Abstract

Quantitative analysis of materials from Heavy Ion PIXE spectra remains impeded by the lack of reliable X-ray production cross section (XPCS) data. Although efforts at experimental Heavy Ion induced XPCS measurements still continue, Multiple Ionisation (MI) effects, which are not fully described by theory, render simulations of heavy ion PIXE data unreliable for large Z1/Z2 collisions, especially at low energies. This is also exacerbated by the random selection of projectile-target combinations for measured and reported experimental data available to validate theory. This study explored heavy ion induced X-ray production cross section deviations from those induced by protons at the same ion velocity. This enabled evaluations of the degree to which cross sections are enhanced through MI effects, with the aim of predicting XPCS due to heavy ion impact. The evaluation was carried out through the scaling of experimental heavy ion to theoretical proton cross section ratios (R), which were then used for the interpolation of XPCS in the same target element for ‘missing’ projectiles within the range of evaluation. Here we present measurements of heavy ion induced total L-shell XPCS in Bi, carried out to determine HI/p MI induced deviations due to C, F, Cl and Ti projectiles at an ion velocity range of (0.2–1.0) MeV/nucleon.

Details

Title
Semi-empirical parameterization of HI/p L-shell X-ray production cross section ratios in Bi for Heavy Ion PIXE
Author
Masekane, M. C. 1 ; Msimanga, M. 2 ; Bogdanović Radović, I. 3 ; Madhuku, M. 4 ; Moloi, S. J. 5 

 University of South Africa, Department of Physics, Florida, South Africa (GRID:grid.412801.e) (ISNI:0000 0004 0610 3238); University of Zagreb, Department of Physics, Zagreb, Croatia (GRID:grid.4808.4) (ISNI:0000 0001 0657 4636); Ruđer Bošković Institute, Zagreb, Croatia (GRID:grid.4905.8) (ISNI:0000 0004 0635 7705); National Research Foundation, iThemba LABS TAMS, Johannesburg, South Africa (GRID:grid.425534.1) (ISNI:0000 0000 9399 6812) 
 National Research Foundation, iThemba LABS TAMS, Johannesburg, South Africa (GRID:grid.425534.1) (ISNI:0000 0000 9399 6812); Tshwane University of Technology, Physics Department, Pretoria, South Africa (GRID:grid.412810.e) (ISNI:0000 0001 0109 1328) 
 Ruđer Bošković Institute, Zagreb, Croatia (GRID:grid.4905.8) (ISNI:0000 0004 0635 7705) 
 National Research Foundation, iThemba LABS TAMS, Johannesburg, South Africa (GRID:grid.425534.1) (ISNI:0000 0000 9399 6812) 
 University of South Africa, Department of Physics, Florida, South Africa (GRID:grid.412801.e) (ISNI:0000 0004 0610 3238) 
Pages
20942
Publication year
2023
Publication date
2023
Publisher
Nature Publishing Group
e-ISSN
20452322
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2894594272
Copyright
© The Author(s) 2023. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.