Electron Energy Loss Spectra of NO2 and SO2

1971 ◽  
Vol 49 (11) ◽  
pp. 1437-1444 ◽  
Author(s):  
J. S. Bulger ◽  
J. M. Goodings

Electron energy loss data are presented for CO2, NO2, and SO2 at scattering angles of 0° and 60° and impact energies in the range 30–140 eV. Energy selectors of the 127° type have been used to detect energy losses in the range 0–20 eV. The energy loss data unify and supplement previous work involving a variety of techniques. They are discussed with reference to the Walsh correlation diagram, particularly with regard to the 6a1 molecular orbital with its unusually large variation of binding energy with bond angle. Below the ionization potential, the energy loss spectra are in good agreement with optical data and electron scavenging measurements at threshold; however, the Rydberg transitions have not reached their maximum relative intensities at the incident electron energies used. Excitation peaks corresponding to the ground state ion are observed in CO2 and SO2; for NO2[Formula: see text], a peak appearing at 9.7 eV is attributed to an excitation of the neutral molecule, however, since direct excitation of the ground state ion involves a large change in bond angle. Compared with CO2 and NO2, the SO2 molecule has an extra closed shell of 8 electrons such that the excitation of SO2+ appears to be dominated by autoionization at low incident electron energies. As the energy is increased to 138 eV, four peaks emerge which agree with previous photoelectron and Penning ionization data.

Author(s):  
M. Isaacson

In an earlier paper1 it was found that to a good approximation, the efficiency of collection of electrons that had lost energy due to an inner shell excitation could be written as where σE was the total excitation cross-section and σE(θ, Δ) was the integral cross-section for scattering within an angle θ and with an energy loss up to an energy Δ from the excitation edge, EE. We then obtained: where , with P being the momentum of the incident electron of velocity v. The parameter r was due to the assumption that d2σ/dEdΩ∞E−r for energy loss E. In reference 1 it was assumed that r was a constant.


A planetary atom is an atom or ion in a state, with two or more excited electrons, which has negligible overlap with the ground state or first few excited states. Classical mechanics and Einstein-Brillouin-Keller quantization are used to study them. They are not produced by direct (one-photon) optical excitation from low states, statistically they predominate over states which can be produced by direct optical excitation, and they are long-lived. Each state is a member of a series labelled by a half-odd-integer scaling number v . The states of the series have energies which are approximately proportional to 1/ v 2 . The energies of the states of a planetary atom depend on the charge of the parent ion, and not on its detailed structure. Electron energy loss spectroscopy is a possible means of studying planetary atoms experimentally.


2019 ◽  
Vol 50 (1) ◽  
Author(s):  
Jeong Eun Chae ◽  
Ji-Soo Kim ◽  
Sang-Yeol Nam ◽  
Min Su Kim ◽  
Jucheol Park

AbstractElectron energy loss spectroscopy (EELS) is an analytical technique that can provide the structural, physical and chemical information of materials. The EELS spectra can be obtained by combining with TEM at sub-nanometer spatial resolution. However, EELS spectral information can’t be obtained easily because in order to interpret EELS spectra, we need to refer to and/or compare many reference data with each other. And in addition to that, we should consider the different experimental variables used to produce each data. Therefore, reliable and easily interpretable EELS standard reference data are needed.Our Electron Energy Loss Data Center (EELDC) has been designated as National Standard Electron Energy Loss Data Center No. 34 to develop EELS standard reference (SR) data and to play a role in dissemination and diffusion of the SR data to users. EELDC has developed and collected EEL SR data for the materials required by major industries and has a total of 82 EEL SR data. Also, we have created an online platform that provides a one-stop-place to help users interpret quickly EELS spectra and get various spectral information. In this paper, we introduce EEL SR data, the homepage of EELDC and how to use them.


2008 ◽  
Vol 1124 ◽  
Author(s):  
Nan Jiang

AbstractThis work demonstrates that absorption near-edge structures of the O K-edge in zircon are directly related to atom structure, including bond length, bond angle and coordination. Small variations in the structure can induce measurable changes in absorption spectrum.


2017 ◽  
Vol 23 (S1) ◽  
pp. 106-107 ◽  
Author(s):  
Niklas Mevenkamp ◽  
Benjamin Berkels ◽  
Martial Duchamp

2004 ◽  
pp. 53-58 ◽  
Author(s):  
B. Predojevic ◽  
Dragutin Sevic ◽  
Vladimir Pejcev ◽  
Bratislav Marinkovic ◽  
Dusan Filipovic

Autoionizing energy-loss spectra of Zn from 10.8 to 12.5 eV, for incident electron energies between 20 and 100 eV, have been recorded at scattering angles from 0? to 10?. These spectra were decomposed using ?2 minimization procedure to show the contribution of the 3d 10 4s 2 ? 3d 9 4s 2 4p, single inner-electron transitions. Relative intensities of lines in the Zn spectra are determined with respect to the 3d 10 4s 2 ? 3d 10 4s4p resonance line. The line shapes and widths are examined. The results are compared with available measurements and theoretical estimates.


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