Effective Atomic Number Determination of Rare Earth Oxides with Scattering Intensity Ratio

Effective atomic numbers () of scientific samples (rare earth) were determined experimentally by scattering of 59.54 keV gamma photons from 5 Ci 241Am annular radioactive source. The scattered gamma photons were collected by using a high-resolution HPGe semiconductor detector placed at to the incid...

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Main Authors: A. Turşucu, D. Demir, P. Önder
Format: Article
Language:English
Published: Wiley 2013-01-01
Series:Science and Technology of Nuclear Installations
Online Access:http://dx.doi.org/10.1155/2013/738978
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author A. Turşucu
D. Demir
P. Önder
author_facet A. Turşucu
D. Demir
P. Önder
author_sort A. Turşucu
collection DOAJ
description Effective atomic numbers () of scientific samples (rare earth) were determined experimentally by scattering of 59.54 keV gamma photons from 5 Ci 241Am annular radioactive source. The scattered gamma photons were collected by using a high-resolution HPGe semiconductor detector placed at to the incident beam. This experiment was carried out on several elements in the atomic range for 59.54 keV incident photons. Photopeak efficiency and air and sample absorption corrections were performed on Rayleigh to Compton scattering intensity ratio; then the ratio was plotted as a function of atomic number and a fit curve was constituted. The effective atomic numbers of rare earth oxide samples were determined by this fit curve. Also, related parameters were determined by absorption technique with the same incident photon energy. Obtained values from this fit curve were compared to theoretical values and were found to closely agree with theoretical calculations.
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publishDate 2013-01-01
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series Science and Technology of Nuclear Installations
spelling doaj-art-d28168f32d354eb9b0f588bb5dacdc1a2025-02-03T06:14:06ZengWileyScience and Technology of Nuclear Installations1687-60751687-60832013-01-01201310.1155/2013/738978738978Effective Atomic Number Determination of Rare Earth Oxides with Scattering Intensity RatioA. Turşucu0D. Demir1P. Önder2Department of Energy System Engineering, Faculty of Engineering, Sirnak University, 73000 Şırnak, TurkeyDepartment of Physics, Faculty of Sciences, Ataturk University, 25240 Erzurum, TurkeyDepartment of Physics, Faculty of Sciences, Ataturk University, 25240 Erzurum, TurkeyEffective atomic numbers () of scientific samples (rare earth) were determined experimentally by scattering of 59.54 keV gamma photons from 5 Ci 241Am annular radioactive source. The scattered gamma photons were collected by using a high-resolution HPGe semiconductor detector placed at to the incident beam. This experiment was carried out on several elements in the atomic range for 59.54 keV incident photons. Photopeak efficiency and air and sample absorption corrections were performed on Rayleigh to Compton scattering intensity ratio; then the ratio was plotted as a function of atomic number and a fit curve was constituted. The effective atomic numbers of rare earth oxide samples were determined by this fit curve. Also, related parameters were determined by absorption technique with the same incident photon energy. Obtained values from this fit curve were compared to theoretical values and were found to closely agree with theoretical calculations.http://dx.doi.org/10.1155/2013/738978
spellingShingle A. Turşucu
D. Demir
P. Önder
Effective Atomic Number Determination of Rare Earth Oxides with Scattering Intensity Ratio
Science and Technology of Nuclear Installations
title Effective Atomic Number Determination of Rare Earth Oxides with Scattering Intensity Ratio
title_full Effective Atomic Number Determination of Rare Earth Oxides with Scattering Intensity Ratio
title_fullStr Effective Atomic Number Determination of Rare Earth Oxides with Scattering Intensity Ratio
title_full_unstemmed Effective Atomic Number Determination of Rare Earth Oxides with Scattering Intensity Ratio
title_short Effective Atomic Number Determination of Rare Earth Oxides with Scattering Intensity Ratio
title_sort effective atomic number determination of rare earth oxides with scattering intensity ratio
url http://dx.doi.org/10.1155/2013/738978
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