptors. In low temperature PL spectra the dominant emission comes from the decay of bound exciton lines at around 3.36 eV. Zeeman measurements allow the identification of the two strongest lines and some weaker lines in-between as donorrelated. From the associated two-electron satellite lines binding energies of the major donors of 48 meV and 55 meV, respectively, can be deduced.


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