Proton-Induced L-shell X-Rays of Pr, Sm, Eu, Gd, and Dy
Characteristic L-shell x rays of the five rare earths Pr, Sm, Eu, Gd, and Dy were studied in this work. The x rays were produced by ionization from 0.3 to 2.0 MeV protons from the 2.0 MV Van de Graaff at North Texas State University. Total L-shell ionization and x-ray production cross sections were...
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North Texas State University
1974
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ndltd-unt.edu-info-ark-67531-metadc5002842017-03-17T08:41:16Z Proton-Induced L-shell X-Rays of Pr, Sm, Eu, Gd, and Dy Abrath, Frederick G. L-shell x-rays Rare earths -- Spectra. Cross sections (Nuclear physics) -- Tables. X-ray spectroscopy -- Tables. L-shell ionization x-ray production Characteristic L-shell x rays of the five rare earths Pr, Sm, Eu, Gd, and Dy were studied in this work. The x rays were produced by ionization from 0.3 to 2.0 MeV protons from the 2.0 MV Van de Graaff at North Texas State University. Total L-shell ionization and x-ray production cross sections were measured for Sm and compared to the BEA, CBEA and PWBA theories. Total L-shell ionization cross sections were measured for Pr, Eu, Gd, and Dy and compared to the BEA, CBEA, and PWBA. The CBEA and PWBA fit the samarium data well for both ionization and x-ray production cross sections. The BEA was generally 40 per cent lower than the data. The CBEA and the PWBA also fit the ionization cross section data for Pr, Eu, Gd and Dy, while the BEA was generally 40 per cent lower than the data. North Texas State University Gray, Thomas James, 1917- Redding, Rogers W. Foster, Bruce P. Seiler, David G. Krishnan, Raj Muthu 1974-08 Thesis or Dissertation iii, 72 leaves: ill. Text call-no: 379 N81d no.823 untcat: b1074291 oclc: 1454812 local-cont-no: 1002777532-Abrath https://digital.library.unt.edu/ark:/67531/metadc500284/ ark: ark:/67531/metadc500284 English Public Abrath, Frederick G. Copyright Copyright is held by the author, unless otherwise noted. All rights reserved. |
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English |
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Others
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L-shell x-rays Rare earths -- Spectra. Cross sections (Nuclear physics) -- Tables. X-ray spectroscopy -- Tables. L-shell ionization x-ray production |
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L-shell x-rays Rare earths -- Spectra. Cross sections (Nuclear physics) -- Tables. X-ray spectroscopy -- Tables. L-shell ionization x-ray production Abrath, Frederick G. Proton-Induced L-shell X-Rays of Pr, Sm, Eu, Gd, and Dy |
description |
Characteristic L-shell x rays of the five rare earths Pr, Sm, Eu, Gd, and Dy were studied in this work. The x rays were produced by ionization from 0.3 to 2.0 MeV protons from the 2.0 MV Van de Graaff at North Texas State University. Total L-shell ionization and x-ray production cross sections were measured for Sm and compared to the BEA, CBEA and PWBA theories. Total L-shell ionization cross sections were measured for Pr, Eu, Gd, and Dy and compared to the BEA, CBEA, and PWBA. The CBEA and PWBA fit the samarium data well for both ionization and x-ray production cross sections. The BEA was generally 40 per cent lower than the data. The CBEA and the PWBA also fit the ionization cross section data for Pr, Eu, Gd and Dy, while the BEA was generally 40 per cent lower than the data. |
author2 |
Gray, Thomas James, 1917- |
author_facet |
Gray, Thomas James, 1917- Abrath, Frederick G. |
author |
Abrath, Frederick G. |
author_sort |
Abrath, Frederick G. |
title |
Proton-Induced L-shell X-Rays of Pr, Sm, Eu, Gd, and Dy |
title_short |
Proton-Induced L-shell X-Rays of Pr, Sm, Eu, Gd, and Dy |
title_full |
Proton-Induced L-shell X-Rays of Pr, Sm, Eu, Gd, and Dy |
title_fullStr |
Proton-Induced L-shell X-Rays of Pr, Sm, Eu, Gd, and Dy |
title_full_unstemmed |
Proton-Induced L-shell X-Rays of Pr, Sm, Eu, Gd, and Dy |
title_sort |
proton-induced l-shell x-rays of pr, sm, eu, gd, and dy |
publisher |
North Texas State University |
publishDate |
1974 |
url |
https://digital.library.unt.edu/ark:/67531/metadc500284/ |
work_keys_str_mv |
AT abrathfrederickg protoninducedlshellxraysofprsmeugdanddy |
_version_ |
1718432271028977664 |