Electronic structure of hydrazoic acid and the azide ion from x-ray and ultraviolet electron spectroscopy

1975 ◽  
Vol 97 (17) ◽  
pp. 4845-4851 ◽  
Author(s):  
Ting Ho Lee ◽  
Richard J. Colton ◽  
Michael G. White ◽  
J. Wayne Rabalais

1975 ◽  
Vol 6 (43) ◽  
pp. no-no
Author(s):  
TING HO LEE ◽  
RICHARD J. COLTON ◽  
MICHAEL G. WHITE ◽  
J. WAYNE RABALAIS








1975 ◽  
Vol 8 (3) ◽  
pp. 391-398 ◽  
Author(s):  
Michael G. White ◽  
Richard J. Colton ◽  
Ting Ho Lee ◽  
J.Wayne Rabalais




2013 ◽  
Vol 190 ◽  
pp. 113-124 ◽  
Author(s):  
Sarp Kaya ◽  
Daniel Friebel ◽  
Hirohito Ogasawara ◽  
Toyli Anniyev ◽  
Anders Nilsson


The electronic structure of matter has so far been studied almost exclusively by means of the electromagnetic radiation which is being emitted (or absorbed) at excitation. Apart from some early attempts, the electrons themselves were not directly detected. The various energy levels which could be studied by different modes of excitations were observed as photons being emitted (or absorbed) when electrons were making quantum jumps between two levels. Over a long period of time spectroscopy in the visible, infrared, ultraviolet, and X-ray parts of the electromagnetic spectrum was gradually perfected and extensively used in many kinds of applications. More recently, other and in some cases more sophisticated techniques, like n.m.r., e.p.r. and microwave spectroscopy, have been added to previously existing spectroscopic tools. During the last decade serious attempts have been made to explore the possibility of developing a spectroscopy based on the direct observation of the electrons. The results are encouraging. Despite many initial experimental difficulties it now seems evident that these can be solved in a surprisingly satisfactory way. Moreover, new types of information have become accessible and the fields of application are numerous.



1981 ◽  
Vol 36 (9) ◽  
pp. 937-943 ◽  
Author(s):  
Siegfried Falch ◽  
Georg Rainer-Harbach ◽  
Friedrich Schmückle ◽  
Siegfried Steeb

Abstract Using an electron microprobe, the position and shape of the characteristic X-Ray emission lines from the elements Cu, Zr, Ti, Fe, Co, and Mn in metallic glasses of the systems Cu-Zr, Cu-Ti, Fe-B, Fe-P, Co-B, Co-P, Fe-Ge-P, Mn-Si-P, and Fe-Si-P were studied. In each case the lines were compared with those of either the crystalline element or the corresponding crystalline compound. Compared to electron spectroscopy methods such as XPS or UPS, the method used during this work has the advantage that the spectra obtained are specific for the corresponding element. The general trend of the results can be described in such a way that the energy of binding of the electrons to the corresponding atomic species is larger in the amorphous state than in the crystalline element, whereas the energy of binding of the electrons in the amorphous state is similar to that of the corresponding crystalline compound.



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