Please use this identifier to cite or link to this item: http://hdl.handle.net/11189/7499
Title: Non-linearity of prompt nuclear satellites relative intensities observed from high energy protons induced X-ray emission
Authors: Pineda-Vargas, C.A. 
Msimanga, M. 
Bark, R. A 
Gihwala, D 
Keywords: High-energy PIXE;Nuclear satellites;Rare earths;Cyclotron
Issue Date: 2011
Publisher: Elsevier
Source: Pineda-Vargas, C. A., Msimanga, M., Bark, R. A. et al. 2011. Non-linearity of prompt nuclear satellites relative intensities observed from high energy protons induced X-ray emission. Nuclear Instruments and Methods in Physics Research B, 273: 33–35. [http:doi.org/10.1016/j.nimb.2011.07.031]
Journal: Nuclear Instruments and Methods in Physics Research B 
Abstract: A study of the relative intensity of K-shell X-ray nuclear satellites as a function of atomic number, Z is presented. These satellites, which are generated during bombardment with high energetic protons of 66 MeV from targets composed of pure fluoride compounds for the rare earths and heavier metals includ- ing the platinum (Pt, Au) and fissionable metals (Th, U) are of particular interest in the quantitative ele- mental analysis of rare earth and heavy metals by energetic protons. This paper will describe aspects that may account for the production cross section of nuclear satellites for atomic numbers 57 6 Z 6 92. Pre- vious results that showed a linear relationship between relative intensities and atomic number will be discussed
URI: http://hdl.handle.net/11189/7499
ISSN: 0168-583X
DOI: http:doi.org/10.1016/j.nimb.2011.07.031
Appears in Collections:HWSci - Journal Articles (DHET subsidised)

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