ESCA spectra and molecular charge distributions for some pyrimidine and purine bases

1978 ◽  
Vol 56 (11) ◽  
pp. 1555-1561 ◽  
Author(s):  
James Peeling ◽  
Frank E. Hruska ◽  
N. Stewart McIntyre

A series of pyrimidine and purine bases bas been studied experimentally by electron spectroscopy for chemical analysis. Individual component peaks in the spectra were assigned on the basis of known substituent effects on core electron binding energies. Binding energies for all the core levels in the molecules provide sufficient data to determine the molecular charge distributions. The results compare favourably with atomic charges determined theoretically in the CNDO/2 molecular orbital formalism.


1988 ◽  
Vol 53 (3) ◽  
pp. 425-432 ◽  
Author(s):  
Zdeněk Bastl ◽  
Heidrun Gehlmann

The core electron binding energies of eighteen compounds containing iodine in different oxidation states ranging from (-I) to (VII) have been measured. The observed chemical shifts differ from the literature data. The anticipated existence of hexavalent iodine in certain compounds has not been demonstrated. The relative subshell photoemission intensities of iodine have been determined. Empirically derived atomic sensitivity factors and theoretical photoionization cross-sections have been used to calculate the surface stoichiometry. The concentration ratios obtained via the two methods are compared. In agreement with generally accepted view the results of this comparison imply that, for quantitative surface analysis, empirical values should be used rather than theoretical data.





2006 ◽  
Vol 106 (13) ◽  
pp. 2581-2586 ◽  
Author(s):  
Yuji Takahata ◽  
Andre K. Okamoto ◽  
Delano P. Chong


1977 ◽  
Vol 49 (2) ◽  
pp. 213-217 ◽  
Author(s):  
M.Salim Banna ◽  
David C. Frost ◽  
Charles A. McDowell ◽  
Louis Noodleman ◽  
Barry Wallbank


1992 ◽  
Vol 7 (8) ◽  
pp. 1984-1986 ◽  
Author(s):  
Shigemi Kohiki ◽  
Mikihiko Nishitani ◽  
Takayuki Negami ◽  
Takahiro Wada

The Cu, In, and Se core-level electron binding energies of the p-type Cu–In–Se–N thin film were larger than those of the n-type Cu–In–Se thin film. The positive shift of the core-electron binding energies for the Cu–In–Se–N film is consistent with that expected from the conduction types of the films. Holes were positioned in the Cu–Se antibonding orbitals of the Cu–In–Se–N film. The analysis using the Auger parameter revealed that the Cu–Se bonding interaction is stronger for the Cu–In–Se–N film than for the Cu–In–Se film.



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